Podcasts about hydrostatic

Space Nuts Episode 496: Life on Other Planets, Centrifugal Forces, and Bone Density in SpaceJoin Andrew Dunkley and Professor Jonti Horner in this thought-provoking Q&A edition of Space Nuts, where they tackle some of the most intriguing questions from our listeners. From the possibility of detecting life on distant planets to the fascinating dynamics of centrifugal force, and the effects of zero gravity on bone density, this episode is brimming with scientific insights that will spark your curiosity about the universe.Episode Highlights:- Detecting Life on Distant Planets: Ron's compelling question leads the discussion on whether scientists in other solar systems could identify life on Earth using current technology, and vice versa. Jonti elaborates on the challenges and potential methods for detecting life beyond our planet.- Spheres vs. Disks: Dean asks why celestial objects form as spheres while others appear as disks. Jonti explains the physical processes at play, including hydrostatic equilibrium and angular momentum, shedding light on the fascinating shapes of stars, planets, and galaxies.- Bone Density in Space: Ann's insightful question about calcium loss in astronauts prompts a deep dive into the effects of microgravity on bone health. Jonti shares findings from recent studies and discusses the implications for long-term space missions.- Centrifugal Force Explained: Aussie Dean's inquiry about the nature of centrifugal force and its measurement leads to a discussion on reference frames and how they relate to our understanding of gravity and motion on Earth.For more Space Nuts, including our continually updating newsfeed and to listen to all our episodes, visit our website. Follow us on social media at SpaceNutsPod on Facebook, X, YouTube Music Music, Tumblr, Instagram, and TikTok. We love engaging with our community, so be sure to drop us a message or comment on your favorite platform.If you'd like to help support Space Nuts and join our growing family of insiders for commercial-free episodes and more, visit spacenutspodcast.com/aboutStay curious, keep looking up, and join us next time for more stellar insights and cosmic wonders. Until then, clear skies and happy stargazing.00:00 - Introduction to the episode and topics02:15 - Discussion on detecting life on other planets10:30 - Exploring the shapes of celestial objects18:00 - Insights into bone density loss in space26:45 - Understanding centrifugal force and reference frames30:00 - Closing thoughts and listener engagement✍️ Episode ReferencesNASA's Studies on Bone Densityhttps://www.nasa.gov/spaceflightHydrostatic Equilibrium in Celestial Bodieshttps://en.wikipedia.org/wiki/Hydrostatic_equilibriumCentrifugal Force and Gravityhttps://www.physicsclassroom.com/class/circles/Lesson-2/Centrifugal-ForceBecome a supporter of this podcast: https://www.spreaker.com/podcast/space-nuts-exploring-the-cosmos--2631155/support.

I veckans Hälsoveckan by Tyngre diskuterar Jacob och Erik först kort en artikel i SvD som fått en missvisande rubrik där det påstås att 47 studier visar vilken kost som motverkar inflammation, artikeln egentligen handlar om en översiktsartikel över översiktsartiklar på hur kosten påverkar IBD. Efter det blir det en lång genomgång av en bra artikel i tidskriften Nature Reviews Endocrinology som tittar på olika metoder att uppskatta fettmassa, förekomsten av fetma och kroppssammansättning i kliniskt arbete. Metoden går systematiskt igenom fördelar och nackdelar med 12 olika metoder. Från det mest enkla med BMI, midjemått och kaliper till avancerade och dyra metoder likt CT och MRI. På Hälsoveckan by Tyngres instagram kan du hitta bilder relaterat till detta och tidigare avsnitt. Hålltider (00:00:00) Introsnack (00:04:42) Kort om "maten som ger mindre inflammation" (00:14:12) Olika sätt att mäta fetma och uppskatta kroppsammansättningen (00:15:25) BMI - enkelt, smidigt och snabbt, men trubbigt (00:17:05) Vad är för mycket fett och varför är mycket fett ett problem? (00:18:51) Fettmassa har olika effekter beroende på var på kroppen de lagras (00:22:38) Midjemått eller midje-höft ratio (00:27:18) Kalipermått för att mäta underhudsfett (00:30:48) Bukhöjd, eller sagittal bukdiameter (00:35:00) Analys av foton eller kroppsscanning med ljus (00:39:28) Bod Pod (00:41:15) Hydrostatic densitometry (undervattensmätning) (00:43:14) Bio-impedansvåg - uppskattar kroppssammansättningen med ström (00:47:39) DEXA - scan av hela kroppen som ger dig en 2D bild (00:49:06) CT - mycket strålning men bra mätvärden (00:50:41) Magnetisk resonanstomografi aka magnetkameran (00:52:45) Vilken metod är att föredra? Spelar den extra precisionen någon praktisk roll?

Skeletons are on the menu today- and the different kinds organisms can have. Sources for this episode: Campbell, N. A., Urry, L. A., Cain, M. L., Wasserman, S. A., Minorsky, P. V. and Reece, J. B. (2018), Biology: a global approach, 11th edition (Global Edition), Harlow, Pearson Education Limited. Clennett, C., Locke, J. and Jackson, T. (editorial consultants) (2023), How Biology Works. LonondM Darling Kindersley Ltd. Hine, R. S. (2019), Oxford Dictionary of Biology (8th edition). Oxford: Oxford University Press. Schmidt-Nielsen, K. (1997), Animal Physiology: Adaptation and environment. Cambridge: Cambridge University Press.

Subscribe to my YouTube channel: http://bit.ly/RonSpomerOutdoorsSubscribe Welcome to the Ron Spomer Outdoors Podcast! In this episode, I answer listener questions about the 243 Winchester vs. the 6mm Remington, hydrostatic shock, and more! Links: Blog Post - https://www.ronspomeroutdoors.com/blog/flattest-shooting-rifle-cartridges-by-caliber Website: https://ronspomeroutdoors.com/ Facebook: https://www.facebook.com/ronspomeroutdoors Instagram: https://www.instagram.com/ronspomer/ Patreon: https://www.patreon.com/RonSpomerOutdoors Who is Ron Spomer For 44 years I've had the good fortune to photograph and write about my passion – the outdoor life. Wild creatures and wild places have always stirred me – from the first flushing pheasant that frightened me out of my socks in grandpa's cornfield to the last whitetail that dismissed me with a wag of its tail. In my attempts to connect with this natural wonder, to become an integral part of our ecosystem and capture a bit of its mystery, I've photographed, hiked, hunted, birded, and fished across much of this planet. I've seen the beauty that everyone should see, survived adventures that everyone should experience. I may not have climbed the highest mountains, canoed the wildest rivers, caught the largest fish or shot the biggest bucks, but I've tried. Perhaps you have, too. And that's the essential thing. Being out there, an active participant in our outdoor world. Produced by: Red 11 Media Disclaimer All loading, handloading, gunsmithing, shooting and associated activities and demonstrations depicted in our videos are conducted by trained, certified, professional gun handlers, instructors, and shooters for instructional and entertainment purposes only with emphasis on safety and responsible gun handling. Always check at least 3 industry handloading manuals for handloading data, 2 or 3 online ballistic calculators for ballistic data. Do not modify any cartridge or firearm beyond what the manufacturer recommends. Do not attempt to duplicate, mimic, or replicate anything you see in our videos. Firearms, ammunition, and constituent parts can be extremely dangerous if not used safely. Learn more about your ad choices. Visit megaphone.fm/adchoices

Struggling with the 'boring' yet vital concepts of oncotic and hydrostatic pressure in nursing school? Join Nicole from Your Nursing Tutor as she demystifies these crucial topics in the latest podcast episode. Perfect for both new and advanced nursing students, this podcast is a deep dive into the world of fluids and electrolytes, linking them with homeostasis for a comprehensive understanding. Whether you're juggling adult responsibilities or just starting out, this episode is tailored to make complex concepts approachable and relevant. Don't miss out on these insights to enhance your studies efficiently!

In this episode of Space Time, Stuart Gary discusses a mysterious neutron star named M82X2 that appears to be breaking the laws of physics by radiating energy that is 100 times brighter than it should be based on the Eddington limit.He also talks about lightning bolts creating a never-before-seen mineral and highlights a new hypothesis on how Saturn got its rings.[00:00:46] Ultra-luminous pulsar.[00:04:54] Never-before-seen mineral from lightning. [00:08:20] Saturn's Axial Tilt.[00:11:48] Saturn's Rings Formation.[00:17:22] Opioid-based drugs and cancer.[00:19:27] Amazon Forest Carbon Sink Threat.For more SpaceTime visit our website at https://www.spacetimewithstuartgary.com or our HQ at https://www.bitesz.comFollow us on twitter, Facebook, Instagram, TikTok and YouTube.#astronomy #space #science #news #podcast #spacetime

