Podcasts about hawc

SpaceTime Series 27 Episode 131*Ultra High Energy Gamma Rays Detected in the Milky Way's CoreScientists have detected ultra high energy gamma rays emanating from the centre of the Milky Way. This discovery, reported in the Astrophysical Journal Letters, offers a new perspective on the violent phenomena occurring in the galactic core. Using the High Altitude Water Cherenkov Observatory in Mexico, researchers measured these gamma rays at over 100 tera electron volts, providing insights into the cosmic processes involving Sagittarius A, the galaxy's central supermassive black hole.*Discovery of a Potential Triple Black Hole SystemAstronomers have identified what may be the first triple black hole system, located 8,000 light years away. This discovery could be the first direct evidence of gentle black hole formation, challenging the typical violent supernova origin theory. The system includes a central black hole, a closely orbiting star, and a far-off companion star, suggesting a more subtle formation process known as direct collapse.*NASA's New Deployable Solar Array System Faces ChallengesNASA has encountered issues with its new deployable solar array and antenna system on the Pathfinder Technology Demonstrator 4 spacecraft. The lightweight integrated solar array and antenna system, designed to enhance power and communication capabilities, is not deploying correctly due to a bent boom. This technology aims to support future deep Space missions with improved efficiency.The Science RobertA recent study reveals that standing, as opposed to sitting, does not improve cardiovascular health, despite the popularity of standing desks. Fossilised remains of a new giant elephant species have been found in India's Kashmir Valley, shedding light on elephant evolution. AI-assisted colonoscopies show a slight improvement in polyp detection. Meanwhile, Apple releases its first AI update, focusing on privacy and user data protection.www.spacetimewithstuartgary.comwww.bitesz.com

En este episodio número 78 Diego platica sobre la misión China Change-6 y la recolección de rocas del lado obscuro, tachen eso… ¡del lado oculto de la Luna ! (2:38). En el tema Jorge nos cuenta sobre el Observatorio HAWC, ubicado muy cerca del Pico de Orizaba (México), con el cual por medio de tinacos de agua y radiación Cherenkov se observa el universo a altas energías (12:33). Al final Diego nos recomienda y critica “La historia sin fin” (24:15). Tras los fotones es un proyecto de comunicación de la ciencia que realizan Jorge Fuentes Fernández (@jorgefuenfer) y Diego López Cámara Ramírez (@drpiki1) en colaboración con @AntifazPolitica. ¡Síguenos en nuestras redes sociales para estar al tanto!

Les chercheurs de la collaboration HAWC qui traquent les rayons cosmiques énergétiques depuis les pentes d'un volcan mexicain, ont exploité le fait que le Soleil influence les rayons cosmiques par son champ magnétique pour l'étudier de façon inédite avec cette sonde physique peu banale. Ils publient leurs travaux dans The Astrophysical Journal. Source Exploring the Coronal Magnetic Field with Galactic Cosmic Rays: The Sun Shadow Observed by HAWCR. Alfaro et al.The Astrophysical Journal, Volume 966, Number 1 (25 april 2024)https://doi.org/10.3847/1538-4357/ad3208

Addiction knows no boundaries.  At some point in our lives every single person will love an addict or be one themselves.  We all know someone whose life has been disrupted or ended because of its deadly force..  This episode focuses on the hard truths of addiction. We talk about how it affects the addict and their family and friends;  as well as the hopefulness that can come from recovery. There is truly no one better to break down addiction than our former classmate, Craig Hettlinger, owner of Huntington Addiction Wellness Center (HAWC). If you or someone you love is currently struggling to overcome addiction, check out the HAWC website for help.#addiction #recovery #thelylaspodcast #mentalhealthawareness #helpisavailablewww.thelylaspodcast for more information and resourcesPlease be sure to checkout our website for previous episodes, our fab, psych-approved resource page, and connect to our social media! www.thelylaspodcast.com

This edition features stories on program designed to help military spouses, Airmen learning to become more fiscal responsible and HAWC performing Gait analysis on Misawa Air Base. Hosted by Tech. Sgt. Chris Decker

MAGIC observations provide compelling evidence of the hadronic multi-TeV emission from the putative PeVatron SNR G106 3+2 7 by MAGIC Collaboration et al. on Wednesday 30 November The SNR G106.3+2.7, detected at 1--100 TeV energies by different $gamma$-ray facilities, is one of the most promising PeVatron candidates. This SNR has a cometary shape which can be divided into a head and a tail region with different physical conditions. However, it is not identified in which region the 100 TeV emission is produced due to the limited position accuracy and/or angular resolution of existing observational data. Additionally, it remains unclear whether the origin of the $gamma$-ray emission is leptonic or hadronic. With the better angular resolution provided by these new MAGIC data compared to earlier $gamma$-ray datasets, we aim to reveal the acceleration site of PeV particles and the emission mechanism by resolving the SNR G106.3+2.7 with 0.1$^circ$ resolution at TeV energies. We detected extended $gamma$-ray emission spatially coincident with the radio continuum emission at the head and tail of SNR G106.3+2.7. The fact that we detected a significant $gamma$-ray emission with energies above 6.0 TeV from the tail region only suggests that the emissions above 10 TeV, detected with air shower experiments (Milagro, HAWC, Tibet AS$gamma$ and LHAASO), are emitted only from the SNR tail. Under this assumption, the multi-wavelength spectrum of the head region can be explained with either hadronic or leptonic models, while the leptonic model for the tail region is in contradiction with the emission above 10 TeV and X-rays. In contrast, the hadronic model could reproduce the observed spectrum at the tail by assuming a proton spectrum with a cutoff energy of $sim 1$ PeV for the tail region. Such a high energy emission in this middle-aged SNR (4--10 kyr) can be explained by considering the scenario that protons escaping from the SNR in the past interact with surrounding dense gases at present. arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2211.15321v1