Summary: Caecilians are legless amphibians, so how do they get around? Join Kiersten as she talks about caecilian locomotion.   For my hearing impaired listeners, a complete transcript of this podcast follows the show notes on Podbean.   Show Notes: “The kinematics of locomotion in caecilians: effects of substrate and body shape” by Anthony Here et. al, J Exp Cool A Ecol Genet Physiol. 2010. Https//pubmed.ncbi.nlm.nih.gov   “A comparative study of locomotion in the caecilian Dermophis mexicanus and Typhlonectes natans (Amphibia: Gymnophiona)” by Adam P. Summers and James C. O'Reilly, Zoological  Journal of the Linnean Society, Vol 121, Issue 1, Sept 1997, pls 65-76. Https://doi.org/10.1111/j.1096-3642.1997.tb000147.x   Music written and performed by Katherine Camp   Transcript (Piano music plays) Kiersten - This is Ten Things I Like About…a ten minute, ten episode podcast about unknown or misunderstood wildlife. (Piano music stops) Welcome to Ten Things I Like About… I'm Kiersten, your host, and this is a podcast about misunderstood or unknown creatures in nature. Some we'll find right outside our doors and some are continents away but all are fascinating.  This podcast will focus ten, ten minute episodes on different animals and their amazing characteristics. Please join me on this extraordinary journey, you won't regret it. This episode continues caecilians and the fifth thing I like about these supercool amphibians is the way they get around.  In previous episodes, we have clearly established that caecilians do not have legs, so you may have been asking yourself, how do they get around? Excellent question. Let's get the answer. Caecilians are definitely not the only no-legged animal on planet Earth. There are snakes, glass lizards, and fish that do not have legs. Each of these examples have a unique way of locomotion. Caecilian locomotion is something that blows my mind!      In the last episode we learned that caecilians are divided into ten different families. Most of those families are terrestrial, which means, according to the Oxford Dictionary, of, on, or relating to the earth. Furthermore, many terrestrial caecilians, are fossorial which means they live underground. Nine of our ten families are considered terrestrial caecilians. So how exactly do caecilians create motion? They use hydrostatic movement. Hydrostatic motion is created when one set of muscles contracts in a circular and longitudinal pattern and another set of muscles stretches in response. Think of how a jellyfish moves. That in and out, almost like breathing, motion is how hydrostatic movement works. Many species of invertebrates use hydrostatic systems to move and several species of vertebrates use hydrostatic systems in specific body parts.  What makes caecilian hydrostatic locomotion unique is that they are the first known vertebrate to use their entire body as a hydrostatic system for locomotion. How could this get more interesting? I shall tell you! Hydrostatic movement generally depends on utilizing fluid filled portions of the body or vertebrae, but caecilians hydrostatic motion depends on a criss-cross array of tendons that surround their body cavity. Caecilians' skin and skeleton move independently of each other. Muscles do not attach the skin to the skeleton like other vertebrates. This allows them to create twice the maximum forward force of similar sized burrowing snakes that rely on longitudinal movement.  This is one more example of what makes caecilians so unique in the animal kingdom. Now that we know exactly how terrestrial caecilians create forward motion let's look at another characteristic that is influenced by their fossorial lifestyle. As you know, caecilians don't have feet, so instead their skull bones have adapted into the perfect shape to move through the soil. They're skulls are often described as wedge-shaped, compact, and robust. Sounds a lot like a shovel which would be perfect for digging through soil! Fossorial caecilians' skull bones have actually fused together in ways that other animals' skull bones are not fused. There are two types of skull structures in caecilians. The first type is zygokrotaphic in which the skull is perforated between the squamosal, or the side of the skull and the parietal, or the top of the skull. The second type of skull is stegokrotaphic which means the skull in completely roofed.  These two skull types are incredibly interesting to researchers and have inspired several scientific studies. One study investigated whether the amount of tunneling a species does determines which skull formation is found in their family. The thought was that the completely roofed skull formation would be  better suited to caecilians that burrow in soil more than other species that live mainly in leaf litter. To withstand the force needed to push through the soil a completely fused skull would be better, right?  What investigators found did not support this hypothesis. There was no evidence showing caecilians with stegokrotaphic skulls had increased burrowing activity. Skull shape may be more influenced by what they eat instead, we'll talk about this more in next week's episode. While investigating this hypothesis the researchers did discover that cranial shape varies greatly throughout caecilians. Even though there is variability in the position of the mouth, the temporal perforation of the skull, and the closure of the eye orbits, caecilian skulls are are generally bullet shaped which helps make burrowing much easier.  Scientists are always asking questions and a group of researchers studying caecilian movement wanted to know if the length of a caecilian impacted the way they moved. Using x-ray video these scientists recorded the movement of five different species of caecilian that ranged in size. What they discovered was that as the length of the caecilian increased their ability to create the internal concertina motion of hydrostatic movement decreased. As the caecilians increased in length they lost the skin and skeletal independent movement because of the increase in body length. The larger species depended more on lateral movement, even though they are still capable of concertina movement.  On an interesting note, in all species locomotion choice was dependent on substrate. When they were burrowing through soil they used a whole body or concertina motion to move forward; yet, when they were above the soil they used a lateral movement. This movement is similar to how snakes move in that side to side slithering motion. Family Typhlonectidae contains our aquatic caecilians. There are 13 species in this family and they all live their entire lives under the water. They also burrow into soil but since the substrate is underwater it's often more sandy or silty. Many species in this family have lost the concertina movement of terrestrial caecilians. Instead, they rely on a lateral motion to move through the water and soft substrate. That's it for caecilian locomotion, I hope you enjoyed this episode because it's my fifth favorite thing about this awesome animal. If you're enjoying this podcast please recommend me to friends and family and take a moment to give me a rating on whatever platform your listening. It will help me reach more listeners and give the animals I talk about an even better chance at change.    Join me next week for another thing I like about caecilians!   (Piano Music plays)  This has been an episode of Ten Things I like About with Kiersten and Company. Original music written and performed by Katherine Camp, piano extraordinaire.

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Hydrostatic Mass Profiles of Galaxy Clusters in the eROSITA Survey by Dominik Scheck et al. on Wednesday 23 November To assume hydrostatic equilibrium between the intracluster medium and the gravitational potential of galaxy clusters is an extensively used method to investigate their total masses. We want to test hydrostatic masses obtained with an observational code in the context of the SRG/eROSITA survey. We use the hydrostatic modeling code MBProj2 to fit surface-brightness profiles to simulated clusters with idealized properties as well as to a sample of 93 clusters taken from the Magneticum Pathfinder simulations. We investigate the latter under the assumption of idealized observational conditions and also for realistic eROSITA data quality. The comparison of the fitted cumulative total mass profiles and the true mass profiles provided by the simulations allows to gain knowledge about the reliability of our approach. Furthermore, we use the true profiles for gas density and pressure to compute hydrostatic mass profiles based on theory for every cluster. For an idealized cluster that was simulated to fulfill perfect hydrostatic equilibrium, we find that the cumulative total mass at the true $r_{500}$ and $r_{200}$ can be reproduced with deviations of less than 7%. For the clusters from the Magneticum Pathfinder simulations under idealized observational conditions, the median values of the fitted cumulative total masses at the true $r_{500}$ and $r_{200}$ are in agreement with our expectations, taking into account the hydrostatic mass bias. Nevertheless, we find a tendency towards a too high steepness of the cumulative total mass profiles in the outskirts. For realistic eROSITA data quality, this steepness problem intensifies for clusters with high redshifts and thus leads to too high cumulative total masses at $r_{200}$. For the hydrostatic masses based on the true profiles known from the simulations, we find a good agreement with our expectations concerning the hydrostatic mass. arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2211.12146v1

Active galactic nucleus jet feedback in hydrostatic halos by Rainer Weinberger et al. on Wednesday 23 November Feedback driven by jets from active galactic nuclei is believed to be responsible for reducing cooling flows in cool-core galaxy clusters. We use simulations to model feedback from hydrodynamic jets in isolated halos. While the jet propagation converges only after the diameter of the jet is well resolved, reliable predictions about the effects these jets have on the cooling time distribution function only require resolutions sufficient to keep the jet-inflated cavities stable. Comparing different model variations, as well as an independent jet model using a different hydrodynamics code, we show that the dominant uncertainties are the choices of jet properties within a given model. Independent of implementation, we find that light, thermal jets with low momentum flux tend to delay the onset of a cooling flow more efficiently on a $50$ Myr timescale than heavy, kinetic jets. The delay of the cooling flow originates from a displacement and boost in entropy of the central gas. If the jet luminosity depends on accretion rate, collimated, light, hydrodynamic jets are able to reduce cooling flows in halos, without a need for jet precession or wide opening angles. Comparing the jet feedback with a `kinetic wind' implementation shows that equal amounts of star formation rate reduction can be achieved by different interactions with the halo gas: the jet has a larger effect on the hot halo gas while leaving the denser, star forming phase in place, while the wind acts more locally on the star forming phase, which manifests itself in different time-variability properties. arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2211.11771v1

Active galactic nucleus jet feedback in hydrostatic halos by Rainer Weinberger et al. on Tuesday 22 November Feedback driven by jets from active galactic nuclei is believed to be responsible for reducing cooling flows in cool-core galaxy clusters. We use simulations to model feedback from hydrodynamic jets in isolated halos. While the jet propagation converges only after the diameter of the jet is well resolved, reliable predictions about the effects these jets have on the cooling time distribution function only require resolutions sufficient to keep the jet-inflated cavities stable. Comparing different model variations, as well as an independent jet model using a different hydrodynamics code, we show that the dominant uncertainties are the choices of jet properties within a given model. Independent of implementation, we find that light, thermal jets with low momentum flux tend to delay the onset of a cooling flow more efficiently on a $50$ Myr timescale than heavy, kinetic jets. The delay of the cooling flow originates from a displacement and boost in entropy of the central gas. If the jet luminosity depends on accretion rate, collimated, light, hydrodynamic jets are able to reduce cooling flows in halos, without a need for jet precession or wide opening angles. Comparing the jet feedback with a `kinetic wind' implementation shows that equal amounts of star formation rate reduction can be achieved by different interactions with the halo gas: the jet has a larger effect on the hot halo gas while leaving the denser, star forming phase in place, while the wind acts more locally on the star forming phase, which manifests itself in different time-variability properties. arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2211.11771v1