MAGIC observations provide compelling evidence of the hadronic multi-TeV emission from the putative PeVatron SNR G106 3+2 7 by MAGIC Collaboration et al. on Tuesday 29 November The SNR G106.3+2.7, detected at 1--100 TeV energies by different $gamma$-ray facilities, is one of the most promising PeVatron candidates. This SNR has a cometary shape which can be divided into a head and a tail region with different physical conditions. However, it is not identified in which region the 100 TeV emission is produced due to the limited position accuracy and/or angular resolution of existing observational data. Additionally, it remains unclear whether the origin of the $gamma$-ray emission is leptonic or hadronic. With the better angular resolution provided by these new MAGIC data compared to earlier $gamma$-ray datasets, we aim to reveal the acceleration site of PeV particles and the emission mechanism by resolving the SNR G106.3+2.7 with 0.1$^circ$ resolution at TeV energies. We detected extended $gamma$-ray emission spatially coincident with the radio continuum emission at the head and tail of SNR G106.3+2.7. The fact that we detected a significant $gamma$-ray emission with energies above 6.0 TeV from the tail region only suggests that the emissions above 10 TeV, detected with air shower experiments (Milagro, HAWC, Tibet AS$gamma$ and LHAASO), are emitted only from the SNR tail. Under this assumption, the multi-wavelength spectrum of the head region can be explained with either hadronic or leptonic models, while the leptonic model for the tail region is in contradiction with the emission above 10 TeV and X-rays. In contrast, the hadronic model could reproduce the observed spectrum at the tail by assuming a proton spectrum with a cutoff energy of $sim 1$ PeV for the tail region. Such a high energy emission in this middle-aged SNR (4--10 kyr) can be explained by considering the scenario that protons escaping from the SNR in the past interact with surrounding dense gases at present. arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2211.15321v1

MAGIC observations provide compelling evidence of the hadronic multi-TeV emission from the putative PeVatron SNR G106 3+2 7 by MAGIC Collaboration et al. on Tuesday 29 November The SNR G106.3+2.7, detected at 1--100 TeV energies by different $gamma$-ray facilities, is one of the most promising PeVatron candidates. This SNR has a cometary shape which can be divided into a head and a tail region with different physical conditions. However, it is not identified in which region the 100 TeV emission is produced due to the limited position accuracy and/or angular resolution of existing observational data. Additionally, it remains unclear whether the origin of the $gamma$-ray emission is leptonic or hadronic. With the better angular resolution provided by these new MAGIC data compared to earlier $gamma$-ray datasets, we aim to reveal the acceleration site of PeV particles and the emission mechanism by resolving the SNR G106.3+2.7 with 0.1$^circ$ resolution at TeV energies. We detected extended $gamma$-ray emission spatially coincident with the radio continuum emission at the head and tail of SNR G106.3+2.7. The fact that we detected a significant $gamma$-ray emission with energies above 6.0 TeV from the tail region only suggests that the emissions above 10 TeV, detected with air shower experiments (Milagro, HAWC, Tibet AS$gamma$ and LHAASO), are emitted only from the SNR tail. Under this assumption, the multi-wavelength spectrum of the head region can be explained with either hadronic or leptonic models, while the leptonic model for the tail region is in contradiction with the emission above 10 TeV and X-rays. In contrast, the hadronic model could reproduce the observed spectrum at the tail by assuming a proton spectrum with a cutoff energy of $sim 1$ PeV for the tail region. Such a high energy emission in this middle-aged SNR (4--10 kyr) can be explained by considering the scenario that protons escaping from the SNR in the past interact with surrounding dense gases at present. arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2211.15321v1

The JCMT BISTRO Survey: Multi-wavelength polarimetry of bright regions in NGC 2071 in the far-infrared submillimetre range, with POL-2 and HAWC+ by L. Fanciullo et al. on Tuesday 20 September Polarized dust emission is a key tracer in the study of interstellar medium and of star formation. The observed polarization, however, is a product of magnetic field structure, dust grain properties and grain alignment efficiency, as well as their variations in the line of sight, making it difficult to interpret polarization unambiguously. The comparison of polarimetry at multiple wavelengths is a possible way of mitigating this problem. We use data from HAWC+/SOFIA and from SCUBA-2/POL-2 (from the BISTRO survey) to analyse the NGC 2071 molecular cloud at 154, 214 and 850 $mu$m. The polarization angle changes significantly with wavelength over part of NGC 2071, suggesting a change in magnetic field morphology on the line of sight as each wavelength best traces different dust populations. Other possible explanations are the existence of more than one polarization mechanism in the cloud or scattering from very large grains. The observed change of polarization fraction with wavelength, and the 214-to-154 $mu$m polarization ratio in particular, are difficult to reproduce with current dust models under the assumption of uniform alignment efficiency. We also show that the standard procedure of using monochromatic intensity as a proxy for column density may produce spurious results at HAWC+ wavelengths. Using both long-wavelength (POL-2, 850 $mu$m) and short-wavelength (HAWC+, $lesssim 200, mu$m) polarimetry is key in obtaining these results. This study clearly shows the importance of multi-wavelength polarimetry at submillimeter bands to understand the dust properties of molecular clouds and the relationship between magnetic field and star formation. arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2209.09604v1

The all-particle energy spectrum of cosmic rays from 10 TeV to 1 PeV measured with HAWC by J. A. Morales-Soto et al. on Monday 19 September The HAWC observatory is an air-shower detector, which is designed to study both astrophysical gamma-rays in the TeV region and galactic cosmic rays in the energy interval from 1 TeV to 1 PeV. This energy regime is quite interesting for cosmic ray research, since indirect observations overlap with direct measurements, which offers the opportunity for cross calibration and studies of experimental systematic errors in both techniques. One quantity that could help for this purpose is the all-particle energy spectrum of cosmic rays. In this work, we present an update of HAWC measurements on the total cosmic-ray energy spectrum between 10 TeV and 1 PeV. The spectrum was obtained from an unfolding analysis of almost two years of HAWC's data, which was collected from January, 2018 to December, 2019. For the energy estimation, we employed the high-energy hadronic interaction model QGSJET-II-04. As in a previous work of HAWC, published in 2017, we observed the presence of a knee-like feature in the region of tens of TeV. arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2208.14245v2

Limits on the Diffuse Gamma-Ray Background above 10 TeV with HAWC by HAWC Collaboration et al. on Monday 19 September The high-energy Diffuse Gamma-Ray Background (DGRB) is expected to be produced by unresolved isotropically distributed astrophysical objects, potentially including dark matter annihilation or decay emissions in galactic or extragalactic structures. The DGRB has only been observed below 1 TeV; above this energy, upper limits have been reported. Observations or stringent limits on the DGRB above this energy could have significant multi-messenger implications, such as constraining the origin of TeV-PeV astrophysical neutrinos detected by IceCube. The High Altitude Water Cherenkov (HAWC) Observatory, located in central Mexico at 4100 m above sea level, is sensitive to gamma rays from a few hundred GeV to several hundred TeV and continuously observes a wide field-of-view (2 sr). With its high-energy reach and large area coverage, HAWC is well-suited to notably improve searches for the DGRB at TeV energies. In this work, strict cuts have been applied to the HAWC dataset to better isolate gamma-ray air showers from background hadronic showers. The sensitivity to the DGRB was then verified using 535 days of Crab data and Monte Carlo simulations, leading to new limits above 10 TeV on the DGRB as well as prospective implications for multi-messenger studies. arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2209.08106v1

Current and future gamma-ray searches for dark-matter annihilation beyond the unitarity limit by Donggeun Tak et al. on Tuesday 13 September For decades, searches for electroweak-scale dark matter (DM) have been performed without a definitive detection. This lack of success may hint that DM searches have focused on the wrong mass range. A proposed candidate beyond the canonical parameter space is ultra-heavy DM (UHDM). In this work, we consider indirect UHDM annihilation searches for masses between 30 TeV and 30 PeV, extending well beyond the unitarity limit at $sim$100 TeV, and discuss the basic requirements for DM models in this regime. We explore the feasibility of detecting the annihilation signature, and the expected reach for UHDM with current and future Very-High-Energy (VHE; $>$ 100 GeV) $gamma$-ray observatories. Specifically, we focus on three reference instruments: two Imaging Atmospheric Cherenkov Telescope arrays, modeled on VERITAS and CTA-North, and one Extended Air Shower array, motivated by HAWC. With reasonable assumptions on the instrument response functions and background rate, we find a set of UHDM parameters (mass and cross section) for which a $gamma$-ray signature can be detected by the aforementioned observatories. We further compute the expected upper limits for each experiment. With realistic exposure times, the three instruments can probe DM across a wide mass range. At the lower end, it can still have a point-like cross section, while at higher masses the DM could have a geometric cross section, indicative of compositeness. arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2208.11740v2

Validation of standardized data formats and tools for ground-level particle-based gamma-ray observatories by A. Albert et al. on Monday 12 September Ground-based gamma-ray astronomy is still a rather young field of research, with strong historical connections to particle physics. This is why most observations are conducted by experiments with proprietary data and analysis software, as it is usual in the particle physics field. However in recent years, this paradigm has been slowly shifting towards the development and use of open-source data formats and tools, driven by upcoming observatories such as the Cherenkov Telescope Array (CTA). In this context, a community-driven, shared data format (the gamma-astro-data-format or GADF) and analysis tools such as Gammapy and ctools have been developed. So far these efforts have been led by the IACT community, leaving out other types of ground-based gamma-ray instruments.We aim to show that the data from ground particle arrays, such as the High-Altitude Water Cherenkov (HAWC) observatory, is also compatible with the GADF and can thus be fully analysed using the related tools, in this case Gammapy. We reproduce several published HAWC results using Gammapy and data products compliant with GADF standard. We also illustrate the capabilities of the shared format and tools by producing a joint fit of the Crab spectrum including data from six different gamma-ray experiments. We find excellent agreement with the reference results, a powerful check of both the published results and the tools involved. The data from particle detector arrays such as the HAWC observatory can be adapted to the GADF and thus analysed with Gammapy. A common data format and shared analysis tools allow multi-instrument joint analysis and effective data sharing. Given the complementary nature of pointing and wide-field instruments, this synergy will be distinctly beneficial for the joint scientific exploitation of future observatories such as the Southern Wide-field Gamma-ray Observatory and CTA. arXiv: http://arxiv.org/abs/http://arxiv.org/abs/2203.05937v3

Entre las armas más avanzadas de los arsenales de las superpotencias se encuentran los misiles hipersónicos. Pueden viajar a más de cinco veces la velocidad del sonido (Mach 5), alcanzar objetivos a miles de kilómetros de distancia volar a baja altura y cambiar de dirección para eludir los sistemas de defensa. Como explica José Manuel Sanjurjo, vicealmirante retirado y miembro de la Real Academia de Ingeniería, no solo la maniobrabilidad es un desafío para el desarrollo de estas armas. A velocidades superiores a 6.000 km/h la fricción con la atmósfera genera temperaturas muy elevadas en la superficie de los miles, superior a los 2.000º C. Se necesitan materiales resistentes, soluciones para disipar el calor y métodos que garanticen el funcionamiento de la electrónica a bordo y las comunicaciones (GPS, etc). Estas armas pueden ser de dos tipos: planeadores y misiles cruceros hipersónicos, cada uno con sus características. En agosto de 2021, China probó uno que se quedó cerca de completar una vuelta completa a la Tierra. Rusia cuenta con los modelos Kinzhal, Zirkon y Avangard. Y EEUU ha presentado su misil HAWC. Estos misiles --explica Sanjurjo-- pueden cargar cabezas convencionales o nucleares. Según el caso, la precisión será más o menos importante. Escuchar audio

It's June 10, 2022. BoxerBlu prepares for a journey to help his mother drive cross country. We learn about companies that illegally lease dogs; how a man "married" a fictional character named Akihiko Kondo; Vladimir Putin's secret attack dolphins; the death of Regine, the creator of the first disco; how PimEyes knows everything you've done online; and a father who created a roller coaster for his 3 year-old.  And we learn about BGG Spring

It's June 10, 2022. BoxerBlu prepares for a journey to help his mother drive cross country. We learn about companies that illegally lease dogs; how a man "married" a fictional character named Akihiko Kondo; Vladimir Putin's secret attack dolphins; the death of Regine, the creator of the first disco; how PimEyes knows everything you've done online; and a father who created a roller coaster for his 3 year-old.  And we learn about BGG Spring