Hydrostatic Mass Profiles of Galaxy Clusters in the eROSITA Survey by Dominik Scheck et al. on Tuesday 22 November To assume hydrostatic equilibrium between the intracluster medium and the gravitational potential of galaxy clusters is an extensively used method to investigate their total masses. We want to test hydrostatic masses obtained with an observational code in the context of the SRG/eROSITA survey. We use the hydrostatic modeling code MBProj2 to fit surface-brightness profiles to simulated clusters with idealized properties as well as to a sample of 93 clusters taken from the Magneticum Pathfinder simulations. We investigate the latter under the assumption of idealized observational conditions and also for realistic eROSITA data quality. The comparison of the fitted cumulative total mass profiles and the true mass profiles provided by the simulations allows to gain knowledge about the reliability of our approach. Furthermore, we use the true profiles for gas density and pressure to compute hydrostatic mass profiles based on theory for every cluster. For an idealized cluster that was simulated to fulfill perfect hydrostatic equilibrium, we find that the cumulative total mass at the true $r_{500}$ and $r_{200}$ can be reproduced with deviations of less than 7%. For the clusters from the Magneticum Pathfinder simulations under idealized observational conditions, the median values of the fitted cumulative total masses at the true $r_{500}$ and $r_{200}$ are in agreement with our expectations, taking into account the hydrostatic mass bias. Nevertheless, we find a tendency towards a too high steepness of the cumulative total mass profiles in the outskirts. For realistic eROSITA data quality, this steepness problem intensifies for clusters with high redshifts and thus leads to too high cumulative total masses at $r_{200}$. For the hydrostatic masses based on the true profiles known from the simulations, we find a good agreement with our expectations concerning the hydrostatic mass. arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2211.12146v1

i cm z , a semi-analytic model for the thermodynamic properties in galaxy clusters: calibrations with mass and redshift, and implication for the hydrostatic bias by S. Ettori et al. on Monday 21 November In the self-similar scenario for galaxy cluster formation and evolution, the thermodynamic properties of the X-ray emitting plasma can be predicted in their dependencies on the halo mass and redshift only. However, several departures from this simple self-similar scenario have been observed. We show how our semi-analytic model $i(cm)z$, which modifies the self-similar predictions through two temperature-dependent quantities, the gas mass fraction $f_g=f_0 T^{f_1} E_z^{f_z}$ and the temperature variation $f_T=t_0 T^{t_1} E_z^{t_z}$, can be calibrated to incorporate the mass and redshift dependencies. We used a published set of 17 scaling relations to constrain the parameters of the model. We were subsequently able to make predictions as to the slope of any observed scaling relation within a few percent of the central value and about one $sigma$ of the nominal error. Contextually, the evolution of these scaling laws was also determined, with predictions within $1.5 sigma$ and within 10 percent of the observational constraints. Relying on this calibration, we have also evaluated the consistency of the predictions on the radial profiles with some observational datasets. For a sample of high-quality data (X-COP), we were able to constrain a further parameter of the model, the hydrostatic bias $b$. By calibrating the model, we have determined that (i) the slopes of the temperature dependence are $f_1=0.403 (pm0.009)$ and $t_1=0.144 (pm0.017)$; and that (ii) the dependence upon $E_z$ are constrained to be $f_z=-0.004 (pm 0.023)$ and $t_z=0.349 (pm 0.059)$. These values permit one to estimate directly how the normalizations of a given quantity $Q_{Delta}$ changes as a function of the mass (or temperature) and redshift halo in the form $Q_{Delta} sim M^{a_M} E_z^{a_z} sim T^{a_T} E_z^{a_{Tz}}$, in very good agreement with the current observational constraints. arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2211.03082v2

Mark talks with Tito Pacheco, the owner of the RIght Guyz Plumbing about "Hydrostatic Testing". Offering full-service sewer and drain repairs and replacements for either your home or your business. Host: Marc Ebinger Crükus Marketing Agency Guest: Tito Pacheco The Right Guyz Plumbing Service 210-744-4397

—- To Apply For Coaching: Click Here Download The Tailored Trainer: Tailored Trainer Sign Up Page To Get Your Questions Answered On The Podcast: Ask Us Here! Download 1 (or ALL) Of Our FREE GUIDES: https://www.tailoredcoachingmethod.com/guides Giant Lifting Equipment (10% Off With Code “TCM10”): GiantLifting.com 1st Phorm Supps: https://www.1stphorm.com/tailoredcoachingmethod To Get Cody’s Amazon Recommendations, Click Here —-- Timestamps: (4:30) - First, thanks for being so generous with your info! My question is this - I am planning to start a cut next week. I have my calories and macros figured out, I think. I have many instances in my past where I stupidly learned the hard way that my body falls apart when I am too low carb. (Lose my period, hormones tank, hypothyroidism, can't gain muscle, can't sleep etc etc) For the record, I am not underweight (and never was). Currently I am at maintenance: 2,400 cals a day, 170g protein, 80g fat, and 250g carbs. I light weights 4 times a week in a hypertrophy program, and get lots of steps and NEAT naturally. When I calculated my 12 week cut (with 3 weeks of diet breaks) I tried to keep my carbs as high as possible, but they obviously have to go down. I came up with: 1,900 cals a day, 160g protein, 46g fat, 185g carbs. I'm curious to get a second opinion about these numbers. Is 185 too high for carbs during a cut, or could I bump them up even more? I know it depends of course. I'm just terrified of having really bad biofeedback right away after making such huge health progress. I have about 15 lbs to lose, and might break it up to not stress my body out too much. I also don't want to be too much of a wuss, and screw it up by not going hard enough.Thanks so much!! (18:35) - I know I have asked this in the past, but will you have any mentorship opportunities coming within the next year? If not, where do you recommend I go to continue my education & just overall be a better coach? (29:40) - Hydrostatic body fat testing… is it accurate? (39:00) - Do you call your clients out on their excuses? —- Social Links: Blog – http://www.tailoredcoachingmethod.com/blog
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Link to bioRxiv paper: http://biorxiv.org/cgi/content/short/2022.11.15.516693v1?rss=1 Authors: Mochizuki, T., Tanigawa, T., Shindo, S., Suematsu, M., Oguchi, Y., Mioka, T., Kato, Y., Fujiyama, M., Hatano, E., Yamaguchi, M., Chibana, H., Abe, F. Abstract: The fungal cell wall is the first barrier against diverse external stresses, such as high hydrostatic pressure. This study explores the roles of osmoregulation and the cell wall integrity (CWI) pathway in response to the high pressure in the yeast Saccharomyces cerevisiae. We demonstrate the roles of the transmembrane mechanosensor Wsc1 and aquaglyceroporin Fps1 in an underlying protective mechanism to avoid cellular rupture under high pressure. The promotion of water influx into cells at 25 MPa, as evident by an increase in cell volume and a loss of the plasma membrane eisosome structure, promotes the activation of Wsc1, an activator of the CWI pathway. The downstream mitogen-activated protein kinase Slt2 was hyperphosphorylated at 25 MPa. Glycerol efflux increases via Fps1 phosphorylation, which is initiated by downstream components of the CWI pathway, and contributes to the reduction in intracellular osmolarity under high pressure. Herein, the elucidation of a cellular pathway that is used as a protective mechanism against high pressure could potentially be translated to mammalian cells and could help to understand cellular mechanosensation and adaptation. Copy rights belong to original authors. Visit the link for more info Podcast created by Paper Player, LLC

Multi-probe analysis of the galaxy cluster CL J1226 9+3332: Hydrostatic mass and hydrostatic-to-lensing bias by M. Muñoz-Echeverría et al. on Sunday 18 September The precise estimation of the mass of galaxy clusters is a major issue for cosmology. Large galaxy cluster surveys rely on scaling laws that relate cluster observables to their masses. From the high resolution observations of ~ 45 galaxy clusters with NIKA2 and XMM-Newton instruments, the NIKA2 SZ Large Program should provide an accurate scaling relation between the thermal Sunyaev-Zel'dovich effect and the hydrostatic mass. In this paper, we present an exhaustive analysis of the hydrostatic mass of the well known galaxy cluster CL J1226.9+3332, the highest-redshift cluster in the NIKA2 SZ Large Program at z = 0.89. We combine the NIKA2 observations with thermal Sunyaev-Zel'dovich data from NIKA, Bolocam and MUSTANG instruments and XMM-Newton X-ray observations and test the impact of the systematic effects on the mass reconstruction. We conclude that slight differences in the shape of the mass profile can be crucial when defining the integrated mass at R500, which demonstrates the importance of the modeling in the mass determination. We prove the robustness of our hydrostatic mass estimates by showing the agreement with all the results found in the literature. Another key information for cosmology is the bias of the masses estimated assuming hydrostatic equilibrium hypothesis. Based on the lensing convergence maps from the Cluster Lensing And Supernova survey with Hubble (CLASH) data, we obtain the lensing mass estimate for CL J1226.9+3332. From this we are able to measure the hydrostatic-to-lensing mass bias for this cluster, that spans from 1 - bHSE/lens ~ 0.7 to 1, presenting the impact of data-sets and mass reconstruction models on the bias. arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2209.07460v1

Multi-probe analysis of the galaxy cluster CL J1226 9+3332: Hydrostatic mass and hydrostatic-to-lensing bias by M. Muñoz-Echeverría et al. on Sunday 18 September The precise estimation of the mass of galaxy clusters is a major issue for cosmology. Large galaxy cluster surveys rely on scaling laws that relate cluster observables to their masses. From the high resolution observations of ~ 45 galaxy clusters with NIKA2 and XMM-Newton instruments, the NIKA2 SZ Large Program should provide an accurate scaling relation between the thermal Sunyaev-Zel'dovich effect and the hydrostatic mass. In this paper, we present an exhaustive analysis of the hydrostatic mass of the well known galaxy cluster CL J1226.9+3332, the highest-redshift cluster in the NIKA2 SZ Large Program at z = 0.89. We combine the NIKA2 observations with thermal Sunyaev-Zel'dovich data from NIKA, Bolocam and MUSTANG instruments and XMM-Newton X-ray observations and test the impact of the systematic effects on the mass reconstruction. We conclude that slight differences in the shape of the mass profile can be crucial when defining the integrated mass at R500, which demonstrates the importance of the modeling in the mass determination. We prove the robustness of our hydrostatic mass estimates by showing the agreement with all the results found in the literature. Another key information for cosmology is the bias of the masses estimated assuming hydrostatic equilibrium hypothesis. Based on the lensing convergence maps from the Cluster Lensing And Supernova survey with Hubble (CLASH) data, we obtain the lensing mass estimate for CL J1226.9+3332. From this we are able to measure the hydrostatic-to-lensing mass bias for this cluster, that spans from 1 - bHSE/lens ~ 0.7 to 1, presenting the impact of data-sets and mass reconstruction models on the bias. arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2209.07460v1

Rice Hydro Inc has released 3 previously unpublished facts about its A pump with pressure ranges up to 30,000 PSI and flow rates up to 56 GPM "Hydro Static Test Pump"

In this episode of the Epigenetics Podcast, we caught up with Sara Wickström, Director at the Max Planck Institute for Molecular Biomedicine in Münster, to talk about her work on the effect of mechanotransduction on chromatin structure and transcription in stem cells. Sara Wickström and her team focus on the stem cell niche and how that niche affects stem cell function. In order to study the native niche and to even be able to manipulate it, the Wickström Lab was able to develop a ex vivo culture system, allowing systematic identification of factors driving stem cell dynamics and plasticity. Stem cells in the stem cell niche are exposed to external stimuli such as physical forces which control their growth, fate and self renewal. Recent work in the Wickström lab showed how mechanical signals influence transcriptional regulation, chromatin organization, and nuclear architecture and how this affects aging or lineage commitment. In this Episode we also discuss how chromatin can act as a sensor of mechanical signals taking advantage of the different physical properties of eu- and heterochromatin.   References Le, H. Q., Ghatak, S., Yeung, C. Y., Tellkamp, F., Günschmann, C., Dieterich, C., Yeroslaviz, A., Habermann, B., Pombo, A., Niessen, C. M., & Wickström, S. A. (2016). Mechanical regulation of transcription controls Polycomb-mediated gene silencing during lineage commitment. Nature cell biology, 18(8), 864–875. https://doi.org/10.1038/ncb3387 Nava, M. M., Miroshnikova, Y. A., Biggs, L. C., Whitefield, D. B., Metge, F., Boucas, J., Vihinen, H., Jokitalo, E., Li, X., García Arcos, J. M., Hoffmann, B., Merkel, R., Niessen, C. M., Dahl, K. N., & Wickström, S. A. (2020). Heterochromatin-Driven Nuclear Softening Protects the Genome against Mechanical Stress-Induced Damage. Cell, 181(4), 800–817.e22. https://doi.org/10.1016/j.cell.2020.03.052 Koester, J., Miroshnikova, Y. A., Ghatak, S., Chacón-Martínez, C. A., Morgner, J., Li, X., Atanassov, I., Altmüller, J., Birk, D. E., Koch, M., Bloch, W., Bartusel, M., Niessen, C. M., Rada-Iglesias, A., & Wickström, S. A. (2021). Niche stiffening compromises hair follicle stem cell potential during ageing by reducing bivalent promoter accessibility. Nature cell biology, 23(7), 771–781. https://doi.org/10.1038/s41556-021-00705-x Maki, K., Nava, M. M., Villeneuve, C., Chang, M., Furukawa, K. S., Ushida, T., & Wickström, S. A. (2021). Hydrostatic pressure prevents chondrocyte differentiation through heterochromatin remodeling. Journal of cell science, 134(2), jcs247643. https://doi.org/10.1242/jcs.247643   Related Episodes Nutriepigenetics: The Effects of Diet on Behavior (Monica Dus) Epigenetic Regulation of Stem Cell Self-Renewal and Differentiation (Peggy Goodell) The Effect of Vitamin D on the Epigenome (Folami Ideraabdullah)   Contact Active Motif on Twitter Epigenetics Podcast on Twitter Active Motif on LinkedIn Active Motif on Facebook Email: podcast@activemotif.com

Osmosis, osmolality, osmolarity, and fluid balance. How hydrostatic pressure and osmotic pressure drive filtration in our capillaries to deliver nutrients and remove wastes. 

Stanislav Molchanov; University of North Carolina 12 June 2007 – 14:30 to 15:30

Photo: The fabled mower to challenge your Corvette. . @Batchelorshow #PacificWatch: CancellingBig Mow 31-HP V-twin Dual Hydrostatic 66-in Zero-turn Lawn Mower.  @JCBliss #FriendsofHistoryDebatingSociety https://www.lowes.com/pd/Swisher-Big-Mow-31-HP-V-twin-Dual-Hydrostatic-66-in-Zero-turn-Lawn-Mower-with-Mulching-Capability/1000181497

In today's short podcast, Bryan explores the dangers of cold tanks during refrigerant recovery.   Whenever you have a recovery tank, you only want to fill it to 80% capacity in the liquid state. The same goes for all sorts of vessels (coils, etc.).    However, capacity isn't the only factor to consider for safety. We need to know what our maximum temperature will be. You will be in greater danger of overfilling a tank when it is cold because higher temperatures increase the pressure. High pressure in a closed space may lead to explosions. When you fill a tank to 80% under cold conditions, normal temperature conditions could put you in the danger zone (let alone temperatures above 100°F).   So, it's better to determine your tank fill based on densities at the MAXIMUM temperatures you will encounter, NOT for the measurements at artificial cooling conditions (such as when you put the tank in ice water during recovery).   In the end, just be careful when you're recovering into a cold tank or using tanks when it's cold outside. That will help you avoid hydrostatic pressure buildup and explosions.   Bryan covers:   The 80% capacity rule for filling vessels with liquid Why the 80% capacity rule varies by temperature Temperature, pressure, and density Hydrostatic pressure AHRI's 77°F guideline Ice buckets for recovery What to do if a tank vents its refrigerant on you while driving If you have an iPhone, subscribe to the podcast HERE, and if you have an Android phone, subscribe HERE.

Linda Finley is the owner and operator of Body Fat Test. A growing line of body composition testing trucks bringing hydrostatic weighing to the general public. Hydrostatic weighing is considered the “Gold Standard” in body composition analysis, and I 100% agree. In this episode I had the pleasure of chatting with Linda about the origin of hydrostatic weighing and its necessity in every fitness plan regardless of age, gender and race. The is the episode that can unlock the answers to every choice you make when it comes down to what you eat, how you train your body in the gym and even the choices you make at times of extreme stress and depression. The latter is the most relevant to the state of our nation today. Pandemic fatigue is real. I believe the first step to taking advantage of a bit more time on your hands now, is to, once and for all, put a better effort in understanding the scientific side of our minds and bodies; as it relates to our future function. I hope you enjoy this as much as I did, so without further ado… Here's, What's What With Linda Finley. (currently covering the bay area, between Bakersfield to north of the I-10, the inland border to the coast, OC, San Diego.) Company Details: Body Fat Test : Linda Finley Owner/ Operator at  Body Fat Test  PO Box 3361 Camarillo CA 93011 P (805) 205-5356  E Linda@BodyFatTest.com  W www.BodyFatTestCA.com

Jack Walker and Paul Atzemis discuss the science of hydrostatic pressure and how it relates to high-performance coating systems. They also compare moisture vapor transmission to hydrostatic pressure. 0:00 – Intro 0:32 – Hydrostatic pressure versus moisture vapor transmission 1:42 – The definition of hydrostatic pressure 2:36 – Areas where hydrostatic pressure and moisture vapor transmission are of concern 3:24 – Specialty coatings required for hydrostatic pressure and coatings for moisture vapor transmission 5:21 – A real-world example of hydrostatic pressure 8:37 – Review of hydrostatic pressure properties 10:12 – Wrap up Subscribe via iTunes, Google Play, or Spotify. Find out more at https://carboline-tech-service-podcast.pinecast.co

Jon Frey is the Head of Engineering Systems and Solutions at Bosch Rexroth. In that role, he leads a team focused on developing unique solutions to complex problems, with an eye towards the creation of new products that support all of Rexroth’s business units. We invited him into our forum to learn more about one of those solutions – hydrostatic gear drives and their growing role in powering hydraulic work functions. Contact Jon via email: Jon.Frey@boschrexroth-us.com Connect with the host Eric Lanke at elanke@nfpa.com or on Twitter @ericlanke

What is the hydrostatic test and does my house need it? In this episode, we dive deep into the city sewer and unclog this history of waste pipes and the modern problems they pose. 