“Why you do the things you do is more important than what you're doing” Bankole Williams.Your why is the reason for a thing which propels your passion, goal and purpose. Knowing your “Why” means understanding the purpose & reason you do the things you do. It's the actual fuel that motivates you to do the things you do. It is the reason why you MUST. The drive that motivates you to get to work each morning and take care of business.In this insightful episode, You will learn the reason and passion behind the relentless passion of Shavon Williams.  I met Shavon at the shelter home where I found a safe haven after I fled for safety.  Shavon  Williams is the President and CEO of Purple Heart foundation, an organization that nurtures and cares for victims and survivors of domestic violence. In this episode, Shavon poured our her heart as a senior family advocate at the riverside community care. Where she provides therapy, advocacy and groups for individuals, children and families who have experienced abuse and those who have experienced child-care trauma within the home. Shavon began her DV experience as an intern at HAWC in 2014, and began working with them following her internship. She has experienced working amongst residential community, domestic violence shelter programs and now out-patient services. This episode reached the climax when Shavon shared her own personal experience which was birthed from being a survivor of domestic violence. She is one of the finest and highly compassionate advocate because of her love, care and empathy for clients and those she care for. To know Shavon is to love her. She is compassionate, empathetic and understanding.This episode will enlighten you to understand the life and activities at the domestic violence shelter program and how to better support victims, survivors and thrivers of domestic violence.Connect with at: www.facebook.com/shavonwilliams

Two weeks ago, an elite team completed the first successful free-flight test of the Hypersonic Air-breathing Weapon Concept (HAWC) missile. Raytheon Missiles & Defense worked with Northrop Grumman to build the prototype for DARPA.For the test, the HAWC was released from underneath the wing of an aircraft. Seconds after it deployed, the missile's solid rocket motor boosted it to supersonic speeds. The HAWC's scramjet (supersonic combustion ramjet) engine ignited and accelerated the missile to hypersonic speeds above Mach 5 (five times the speed of sound).

Last month, the Defense Advanced Research Projects Agency (DARPA) took a hypersonic missile prototype built by Raytheon Missiles & Defense and Northrop Grumman and completed a successful free-flight test.This test involved a Hypersonic Air-breathing Weapon Concept (HAWC) missile. The HAWC's engine got it to as fast as five times the speed of sound, about 3,853 miles per hour. It was a monumental moment for hypersonics, which are expected to be the new frontier for advanced weaponry. But now, Reuters reports the Pentagon is saying hypersonics are too expensive. It requests defense contractors cut the ultimate cost of such weapons as a unit can cost tens of millions.

The Today in Manufacturing Podcast is brought to you by the editors from Manufacturing.net and Industrial Equipment News (IEN).In each episode, we discuss the five biggest stories in manufacturing, and the implications they have on the industry moving forward. This week:NAM: China 'Remains a Hub of Bad Behaviors'On Monday, U.S. Trade Representative Ambassador Katherine Tai took a shot at China's trade practices. In response, National Association of Manufacturers President and CEO Jay Timmons released a statement. In it he said, “China is not following through on important commitments made in the 2020 U.S.–China ‘Phase One' agreement."Taiwan's Foxconn Has Deal to Buy Lordstown Plant in OhioFoxconn Technology Group has reportedly reached a deal to buy an auto assembly plant in Ohio from Lordstown Motors.Hypersonic Missile Passes Crucial Flight TestA few weeks ago, an elite team finished the first free-flight test of the HAWC, the Hypersonic Air-breathing Weapon Concept missile. Raytheon worked with Northrop Grumman to build the prototype for DARPA and the test was a success.Chinese Automaker Sells SUV Under Dodge BrandChinese automaker GAC Group is making its first significant vehicle exports to Mexico. What is interesting is that the SUVs will carry the Dodge brand name.Workers at All of Kellogg's U.S. Cereal Plants Go on StrikeKellogg's cereal plants in Omaha, Nebraska, Battle Creek, Michigan, Lancaster, Pennsylvania and Memphis, Tennessee came to a halt on Tuesday when some 1,400 workers went on strike. Kellogg's says its employees made an average of $120,000 last year. However, workers say it took a lot to get there, including 74- to 84-hour weeks.In Case You Missed It:Toymakers Race to Get Products on Shelves Amid Supply ClogsThe Basic Fun toy company did something crazy this week. It decided to ditch one-third of its Tonka Mighty Dump Trucks in China.New Kellogg Breakfast Cereal Inspired by Wendy's FavoriteDubbed "Wendy's Frosty Chocolatey Cereal," the limited edition item will feature chocolate marshmallow pieces and “cocoa-coated round cereal bites."William Shatner Will Fly to Space Aboard Blue Origin RocketBlue Origin will blast “Star Trek” actor William Shatner into space on Oct. 12.Please make sure to like, subscribe and share the podcast. You could also help us out a lot by giving the podcast a positive review. Finally, to email the podcast, you can reach any of us at Jeff, Anna or David [at] ien.com, with “Email the Podcast” in the subject line.

[年代向钱看] 美成功試射HAWC飛彈！強化國防！抗中武器發展要能打得遠！關鍵中南海？ ！新八國聯軍分進合擊？！【2021.10.02『年代向錢看』週末精選】

[年代向钱看] 獨！中國限電遍地開花！紅綠燈罷工大塞車！ 習近平瞄準金融虎！下令巡視25家金融構？！美成功試射HAWC飛彈？！【年代向錢看】20210928 獨！中國無預警停電！衝擊台灣PCB大本營？囂張擾台！中國軍機侵我國ADIZ逾500架次！前AIT處長認為習近平搞壞兩岸關係？！朱習會很快登場？！【年代向錢看】20210928

The Amazing and super talented Angela Lee talks with Trev about her band, Radio Compass. How it feels being featured in the video game Rock Band!  The annual fundraiser she does with HAWC, and more!Website:RADIO COMPASSBandcamp:radiocompass.bandcamp.comSocial Media: FacebookIGDon't forget to head to Get-Punk.com  , the internets best source for punk vinyl and use the discount code STRUGGLE at check out for 10% off your order!Record of the week:Mark Lind and the Unloved:  The Last BastionGetPunk.com The internets best source for punk vinyl Use the offer code STRUGGLE at check out for 10% off your order

La collaboration HAWC de détection de rayons cosmiques vient d'identifier une imposante source de rayons cosmiques très énergétiques, et à la surprise des chercheurs, celle-ci n'est pas un des accélérateurs astrophysiques classiquement attendus comme des résidus de supernova, mais simplement un amas d'étoiles en formation. Une étude publiée dans Nature Astronomy.