Originally released in Episode 21Your browser does not support this audio Direct link: http://dl.hydrostaticpodcast.com/kyla/HKYLA_019_Quafe.mp3Links and Resourceshttps://wiki.eveonline.com/en/wiki/Quafe_(Chronicle)https://wiki.eveonline.com/en/wiki/Quafe_Company_(NPC_corporation)https://wiki.eveonline.com/en/wiki/Poire_Viladillethttps://wiki.eveonline.com/en/wiki/Lost_Stars_(Chronicle)https://wiki.eveonline.com/en/wiki/Lost_Stars,_Inc.A capsuleer suggests reviving Quafe+ with artificial biomassAbout Hydrostatic's Know Your Lore ArchivesThe Archives are re-releases of just the Know Your Lore segment of the larger podcast, and are released between normal episodes.

Originally released in Episode 18Your browser does not support this audio Direct link: http://dl.hydrostaticpodcast.com/kyla/HKYLA_016_Maleatu_Shakor.mp3Links and Resourceshttps://wiki.eveonline.com/en/wiki/Brutorhttps://wiki.eveonline.com/en/wiki/Maleatu_Shakorhttps://wiki.eveonline.com/en/wiki/Maleatu_Shakor_(Chronicle)About Hydrostatic's Know Your Lore ArchivesThe Archives are re-releases of just the Know Your Lore segment of the larger podcast, and are released between normal episodes.

Originally released in Episode 16Your browser does not support this audio Direct link: http://dl.hydrostaticpodcast.com/kyla/HKYLA_015_Black_Eagles.mp3Links and Resourceshttps://wiki.eveonline.com/en/wiki/Mentas_Blaquehttps://wiki.eveonline.com/en/wiki/Black_EaglesTwo Deaths, as read by Zendane of Eve Readerhttps://wiki.eveonline.com/en/wiki/The_Paths_They_Chose_(Chronicle)https://wiki.eveonline.com/en/wiki/Taught_Thoughts_(Chronicle)About Hydrostatic's Know Your Lore ArchivesThe Archives are re-releases of just the Know Your Lore segment of the larger podcast, and are released between normal episodes.

Originally released in Episode 15Your browser does not support this audio Direct link: http://dl.hydrostaticpodcast.com/kyla/HKYLA_014_Sisters_of_Eve.mp3Links and ResourcesNPC corporations in the SOEAnte, the chronicle where Santimona Sarpati isn't quite as hostile with Silphy en Diabel as she should beAbout Hydrostatic's Know Your Lore ArchivesThe Archives are re-releases of just the Know Your Lore segment of the larger podcast, and are released between normal episodes.

Originally released in Episode 11Your browser does not support this audio Direct link: http://dl.hydrostaticpodcast.com/kyla/HKYLA_011_Jamyl.mp3Links and ResourcesThe current Empress: https://wiki.eveonline.com/en/wiki/Jamyl_IThe second-most-recent Amarr Emperor: https://wiki.eveonline.com/en/wiki/Doriam_Kor-AzorThe third-most-recent Amarr Emperor: https://wiki.eveonline.com/en/wiki/Heideran_VIIShathol'Syn, the ritual suicide committed by any heir who doesn't become emperor: https://wiki.eveonline.com/en/wiki/Shathol%27SynVideos and narrative of the Amarr Championship to determine Heideran's successor, and in which Jamyl commits suicide: https://wiki.eveonline.com/en/wiki/Amarr_ChampionshipKirith writes about the Golden and Silver magnates given as prizes during the championship: http://www.ninveah.com/2010/06/unique-ships-amarr-magnate-frigates.htmlVideo of Jamyl I's coronation: About Hydrostatic's Know Your Lore ArchivesThe Archives are re-releases of just the Know Your Lore segment of the larger podcast, and are released between normal episodes.

Originally released in Episode 23Your browser does not support this audio Direct link: http://dl.hydrostaticpodcast.com/kyla/HKYLA_021_Mindclash.mp3Links and Resourceshttps://wiki.eveonline.com/en/wiki/Mind_Clashhttps://wiki.eveonline.com/en/wiki/Mind_Clash_(Chronicle)The latest Lore Panel where Aedre Lafisques talked about MindclashAbout Hydrostatic's Know Your Lore ArchivesThe Archives are re-releases of just the Know Your Lore segment of the larger podcast, and are released between normal episodes.

Originally released in Episode 19Your browser does not support this audio Direct link: http://dl.hydrostaticpodcast.com/kyla/HKYLA_017_Karin_Midular.mp3Links and Resourceshttps://wiki.eveonline.com/en/wiki/Karin_MidularHow Karin got her tattooThe Voluval, the ceremony in which most Minmatar get a special tattooAbout Hydrostatic's Know Your Lore ArchivesThe Archives are re-releases of just the Know Your Lore segment of the larger podcast, and are released between normal episodes.

Originally released in Episode 22Your browser does not support this audio Direct link: http://dl.hydrostaticpodcast.com/kyla/HKYLA_020_Speakers_of_Truth.mp3Links and Resourceshttps://wiki.eveonline.com/en/wiki/Speakers_of_Truthhttps://wiki.eveonline.com/en/wiki/The_Speakers_of_Truth_(Chronicle)https://wiki.eveonline.com/en/wiki/The_Speaker_of_Truths_(Chronicle)About Hydrostatic's Know Your Lore ArchivesThe Archives are re-releases of just the Know Your Lore segment of the larger podcast, and are released between normal episodes.

Originally released in Episode 14Your browser does not support this audio Direct link: http://dl.hydrostaticpodcast.com/kyla/HKYLA_013_Concord.mp3Links and Resourceshttp://eve.wikia.com/wiki/CONCORD_Assemblyhttps://wiki.eveonline.com/en/wiki/Aidonis_Elabonhttps://wiki.eveonline.com/en/wiki/Heideran_Gets_the_Aidonis_(Chronicle)https://wiki.eveonline.com/en/wiki/Aidonis_StatueAbout Hydrostatic's Know Your Lore ArchivesThe Archives are re-releases of just the Know Your Lore segment of the larger podcast, and are released between normal episodes.

Originally released in Episode 13Your browser does not support this audio Direct link: http://dl.hydrostaticpodcast.com/kyla/HKYLA_012_Blood_Raiders.mp3Links and Resourceshttps://wiki.eveonline.com/en/wiki/Category:The_Blood_Raider_Covenant_ChroniclesOur discussion on the Seyllin incident (in which the Blood Raiders played an important part) starts at about 51 minutes into Hydrostatic Episode 9About Hydrostatic's Know Your Lore ArchivesThe Archives are re-releases of just the Know Your Lore segment of the larger podcast, and are released between normal episodes.

Originally released in Episode 20Your browser does not support this audio Direct link: http://dl.hydrostaticpodcast.com/kyla/HKYLA_018_Serpentis.mp3Links and Resourceshttps://wiki.eveonline.com/en/wiki/Serpentishttps://wiki.eveonline.com/en/wiki/Salvador_Sarpatihttps://wiki.eveonline.com/en/wiki/Guardian_Angelshttps://wiki.eveonline.com/en/wiki/The_Sarpati_Family_(Chronicle)https://wiki.eveonline.com/en/wiki/SoltueurAbout Hydrostatic's Know Your Lore ArchivesThe Archives are re-releases of just the Know Your Lore segment of the larger podcast, and are released between normal episodes.

Jack Walker and Paul Atzemis feel the pressure. This week the guys discuss Hydrostatic Pressure and its effects on coatings.

Watch Henry’s MinutePhysics video: https://www.youtube.com/watch?v=NucdlR9EGbA MinuteEarth & MinutePhysics are on Patreon: http://www.patreon.com/minuteearth & http://www.patreon.com/minutephysics It’s becoming harder and harder to categorize moons as moons. ___________________________________________ To learn more, start your googling with these keywords: Moon: a natural satellite of a satellite of a star. Satellite: A celestial body orbiting a larger celestial body. Orbit: The path followed by one object revolving around another object under the influence of gravity. Barycenter: The center of mass that two or more bodies orbit around. Binary System: A system in which two similarly sized object orbit the same barycenter. Hydrostatic equilibrium: Roundness that occurs when gravity is balanced by a pressure gradient force. ___________________________________________ If you liked this week’s video, you might also like: That’s no moon … it’s a space station! https://www.youtube.com/watch?v=JGp_5gOww0E. And here's a tidy illustrated difference between geocentrism and heliocentrism: http://www.malinc.se/math/trigonometry/geocentrismen.php _________________________________________ Subscribe to MinuteEarth on YouTube: http://goo.gl/EpIDGd Support us on Patreon: https://goo.gl/ZVgLQZ And visit our website: https://www.minuteearth.com/ Say hello on Facebook: http://goo.gl/FpAvo6 And Twitter: http://goo.gl/Y1aWVC And download our videos on itunes: https://goo.gl/sfwS6n ___________________________________________ Credits (and Twitter handles): Script Writer: David Goldenberg (@dgoldenberg) Script Editor: Henry Reich (@MinutePhysics) Video Illustrator: Ever Salazar (@eversalazar) Video Director: Henry Reich (@MinutePhysics) Video Narrator: Kate Yoshida (@KateYoshida) With Contributions From: Alex Reich, Emily Elert, Peter Reich Music by: Nathaniel Schroeder: http://www.soundcloud.com/drschroeder ___________________________________________ References: Norton, J. (2008) Could a moon have moons? Popular Science. Retrieved from: http://www.popsci.com/scitech/article/2008-04/could-moon-have-moons H. A. Weaver, S. A. Stern, M. J. Mutchler, A. J. Steffl, M. W. Buie, W. J. Merline, J. R. Spencer, E. F. Young, L. A. Young (2006). The Discovery of Two New Satellites of Pluto. Nature. 439: 943-945. Retrieved from: http://www.nature.com/nature/journal/v439/n7079/abs/nature04547.html?foxtrotcallback=true Tiscareno, M., Burns, J., Sremcevi, M., Beurle, K., Hedman, M. Copper, N., Milano, A., Evans, M., Porco, C., Spitale, J., and WEiss, J. (2010) Physical Characteristics And Non-Keplerian Orbital Motion Of “Propeller” Moons Embedded In Saturn’s Rings. The Astrophysical Journal Letters, 718: 92-96. Retrieved from: http://iopscience.iop.org/article/10.1088/2041-8205/718/2/L92 Spahn, F., and Schmidt, J. (2006) Saturn’s Bared Mini-Moons. Nature, 440: 30-31. Retrieved from: https://www.nature.com/nature/journal/v440/n7084/full/440614a.html

Give this episode a download! If you like what you hear don’t forget to subscribe and leave us a 5 star review For Video Content Subscribe on Youtube: www.youtube.com/abfitnesstrainer —————————————————- Stay Connected to New York Muscle Radio Like our Facebook Page: www.facebook.com/newyorkmuscleradio  Follow us on Instagram Anthony @abfitness Pete @jakkedfitness Take yourself to the next level with our Online Coaching Program visit: NewYorkMuscleRadio.com ————————————————— Intro Topics ------------------------- Quote of the Day ------------------------- Trending Fitness Topic New Muscle in quad —————————————— Listener Question of the Day  If you have a question you would like us to answer for you submit it on our website: www.newyorkmuscleradio.com/listenerquestion Call Your Question in: 508- 687-2534 Question –  ANDREW bUSH Hey, dudes. Great podcast. Just wondering if you ever heard of anyone puting swimming as part of their cardio. It seems like people always run or cycle or mayyyybe do kickboxing but I've never heard of anyone adding swimming. It seems like it'd be the most complete cardio one could do. Is it just a timing thing? Does getting ready for the pool after a workout and then showering before and after you get out of the pool just add too much time to the workout? Anyway, personally, I try to add swimming to my workout when possible. Thanks. Daria Hi guys! I'm sending this message all the way from San Francisco, CA. It has taken me forever to find a fitness podcast that is super informative without all the fluff and science jargon. NYMR is entertaining and very relatable. I listen to your podcast religiously and I'm not even religious! Anyway, I have a diet and fitness related question: 1.) I'm am a 35 year old female standing at 5'9" weighing at 142lbs w/ 14% body fat (via Hydrostatic). My ultimate goal is to be super lean. Although 14% BF is relatively low, I would like to be more shredded/cut. Based on my Hydrostatic test, I currently burn 1730 calories resting. Listening to your podcast, I know that I should be at a deficit if I want to lose more fat or get shredded. How much of a deficit is ideal? I'm currently averaging a 150-300 calorie deficit. 2.) My main form of fitness is Crossfit (which includes conditioning and strength training i.e. deadlift, squatting, cleans, snatching) but I also lift weights at your old regular gym (aka bro gym'ing) 1-2x/week. I understand that cardio is not the most ideal for muscle gain/fat loss, but HIIT is acceptable. How is Crossfit and HIIT different? And does Crossfit affect my goal to shred/cut? Crossfit makes me strong and I LOVE how it makes me feel after a workout. But if I'm being honest, I want to look good, too. What is the happy medium? Thanks guys! Looking forward to trying your coffein + BCAA! Taria (pronounced like Daria the cartoon) ——————————————— Podcast Topic  Today we have on a special guest Paul Revelia from Pro Physiques. Paul is someone I met on bodybuilding.com boards years ago and I have watched paul just get better with age, both in the gym and in business. Paul is one of the top online coaches and works with hundreds of people. Paul its an honor to have you on the show! Welcome to the NYMR podcast Paul for those that may not know you, tell us alittle bit about yourself, talk about your beginnings to where you are now? What are some of the trials and tribulations of your journey? Have you had any major setbacks and how did you overcome them? Whats a good layne story What does the future look like for you?  Ending Ok guys don’t forget to share this episode with all your friends

Your browser does not support this audio The editors apologize for how late this was posted into the podcast feedDirect link: http://dl.hydrostaticpodcast.com/Ascension_Lore_Panel.mp3An overview of the latest lore from AscensionLinks and ResourcesEmergent ThreatsHilen Tukoss BroadcastEmpress Jamyl's coronationFor mor on the lore, read Ash's lore primer or Mark726's Lore Survival Guide

Your browser does not support this audio Direct link: http://dl.hydrostaticpodcast.com/loreupdate/loreupdateyc118_9.mp3Hydrostatics Lore Update on the Corination, Purity of the Thrones, and Crimson HarvestAsh's note: Unfortunately some technical difficulties caused some audio distortion, and significantly delayed the release. I have learned quite a bit about editing, so hopefully can avoid this in the future.PanelistsAlizabeth Morwen LagannAshterothiLinks and ResourcesPurity of the Throne IMPERIAL GUARD TOUR DAM-TORSAD AHEAD OF CORONATIONIMPERIAL GUARD CONFIRMS RUMORS OF THWARTED ATTACK IN THRONE WORLDSAMARR THIRD FLEET ADMIRAL SPEAKS OUT ON ‘PURITY OF THE THRONECoronation Event September 27thCrimson HarvestThe EVE Lore PrimerSOMETHING IS ROTTEN IN THE STATE OF AMARRTHE IMPERIAL SUCCESSION TRIALS: WHAT IF?Music is Freedom At Last, by CCP Games

Your browser does not support this audio Updated with fixed audio!Direct link: http://dl.hydrostaticpodcast.com/fanfestsurvival.mp3A special Fanfest 2016 Survival episode with Ash, Phy, and LyseLinks and ResourcesSchedualDev BlogLive StreamSuccession Trials: What If

After just reviewing how you can calculate your BMI (Body Mass Index) and whether it even matters or not, we're going to now just answer your #WeightLossWednesday questions! Ginny: Should I workout even if I'm tired? Max: Can I do hydrostatic underwater body composition testing? Wanda: Will not eating dinner slow my metabolism? Get all these questions and more on today's Cabral House Call! - - -  

Updated with audio and video of the panel!Our Eighth Lore Panel on the latest lore events including:Drifters The SoCT, CONCORD, and UpwellWhat are the SoE up to?Watch and Listen On DemandYour browser does not support this audio Direct link: http://dl.hydrostaticpodcast.com/Upwell_Lore_Panel.mp3Watch our Twitter, and subscribe to our Twitch channel to be the first to know about upcoming panels and episodes!

Your browser does not support this audio Direct link: http://dl.hydrostaticpodcast.com/loreupdate/Lore_Update_003.mp3A special Lore Update all about EVE Valkyrie.PanelistsMakoto PrianoMorwen LagannMark726Links and ResourcesShiny Lore Tidbits: http://puu.sh/nGw7f/541b66a1f9.jpgThe Guristas assault Vellaine III https://community.eveonline.com/news/news-channels/world-news/guristas-assault-vellaine-iii-abscond-with-ground-combatants/Fatal's back! https://community.eveonline.com/news/news-channels/world-news/guristas-pirates-in-disarray-as-they-seek-to-offload-scientists/Valkyrie Gameplay Trailer: https://www.youtube.com/watch?v=3SI1CB4rcf8CGP Grey explains Transporters: https://www.youtube.com/watch?v=nQHBAdShgYIHardcore vs. Softcore playing: https://www.youtube.com/watch?v=Ho-yOSgJd48Music is from the Frostline Release, by CCP Games

You didn't want to read last episode's mailbag again, did you?Recorded March 16th, 2016Your browser does not support this audio Direct link http://dl.hydrostaticpodcast.com/HP_27_The_Powerhouse_of_the_Cell.mp3IntroductionWe welcome HPA_Dichroic and Yadaryon to the show!Question for the PanelWhat would you most like to change about Project Discovery in the future?Phyridean's Pub QuizLast Episode's question: A certain Gallente songwriter once wrote a song about his lost love. Name the artist.Answer: Jaroud Dertier (check the show info for Azure Plagioclase)Thanks to Meliannah for this question.Congratulations to MinisculeMinja Barviainen for being our random winner of 4000 Aurum! (And honorable mention to Ibrahim Tash-Murkon, the only other listener to get the question, even though we gave everybody five months to answer.)No new question for this episodeMailbag, Corrections, and UpdatesNew Patrons: Alan Shroue, Angel Penshar (who compares us favorably to piss!), Degestus Chene, Yuriegh(Yur-ig) Orindril(Orin-drill), Benji, Ibrahim Tash-Murkon, and El'Basin, who upped his gift for the holiday seasonJames Sylvestre's list of collective nouns:Uprising of MinmatarCongregation of AmarrHustings of GallentePantheon of JoveOrgy of Blood RaidersShamble of SanshaBand of GuristasExplosion of Rogue Drones (Assembly?)Murmur of Sisters of EveGang of SerpentisKnuckle of Shadow CartelMechanics DrilldownProject Discoveryhttp://www.proteinatlas.org/http://mmos.ch/Know Your LoreSpecial guest Rhavas gives us the lowdown on Inheritancehttps://community.eveonline.com/backstory/chronicles/inheritance/From Rhavas's blog:https://interstellarprivateer.wordpress.com/2016/01/02/the-revelations-of-delegate-zero/https://interstellarprivateer.wordpress.com/2016/01/15/carolines-star-4-kardashevs-children/Closing ThoughtsDichroic shouts out his scientist friends at HPA, Atilla at MMOS, and the team at CCPYadaryon shouts out CCP Wonderboy, and suggests that CCP hire him full timeLocke creatively gives a shoutout to the guests and all of Project DicsoveryPhy gives a shoutout to the Tweetfleet Slack Moderation team member SibsRate us on iTunes and Stitcher radioSend Feedback to hydrostaticeve@gmail.comOr check out our other projectsMusicIntroduction, transition, and closing music "In the Magnificent Realm" by CCP Games