渦輪星系 ê 磁場 磁場敢一定會佮星系 ê 捲螺仔手骨仝一个方向？這个用正面向咱 ê 渦輪星系 (M51) ，是佇盤仔形星系內底，一个看會著真清楚 ê 捲螺仔波形 ê 星系。咱用電波望遠鏡來 kā 看，會當看著磁場綴著捲螺仔手骨 ê 曲度。毋閣，NASA 有一台佇天頂咧飛 ê 紅外線平流層望遠鏡 (SOFIA) ，煞看著 M51 ê 磁場佇星系盤 ê 外沿交織。磁場會當佇紅外線波段，像偏光鏡原理按呢，ùi 塗粉粒 ê 排列方向推算出來。疊佇這張影像面頂 ê 線，是用演算法 kā 偏振光算出來 ê 磁場方向連起來 ê 。影像頂懸反紅 ê 恆星形成區，是用哈伯太空望遠鏡翕 ê 。是講，可能是影像頂懸彼粒星系伴 ê 引力，kā 這粒塗粉滿滿是 ê 星系拖去，產生較強 ê 亂流，kā 塗粉絞絞去，才會佇星系 ê 外沿手骨，產生這款料想袂到 ê 磁場形態。 ——— 這是 NASA Astronomy Picture of the Day ê 台語文 podcast 原文版：https://apod.nasa.gov/ 台文版：https://apod.tw/ 今仔日 ê 文章： 影像：NASA, SOFIA, HAWC+, Alejandro S. Borlaff; JPL-Caltech, ESA, Hubble 音樂：PiSCO - 鼎鼎 聲優：蔡老師 錄音：玉成戲院錄音室 翻譯：An-Li Tsai (NCU) https://apod.tw/daily/20210120/ 原文：https://apod.nasa.gov/apod/ap210120.html Powered by Firstory Hosting

On Tuesday's Houston Matters: Texas Republican Ron Wright has died, making him the first sitting member of Congress to lose his life after testing positive for the coronavirus. And why is Attorney General Ken Paxton’s office facing deeper cuts than most state agencies in lawmakers’ proposed budget for the next two years? Also this hour: City Councilmember Tiffany Thomas, who represents District F, answers listener questions. Then we learn how local nonprofits assist law enforcement... Read More

Emilee Whitehurst is the president and CEO of the Houston Area Women’s Center (HAWC). Their multi-lingual staff is about to decentralize its operations to bring help closer to those who need it most. Emilee explains how with the help of a huge grant from the City of Houston and matching donations and various reinvestments, HAWC will open locations strategically placed around Houston to help women get out of abusive situations and restart their lives with housing help. The goal is to help them become independent and their programs are very successful . They are overwhelmed by the rise in violence due to the pandemic and now is a good time to give them our support. Small donations matter a great deal!www.hawc.org Domestic Violence Hotline: 713-528-2121Sexual assault Hotline: 713-528-7273

Join us as we do a deep dive into what the HAWC can do for you during COVID! And it turns out we barely scratch the service. Today our gets provide us with practical ways to take care of ourselves with nutrition, relaxation techniques, and we even get let in on what is called the 20/20/20 rule that'll change the way you work from home! You can find information on their programs and activities on FACEBOOK: @628MedicalGroup @JB.CHS.CARES Call: 843.963.4087 and leave a message to get in touch with the team or leave your Email to get on their mailing list. Email nikki.conley.3@us.af.mil or alaine.mlls.ctr@us.af.mil for further information on programs and classes.

49 - Embriones dinosaurianos, jet de proporciones cósmicas y un telescopio en mi tierra (y un bonus) En este episodio, platicamos acerca de fósiles de embriones de dinosaurio como nunca se habían estudiado, nos sorprendemos de la observación de una imagen cósmica inédita, traída hasta nosotros por el mismo telescopio que nos trajo al agujero negro, y en la voz de nuestro invitado David Venegas, escuchamos una historia de puentes sociales entre un proyecto científico y los habitantes de un pueblo. Ah, y un bonus al final. Menú 00:20 - Introducciones y saludos 02:13 - Cráneos de embriones de dinosaurio 22:04 - Primera imagen del jet de un agujero negro 45: 31 - Astrofísica en el volcán Sierra Negra 1:25:24 - Agradecimientos y despedidas 1:26:36 - BONUS!: Nuestro invitado de cerca Invitado - David Venegas Voces y contenido: David Venegas, Sofía Flores, Rodrigo Pacheco y Víctor Hernández Producción: Sofía Flores, Rodrigo Pacheco y Víctor Hernández Edición: Víctor Hernández Voz en la rúbrica: Valeria Sánchez Este podcast es producido desde un lugar de la Ciudad de México que bien podría ser realmente cualquier lugar porque ya todo lugar es adentro. Fuentes y lecturas recomendadas Sobre los huevos de dinosaurio: El comunicado institucional:http://www.esrf.eu/home/news/general/content-news/general/synchrotron-x-ray-sheds-light-on-some-of-the-worlds-oldest-dinosaur-eggs.html El artículo original (en inglés, de libre acceso): https://www.nature.com/articles/s41598-020-60292-z Sobre el telescopio de horizonte de eventos: Nota periodística en inglés: https://astronomy.com/news/2020/04/event-horizon-telescope-peers-down-a-black-holes-jet Artículo original: https://iopscience.iop.org/article/10.3847/1538-4357/ab754f Sobre telescopios y defensa del territorio: El proyecto HAWC: https://es.wikipedia.org/wiki/Observatorio_de_Rayos_Gamma_HAWC Página oficial: https://www.inaoep.mx/~hawc/telescopio/ El caso del telescopio en Hawaii: https://www.insidehighered.com/news/2019/07/25/u-hawaii-pursues-controversial-thirty-meter-telescope-mauna-kea-and-leading Música y audios "Telescope" de Cage the Elephant: https://www.youtube.com/watch?v=9OCEh6g6whc "Brightest star" de Santana: https://www.youtube.com/watch?v=O2etxFGeG2s (sí, sabemos que no es una estrella, pero sí es la más brillante) "Huevos con aceite" en vivo, de Twisted Sisters (sí, se enteraron y la cantaron así en Chile; miren:): https://www.youtube.com/watch?v=SGBAAgLFGUs Intro y salida: Little Lily Swing, de Tri-Tachyon, bajo una licencia Creative Commons 3.0 de Atribución: freemusicarchive.org/music/Tri-Tachyon/ Rúbrica: Now son, de Podington Bear, freemusicarchive.org/music/Podington_Bear/ Bajo una licencia Creative Commons Internacional de Atribución No Comercial 3.0 Eggs! Toast! Gas! Fish! by Elvis Herod is licensed under a Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 License.