Your browser does not support this audio Direct link: http://dl.hydrostaticpodcast.com/loreupdate/Lore_Update_002.mp3PanelistsMakoto PrianoMorwen LagannLinks and ResourcesList of Christmas gifts: https://www.reddit.com/r/Eve/comments/3tglwc/does_feawen_like_this/cx62137?context=10000Serpentis strike back:The Inheritance: http://community.eveonline.com/backstory/chronicles/inheritanceMerry Christmas from all of us at Hydrostatic!About Hydrostatic's Lore UpdateThe Lore Update is a regular update of the lore with a subset of our excellent lore panelists.Music is fron the Frostline Release, by CCP Games

Updated with audio and video of the panel!The hosts of Hydrostatic Podcast invite you to join our panelists, on our Twitch channel at http://twitch.tv/HydrostaticEVE3pm EST, Sunday, December 13th(20:00 Sunday, December 13th Eve time)For our Seventh Lore Panel on the latest lore events including:Operation FrostlineNew ChroniclesThe Amarr SuccessionUpwell ConsortiumThe Space Urchin/Pickup SticksWatch and Listen On DemandYour browser does not support this audio Direct link: http://dl.hydrostaticpodcast.com/Frostline_Lore_Panel.mp3Watch our Twitter, and subscribe to our Twitch channel to be the first to know about upcoming panels and episodes!

Your browser does not support this audio The editors apologize for substantial date confusion. We're a little tired.Direct link: http://dl.hydrostaticpodcast.com/loreupdate/Lore_Update_001.mp3PanelistsAedre LafisquesMorwen LagannAlizabethLinks and ResourcesOperation FrostlineFalcon's Cloning Description on RedditOuside the Wire - By AlizabethAbout Hydrostatic's Lore UpdateThe Lore Update is a regular update of the lore with a subset of our excellent lore panelists.

On Episode 176 of Trick or Treat Radio we settle into our second week in the brand new Castle Wolfenstein! We are joined by our good buddy and honorary Deadite, Teeel frontman Jim Smith to review the 80s slasher homage flick, The Final Girls! We also discuss songwriting, album construction, we play YOUR voicemails and we even leave time for a Double Tap! So grab your tinfoil hat, your pyramid schematics and strap on! Topics discussed: Tiny's Synth room meme, The Wiz, iheartsynths.com, Patreon projects, the Great Gazoo, Teeel, Ryan Gosling, Elm St. Kids Movie Club, Derek Rook, Workaholics, man crushes, characters in slasher films, Looks that Kill, Warrant’s Cherry Pie, Malin Akerman, Unchayned with the Chayn Gang, Thai Day of the Dead poster, Transformers, Loopmasters, Weehawken New Jersey, The Final Girls, Dynamo film commentary, University Heights, ginormous raffle, The Last Action Hero, Tiny’s graphic tees, Cub, The Final Girl, The Carrie Diaries, Chloe Bridges, who built the pyramids, Narcos, Television Crossover Universe Podcast, Gloryhammer, the construction of the Hydrostatic vinyl, Krampus, putting together a fluid album, Mondo Releasing, Simon R Green, Han Solo, importance of nudity, X-Files, Dark Tower casting, Black Christmas remake, Gilmore Girls, Adam Devine, the stuff that makes it from script to screen, favorite holiday movies, Dark Star, putting together a great set list, PG-13, Good Movies for Bad People.Support the show (https://www.patreon.com/trickortreatradio)

Suck in your gut, grab all your gold, and head down to the musty basement where Christy, Meredith, and Mike fire up the Andyman Grill to roast last week's TBTL Please bring an armload of towels and wear a tuxedo. Even though it's obvious to everyone you do not want to wear a tuxedo.

Suck in your gut, grab all your gold, and head down to the musty basement where Christy, Meredith, and Mike fire up the Andyman Grill to roast last week's TBTL Please bring an armload of towels and wear a tuxedo. Even though it's obvious to everyone you do not want to wear a tuxedo.

Updated link to the timeline of New EdenRecorded November 10th, 2015Your browser does not support this audio Direct link: http://dl.hydrostaticpodcast.com/HP_26_Netflix_and_Chill_in_Nullsec.mp3IntroductionWe welcome Elise Randolph of Pandemic Legion to the show!Question for the PanelWhich feature do you want to see as the main focus for the expansion after Citadels?Phyridean's Pub QuizLast Episode's question: How long did the fires of Malkalen burn?Answer: 6 years, 19 days (2210 days, from Thursday, May 15th YC110/2008 to Tuesday, June 3rd YC116/2014)Thanks to Kamar Raimo for this question.Congratulations to Yanarfal, Ibrahim Tash-Murkon, and Rex Findley (who got the exact answer) for being our random winners of 1965 Aurum!This Episode's question: A certain Gallente songwriter once wrote a song about his lost love. Name the artist.(Thanks to Meliannah for suggesting this question!)One person who gets the correct answer will be drawn at random, and will receive any combination of NES store items worth 4000 AURMailbag, Corrections, and UpdatesNew Patrons: Mason, Abel Modeste, Wolf HeikuraWorking on getting out stickers to those who requested themAlexandr Ivanovic on slack has created a timeline of New Eden Update: Alexandr is now also working with Saftsuze hereRocketX Capital Balance ReportAsh's new favorite FCing tool, Inf[l]ight by ZeitonautMechanics DrilldownResistancesEve University on Natural Resistances: http://wiki.eveuniversity.org/Natural_ResistancesNPC Damage Types cheat sheet: http://i.imgur.com/xOMYf1L.png0Eve University on Stacking Penalties: http://wiki.eveuniversity.org/Stacking_penalties Emergent GameplayPandemic LegionKnow Your LoreThe Order of St. Tetrimonhttps://wiki.eveonline.com/en/wiki/The_Cult_of_Tetrimon_(Chronicle)http://community.eveonline.com/backstory/chronicles/testament/Closing ThoughtsLocke points us to his interview with DelonewolfPhy gives a shoutout to Matterall, who has moved to themittani.comPhy's Amarr Championships teammates, Uriel Paradisi, Gorski Car, and Ferox, are awesomeElise gives a shoutout to the Amarr Championships teams and to CCP for the new formatRate us on iTunes and Stitcher radioSend Feedback to hydrostaticeve@gmail.comOr check out our other projectsMusicIntroduction, transition, and closing music from the Parallax release by CCP Games

Originally released in Episode 10Your browser does not support this audio Direct link: http://dl.hydrostaticpodcast.com/kyla/HKYLA_010_Crielere.mp3Links and ResourcesAll 16 chapters of the Crielere project chroniclesThe very light summary of the eventsEve Travel article on the research station. (Locke said "they should both be functional stations, last I checked" so he probably last checked sometime in 2010.)Thanks to Kirith Kodachi for pointing out to me that the Capsuleer defense of Crielere was in fact an ingame event.About Hydrostatic's Know Your Lore ArchivesThe Archives are re-releases of just the Know Your Lore segment of the larger podcast, and are released between normal episodes.

Recorded October 25th, 2015Your browser does not support this audio Direct link: http://dl.hydrostaticpodcast.com/HP_25a_Eve_Vegas_2015.mp3IntroductionWe're recording from Eve Vegas Sunday morning, and we've brought on Blake of K162space.com, Mark726/Webspaceships of the Eve Travel blog, and Makoto Priano, of IKAME.Question for the PanelWhat has been your favorite part of Eve Vegas?Citadel expansion image and articleEve Vegas Brain DumpGeneral Stargazer made some awesome posters for us to put up to troll Mark726/Webspaceships at Eve VegasClosing ThoughtsVisit an Eve player gathering!Rate us on iTunes and Stitcher radioSend Feedback to hydrostaticeve@gmail.comOr check out our other projectsMusicIntroduction and Transition music: Music from the Parallax release by CCP Games

Originally released in Episode 9Your browser does not support this audio Direct link: http://dl.hydrostaticpodcast.com/kyla/HKYLA_009_Seyllin_Incident.mp3Links and ResourcesThe series of chronicles leading up to the Seyllin Incident:https://wiki.eveonline.com/en/wiki/The_Spiral_(Chronicle)https://wiki.eveonline.com/en/wiki/Half_a_Life_(Chronicle)https://wiki.eveonline.com/en/wiki/1_(Chronicle)https://wiki.eveonline.com/en/wiki/The_Great_Harvest_(Chronicle)https://wiki.eveonline.com/en/wiki/We_Humans_(Chronicle)https://wiki.eveonline.com/en/wiki/World_On_Fire_(Chronicle)About Hydrostatic's Know Your Lore ArchivesThe Archives are re-releases of just the Know Your Lore segment of the larger podcast, and are released between normal episodes.

Recorded September 27th, 2015Your browser does not support this audio Direct link: http://dl.hydrostaticpodcast.com/HP_25_Theres_Nothing_Stopping_You.mp3IntroductionWe welcome ISD Sheliak Mesarthim and ISD Tedra Kerrigan to the show!Question for the PanelWhich heir do you back for the succession trials?https://wiki.eveonline.com/en/wiki/Amarr_Emperorship_Heirs,_YC118Phyridean's Pub QuizLast Episode's question: What is the special ingredient in real-life Quafe?Answer: Kacha root extract from teh mountains of Manesh on Athra. (Label: https://twitter.com/Gazimoff/status/328166544368599040)Congratulations to Eric Freeman, Stalence, and Airacaz Astreaus for winning our random draw from the 12 people who submitted.This Episode's question: How long did the fires of Malkalen burn?(Thanks to Kamar Raimo for suggesting this question!)Three people who get the correct answer will be drawn at random, and will receive any combination of NES store items worth 1965 AURMailbag, Corrections, and UpdatesNew Patrons: Jeff, Baldur, Atomic Surge, Sarah Outamon, New Eden MetaThanks to our Patrons for supporting us while we’re in a lull. We won’t think any less of you if you reduce your patronage amountDrone segment feedback:Samira took issue with Ash’s suggestion in the last mechanics drilldown that Hornets are bad. They were bad, but aren’t anymoreYanarfal points out that we neglected to talk about augmented, faction, and integrated dronesVoltaire Stonecraft of Aideron Robotics took it upon himself to figure out how to say Locke’s now-iconic “Truckloads of Drugs” in Icelandic so that we can all be prepared at Fanfest. They’re in the soundboard.Eustise pointed us to the EveEye patreon. Check it out: https://www.patreon.com/eveeye?ty=hKylan suggested we do a drill down on Factional Warfare or Incursions. Those are two things we’ll likely get around to, probably in smaller bits, and thanks for the suggestion!TheoriesReceived an interesting and well-developed theory on the Other and the AI Singularity from Kyle Craze. As with all Lore theories, I wanted to remind people that while I personally really enjoy reading them, the experts are all in the #lore channel on the Tweetfleet slack!Rick Mackling, like many of you, is expecting Jamyl to come back as a Drifter, but we’re pretty sure that CCP Falcon’s statement that Jamyl is permanently dead is going to preclude that.Resa Moon reminded us that Ghost Sites looked like they were going to be a major plot development, but they’ve sort of dropped off the radar. What gives, CCP?Kami Nakama writes in to tell us quote “Hydrostatic is my motivation to keep on flying.”Just so you know, we try to use the show to respond to mails we get, so if you don’t see an answer to your email, look for it on the next show. Same with the trivia--we’re no longer responding individually to those mails.1K subscribers to the Youtube channel. Woo!InterviewISDAn up-to-date list of what ISD is writing for us: https://forums.eveonline.com/default.aspx?g=posts&t=429656&find=unreadInformation about, and applications for, ISD: http://community.eveonline.com/community/volunteer-program/You can email ISD to let them know about important stories by using news@isd.eve-online.com or leads@eve-ic.net or leads@eve-mercury.netFind them on twitter @eveonlineisdicIC: https://wiki.eveonline.com/en/wiki/ISD_ICMercury: https://wiki.eveonline.com/en/wiki/ISD_MercuryRegion descriptions: http://backstage.eve-inspiracy.com/index.php?topic=67.0Know Your LoreISDhttps://wiki.eveonline.com/en/wiki/ISD_(Chronicle)https://wiki.eveonline.com/en/wiki/STAR_(Chronicle) (new player support)https://wiki.eveonline.com/en/wiki/Bug_Hunters_(Chronicle) (bug hunting, obviously)https://wiki.eveonline.com/en/wiki/AURORA_(Chronicle) (writing IC news articles and running events. News articles now with Mercury and Interstellar Correspondents)https://wiki.eveonline.com/en/wiki/The_Communication_Relay_Committee_(Chronicle) (Forum moderators)Closing ThoughtsThanks to Simukz for running the Eve303 meetups in Denver!/u/UpgradeNova is doing great work on Reddit with the Friendship Friday Nice Threads/u/Cormak got CCP Pizza!There’s a new awesome “Drifter Activity Intensifies” gif, that we’re told was made by KyokoShoutouts to Darth Skorpius and Nova Haven from Ash@psychosteve on Twitter let us know about a gofundme for an Eve player who lost his wife August 12th. He's sent us details that make us pretty confident this is legitimate.We'll all be at Eve Vegas! Come say hi and get stickers!Rate us on iTunes and Stitcher radioSend Feedback to hydrostaticeve@gmail.comOr check out our other projectsMusicIntroduction and Transition music: Music from the Vanguard release by CCP GamesClosing music is Pandemic Legion by David K. Magnus with additional vocals by Wendy Magnus

We are going to look at a problem that is an example of a 2-d vector calculation. A cyclist travels along a horizontal road and 5.5 m/s. A strong wind blows from one side for 1 minute, after which the cyclist is moving at 7.0 m/s at an angle of 12 degrees to their intial direction. What was their average acceleration while the wind blew?

A PhysCast on buoyancy.

A fully loaded Volvo station wagon has a mass of 1950kg. If each of its four tires is inflated to a gauge pressure of 230kPa, what is the total tire area in contact with the road?

An iron ball is suspended by a thread of negligible mass beneath a floting cylinder. The cylinder has a height of 6.0 cm, a top surface area of 12.0 cm2 and a density of 0.3 g/cm3. If the cylinder is submerged by 2.0 cm what is the radius of the iron ball?

In this hydrodynamics problem we are asked what guage pressure must a machine produce in order to suck mud of a density 1800 kg/m3 up a tube by a height of 1.5 m?

Can an emergency exit window be open mid-flight?

This question deals with both hydrostatics and hydrodynamics. A 4.0cm diameter horizontal pipe connects passes through a freshwater dam at a depth of 6.0 meters and is sealed by a plug. A) Find the magnitude of the frictional force between a plug and the pipe wall? B) With the plug removed what volume of water exits the pipe in 3.0h?

The hydrostatic law describes the weight of a fluid overlying a given area, or the pressure at a particular point. It can be used to calculate the approximate atmospheric mass over a particular area, or to calculate the change in pressure over a given change in altitude. A calculation of the pressure difference from the ground to the twelfth floor of Klein Biology Tower is found to agree well with measurements taken at both locations. The hydrostatic law also applies to pressure changes with depth in the ocean. Complete course materials are available at the Open Yale Courses website: http://oyc.yale.edu This course was recorded in Fall 2011.

The material covered throughout the course is reviewed. Properties of air and water are discussed. Hydrostatic balance is discussed as related to the atmosphere, ocean and solid earth. Geostrophic balance is a force balance between the Coriolis force and the pressure gradient force, and applies to winds in the atmosphere as well as currents in the ocean. Several examples of equilibrium states are reviewed. Heat and mass are transported by fluid motion in the earth system through winds, ocean currents and rivers. Mixing, dilution and concentration is discussed as related to ocean and atmosphere pollutants as well as salinity in the ocean. Finally, symmetry between the northern and southern hemispheres is discussed, focusing on differences in land mass, Coriolis force and the seasons. Complete course materials are available at the Open Yale Courses website: http://oyc.yale.edu This course was recorded in Fall 2011.

They say it's the best way to measure body fat percentage. Hear how it went for me. I also  tried a new machine that scans your body and recommends the right clothes for you.

Transcript: Stars are stable. For most of their lives, fusion provides the energy source. Even though the Sun and other stars are fusing hydrogen into helium, it does not mean that they are bombs. The Sun will be stable for billions of years. Stars also do not cool off. Energy flows continuously from the core where fusion occurs to the outer cooler regions. At every point within a stable star there’s an energy balance between two forces: the inward force of gravity and the outward pressure caused by energy release from nuclear reactions. This balance is called hydrostatic equilibrium.

Hydrostatic equilibrium, Big sun Eta Carinae, Stuart Layt tells three ways the world will end, This day in History. Sketches: Exile, Abraham

The electronic and magnetotransport properties of conduction electrons in the grain boundary interface of p-type Hg1−xCdxTe bicrystals are investigated. The results clearly demonstrate the existence of a two-dimensional degenerate n-type inversion layer in the vicinity of the grain boundary. Hydrostatic pressure up to 103 MPa is used to characterize the properties of the two-dimensional electron gas in the inversion layer. At atmospheric pressure three series of quantum oscillations are revealled, indicating that tthree electric subbands are occupied. From quantum oscilations of the magnetoresistivity the characteristics parameters of the electric subbands (subband populations nsi, subband energies EF−Ei, effective electron masses m*ci) and their pressure dependences are established. A strong decrease of the carrier concentration in the inversion layer and of the corresponding subband population is observed when pressure is applied A simple theoretical model based on the triangular-well approximation and taking into account the pressure dependence of the energy band structure of Hg1−xCdxTe is use to calculate the energy band diagram of the quantum well and the pressure dependence of the subband parameters.

While Cameron says some words of encouragement, Lakari calls out all his haters! We both try to save the rainforest by raising awareness of the lack of action from the world's governments. Remember kids, the world is ending! Can you say, "Apocalipsis"