Chau Nguyen, Chief Public Strategies Officer at Houston Area Women's Center Chau Nguyen is the Chief Public Strategies Officer for the Houston Area Women’s Center, tasked with managing and expanding key partnerships while positioning HAWC as thought leaders in order to drive broad awareness of domestic violence and sexual assault, with a goal of reducing interpersonal violence and changing cultural norms about how survivors are understood. Prior to her leadership in the non-profit space, Chau spent 15 years as a television news journalist and last served as an anchor and reporter with KHOU TV. She is the first Vietnamese American journalist to receive an Emmy Award for her documentary series covering a medical mission in Vietnam, and the Houston Press has named her Reporter of the Year. A native Houstonian, Chau is passionate about staying connected to her community, serving on numerous Boards. She currently sits on the Boards of Catapult and The University of Houston Friends of Women’s Studies, and she is on the advisory board of Houston Achievement Place. Chau is a Licensed Master Social Worker and holds a Masters of Arts in Social Work from the University of Houston and a Bachelor of Arts in Communications from the University of St. Thomas.  She is frequently asked to emcee events, including Houston Mayor Sylvester Turner’s Inauguration in 2016.  Chau is the proud mother of two young girls, Ryan and Myles, a Yorkie named Peanut, and she is an active member of Unity of Houston. Additional information: https://houstonfamilymagazine.com/i-am-houston/chau-nguyen-giving-women-voice-abuse/ --- Send in a voice message: https://anchor.fm/sammyz/message

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TW: Discussions of physical, emotional, and sexual assault. On this week’s special Riveting Broads’ episode, Molly talks to Jacqui about her experience with domestic abuse. Through recounting her relationship, the broads discuss the blurred lines of toxic vs. abusive behavior, mixed with the confusion, manipulation, policing, intimidation and the loss of oneself. Further, they discuss how to validate one’s experience and how to move on from trauma. Or alternatively, how to support someone going through it. NOTE: If you or a loved one are in an abusive situation, you are not alone. We are here and there are resources for you. If you are local to the North Shore, please consider using HAWC as a resource. HAWC provides free services to abuse victims. To understand if what you’re experiencing is abuse, or to start making a safety plan, call their hotline at 1-800-547-1649.

Nicki talks with Elisabeth Wren of HAWC (Healing abuse working for change) 

On this episode Nicki talks with Sara Stanley, Executive Director of HAWC (Healing Abuse Working for Change).   October is Domestic Violence Awareness Month! 

Jan Saylors with Helping Animals of Warren County chats with Sheila about what HAWC does and how they make the lives of the animals better in their area. Brought to you by Dog & Company. Lite Rock 95.9

News Talk 94.1 — Jan Saylors with Helping Animals of Warren County chats with Sheila about what HAWC does and how they make the lives of the animals better in their area. Brought to you by Dog & Company.

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https://www.tourdecrypto.com/ https://bitninjasupply.com/ https://hodlfuel.com/  Biking Across America, Crypto Cyclists Look to Raise $1 Million for Charity September 12, 2018, 03:43:31 PM EDT By Rebecca Campbell, Bitcoin Magazine Crypto, charity and cycling. It's an unlikely triad, but two fitness enthusiasts-turned-crypto philanthropists believe that, taken in combination, the three can drive positive change. Taking a cross-country cycling trip around the U.S., Tour de Crypto riders Jason Berlin and Jovel Velasquez want to raise $1 million in cryptocurrencies and USD for the Houston Area Women's Center ( HAWC ), a non-profit organization with the mandate to "[end] domestic and sexual violence for all." Through its advocacy, counselling, education, shelters and support services, HAWC works to help survivors build safe and healthy lives. If Berlin and Velasquez meet their goal, the money will be enough to fund half a year of services to HAWC's 120-bed secure shelter. To ensure transparency, donors can verify that the wallet addresses listed on Tour de Crypto's website and HAWC's own are the same, and "100% of the donations will go directly to HAWC via wallets maintained and controlled by HAWC," Tour de Crypto's donation page states. The tour will kick off on Friday, September 14, 2018, in the Hamptons, New York, ending on Friday, November 9, 2018, in Huntington Beach, California, and the entire trip will also be recorded with videographers and an audio crew along the way. Along the route , Berlin and Velasquez will be stopping in Houston to visit the headquarters of HAWC. At the time of publication, the project is accepting donations in bitcoin, ether, litecoin, monero, digibyte, reddcoin, electra, paccoin and phore. The Electra community was the first to sign up, according to Blake Rizzo, head of charity affairs for Tour de Crypto. At last count, he said that over 7 million electra (~$4,340) had been donated to HAWC. Speaking to Bitcoin Magazine , Rizzo explained that he was approached by Berlin with the idea of the tour. Rizzo said that Berlin came up with the concept, a play on the Tour de France, as a way to do something that raises awareness for cryptocurrency donations to charity. "He also had a personal goal to ride a bike across the United States, so he decided to combine the two," Rizzo added. With a background in law as a commercial litigation attorney, Berlin originally approached Rizzo to draft documents for the tour. However, the more Rizzo got involved, the more opportunity he saw, so he took on a more active role to help increase awareness of the riders' mission and how they hope to accomplish it. When Berlin began speaking to Rizzo about potential charities, Rizzo immediately suggested HAWC, which has a four-star rating on Charity Navigator . It wasn't long before Berlin decided to make the sexual assault survivor center the main focus on the first tour, which is expected to be the first of many. "The goal is to do this every year and not only have a charity that is the main focus, but also ask other communities and coins to get involved and do one of two things," said Rizzo. "They can have me set up HAWC with their particular wallet so their community can donate or [they can] go out and get another charitable organization accept their coin, so we can add them to the list and promote different charities along the way." In a way, the first tour will be a trial run to see how crypto communities can come together to benefit charitable organizations. Beyond raising money for HAWC, the tour will be a challenge for its two riders. According to Rizzo, Berlin and Velasquez are not your typical Lycra-clad cyclists, but that's not to say they haven't put the work in prior to the start of the trip. During the interview, Rizzo told me that the pair had just completed a 130-mile training trip, and the two are riding each day to condition themselves and prep their legs for the roughly 4,000 mile journey. When they're not riding, Berlin is talking to various exchanges and coin operators who are interested in getting involved on the tour, either as sponsors or participating coins. So far, Ronnie Moas, founder of Standpoint Research and World Crypto Con , is a leading sponsor. World Crypto Con's website states that it will donate 5 percent of all ticket sales to HAWC. Moas was quick to join the effort. When raising awareness for Tour de Crypto, Rizzo came across a tweet from Moas regarding World Crypto Con, so he reached out to talk to him about the tour's charitable mission. "Within minutes he responded," added Rizzo. "He had checked out our Twitter page and our mission and basically said 'I'm in, call me or send me your number,' and just like that I was on the phone with him for an hour and a half going through everything. He agreed right there to be our lead sponsor."

Los rayos cósmicos son partículas de alta energía que llegan a la Tierra procedentes de fuentes galácticas lejanas. En su mayoría están formados por protones o núcleos atómicos, pero junto a ellos llegan también, en menor proporción, electrones y positrones. Hace más de 10 años, gracias a observaciones con satélites espaciales, se observó que llagaban a la Tierra más positrones de lo que las teorías predicen, especialmente de aquellos que tienen mayor energía. Desde entonces se han propuesto distintas hipótesis que justifican el resultado, una de ellas propone que la fuente debe estar en ciertos púlsares y otras señalan a la materia oscura o procesos desconocidos. Una investigación, en la que participa Rubén López Coto, ha utilizado el High-Altitude Water Cherenkov Observatory (HAWC), situado en México, para estudiar dos púlsares conocidos y propone que el origen de los positrones podría ser más exótico de lo que se pensaba.

Grâce à une mesure inédite de la région d'émission gamma entourant deux pulsars proches avec le détecteur HAWC, une grande collaboration internationale arrive à déterminer que les positrons détectés en excès sur Terre ne viennent pas de ces pulsars mais auraient une toute autre origine...

In this week’s show our guest is Leticia Manzano from the Houston Area Women’s Center (HAWC). Ms. Manzano is the Sexual Assault Services Coordinator at HAWC. During this episode we discuss current affairs, such as the accusations against Harvey Weinstein and Donald Trump, the definitions of rape and sexual assault, and how the media can serve as a resource for survivors. We also explore how it is often challenging for those who have experienced sexual violence to share their story and how victim-blaming shifts responsibility away from the perpetrators. Anyone seeking additional information on this issue can contact the National Sexual Assault Hotline at 1.800.656.HOPE (4673).

In our own galaxy and beyond, violent collisions fling a never-ending stream of stuff at the earth, and astrophysicists are eager to learn more about the processes that produce this cosmic barrage.

In our own galaxy and beyond, violent collisions fling a never-ending stream of stuff at the earth, and astrophysicists are eager to learn more about the processes that produce this cosmic barrage.Researchers from around the world have teamed up to build the High-Altitude Water Cherenkov (HAWC) gammy-ray observatory, an array of hundreds of huge water tanks on a mountain in Mexico. HAWC helps astrophysicists spot active cosmic neighborhoods by capturing the shower of particles created when high-energy packets of light smash into the earth’s atmosphere.Jordan Goodman, HAWC’s lead investigator, and Dan Fiorino, a postdoctoral researcher at UMD, tell Chris Cesare about the details of the HAWC experiment and how it promises to fill some gaps in our understanding of the universe. To learn more about HAWC, please visit www.hawc-observatory.org. The collaboration is preparing to publish the first results of its search, and you can read about the details in an upcoming source catalog or a paper about high-energy gamma rays from the Crab Nebula.This episode of Relatively Certain was produced by Chris Cesare, Sean Kelley and Emily Edwards and edited by Chris Cesare and Kate Delossantos, featuring music by Dave Depper, Podington Bear, Kevin MacLeod and Chris Zabriskie. Relatively Certain is a production of the Joint Quantum Institute and the University of Maryland, and you can find it on iTunes, Google Play or Soundcloud.

L'observatoire gamma High Altitude Water Cherenkov (HAWC) a débuté ses opérations à l'été 2013 (voir ici). Cet observatoire qui a pour objectif d'étudier l'origine des rayons cosmiques et des rayons gamma ultra énergétiques vient de rendre publique la semaine dernière sa première carte du ciel gamma couvrant 2/3 du ciel. On y découvre de nouvelles sources d'émission gamma ainsi que des zones déjà connues mais avec plus de détails.

This week on The Little Radio Show we talk about Twitter's new “buy” button; we have an interview with Leticia Manzano from the Houston Area Women's Center about Domestic Violence Awareness Month, and we reminisce on ghost stories in celebration of Halloween. In the In Case You Missed it Segment (ICYMI) we talk about changes in LinkedIn, with LinkedIn Groups becoming private. And … did you hear the story about the drunk driver who was Periscoping herself and gots arrested? Her viewers called the police on her. You can find the complete story on CNN, after you listen to the show. Twitter has rolled out their “Buy” button, making it possible to purchase from select ecommerce providers without ever leaving Twitter. What does this mean for us as conspicuous consumers, and for business owners? You can read more about this new feature in the Twitter announcement, or find out how to implement this for your business. October is Domestic Violence Awareness Month. To talk about this we invited Leticia Manzano from the Houston Area Women's Center (HAWC) to join us on the show. She provides us with more information about the services and programs HAWC offers. They are located at 1010 Waugh Dr., Houston TX 77019. Their hotline is 713-528-2121. And getting in the spirit of Halloween, we talk about ghost stories, scary moments, and other things that go bump in the night. “The Little Radio Show” is on HMSNetRadio.org on Thursdays at 2 pm (CST). The show hosts are Sandra Fernandez (@sandrasays), Juan Alanis (@juanofwords), and Anjelica Cazares (@la_anjel). Subscribe to the Podcast via (RSS), on the iTunes channel or on our Stitcher channel, and keep up with new episodes. Subscribe to the Blog and keep up with new posts. The show's website can be found at thelittleradioshow.com.

Episodio 64 – Las partículas que vinieron del espacio, con Hermes León “Radiación cósmica” es un buen nombre para una banda de rock progresivo, pero también es un fenómeno que nos permite conocer mejor el universo. La radiación cósmica ha sido estudiada por más de 100 años, y su historia conecta un globo aerostático en las planicies de Bohemia en Alemania, con un conjunto de tanques de agua ultra-pura en las laderas de la Sierra Negra, en Puebla, México. En este episodio, platicamos con Hermes León Vargas, un joven investigador del Instituto de Física de la Universidad Nacional Autónoma de México, quien nos contó cómo es que esos tanques de agua se usan a manera de observatorio de radiación cósmica (un observatorio llamado HAWC), qué tipo de fenómenos puede estudiar ese observatorio y la importancia de esos estudios para entender mejor nuestro universo. ¡Que lo disfruten! --Créditos-- Invitado: Dr. Hermes León Vargas Secciones: Sofía Flores Guión: Víctor Hernández Marroquín, Sofía Flores Fuentes, Rodrigo Pacheco Muñoz, Emiliano Rodríguez Mega y Alejandra Ortiz Medrano. Producción: Marcela Montiel Grabación en cabina y edición: Roberto Portillo Edición y diseño de audio: Carolina Durán Agradecemos al IMER por la realización de este programa. Imagen tomada de Wikipedia: https://en.wikipedia.org/wiki/High_Altitude_Water_Cherenkov_Experiment

Hello everyone and welcome back to another episode of the Women's Sports Matter Podcast! In today's episode, I had Boston Renegades Player Erin Truex on the podcast! We talked about what it was like being supported by Robert Kraft and the New England Patriots organization last season, the disparities between men's and women's sports, and how you can support the Women's Football Alliance. You can follow me on Twitter and Facebook @WSMpodcast & Instagram @womenssportsmatter. To submit questions, topics, folks I should interview, and more, send me a DM! Want to message me about coming on the podcast or for suggestions? Email the podcast here: womenssportsmatterpodcast@gmail.com. Make sure to subscribe and thanks for listening!Links from today's episode:Cleat Sheets: https://open.spotify.com/show/3TtHQNsNw9Ul5fRlUOxsTo?si=05fc37880bcc477eWomen's Football Alliance: https://wfaprofootball.com/Mabel Center for Immigrant Justice: https://www.mabelcenter.org/HAWC: https://hawcdv.org/Behind You Inc.: https://www.behindyouinc.org/United Soccer Coaches Convention: As I've mentioned in previous episodes, I will be attending the United Soccer Coaches Convention in Kansas City, MO from January 20-22, 2022! Want to register? Visit unitedsoccercoachesconvention.orgPodcasts I've Been On:On the Beat: https://youtu.be/10T5LhMZAOoBrandon's Sports Talk: https://youtu.be/tb2HRNhfjzMBryant and Me: https://open.spotify.com/episode/6kGMOl46uzRKgBohNAfUpf?si=e5843333182745c8The Final Third Podcast: https://open.spotify.com/episode/4gE0UOhI0iebqzlRqDZZC1?si=74684a56e5814481https://open.spotify.com/episode/5tSpItgcs1OuCxiK9fpTQO?si=13064cd24e7b4298https://open.spotify.com/episode/2E1APdTg8qLzczXCjuKWUL?si=0af34ff428134139United Soccer Coaches Podcast: https://open.spotify.com/episode/4cChnScMp0iULj5ybfWyP5?si=3b2c539f8ab14090 Articles About The Podcast: Medi-Nerd: https://medi-nerd.com/2021/10/23/2021-wizardworld-chicago-trip/On the Beat: https://globalwomenssportsradio.com/f/on-the-beat-with-gianna-belcastro-of-womens-sports-matter?fbclid=IwAR0YWeAZ6d5ki56qmiMHNadjIVMnsEtrbArX4fMCqiGGKIU1U-1eTaaxnBw Patch: https://patch.com/illinois/chicago/beat-wizard-world-2021?fbclid=IwAR0ciAAH2Pimi1I1ocBNaULIq_5gUGElASCTxSqENcKvaJdhY2neFvzSvjs  Resources:Register to Vote: https://www.vote.org/Find A Vaccine Near You: https://www.vaccines.gov/search/Black Women's Player Collective: https://www.bwplayercollective.org/NWSL Player's Association: https://www.nwslplayers.com/Find Your Legislator: https://openstates.org/find_your_legislator/The Trevor Project: https://www.thetrevorproject.org/NAMI: https://www.nami.orgBLM: https://blacklivesmatters.carrd.co/ Other great sports podcasts: https://sportsmarketanalytics.com/Resource-Center/Media/Podcasts.aspxhttps://open.spotify.com/show/2rc8WvMP4yAy3mZOgD1L71?si=5a7bd57f58404788https://open.spotify.com/show/4n4ZxsVs1Ix9DY9E0KPSc6?si=2f7b7ef1b1554649https://open.spotify.com/show/5sNbmAKpf7nzOJMFuJZFSZ?si=22be190fea90463ahttps://open.spotify.com/show/6QcIR6XhR2SEYtN5rI2cFl?si=d12ca95561d54ab8https://open.spotify.com/show/7ut3cCgCUDIJ7KMNBfX2fa?si=3948d14db2e74766Social Media:Instagram: https://www.instagram.com/womenssportsmatter/Twitter: https://twitter.com/WSMpodcastFacebook: https://www.facebook.com/WSMpodcastMy Youtube Channel: https://www.youtube.com/channel/UCfvUE_I7u2rbN3aOFOX1M-A/My podcast website: https://redcircle.com/shows/womens-sports-matter Where you can listen to my podcast: Amazon Music, Anghami, Apple Podcasts, Audacy, Audible, Breaker, Gaana, Google Podcasts, iHeart Radio, Overcast, Pocket Casts, RadioPublic, RedCircle, Spotify, Stitcher, and TuneIn.More Platforms Coming Soon!Support this podcast at — https://redcircle.com/womens-sports-matter/exclusive-content