Podcasts about tude

Après avoir conduit une étude sur les primo-accédants avec l'Ifop, le courtier Cafpi a dressé une carte de France des jeunes emprunteurs riche d'enseignements. Quelles sont les régions où on emprunte le plus tôt, le plus longtemps, où l'on favorise le neuf...? Les réponses avec Philippe Taboret, directeur général adjoint de Cafpi. Mon Podcast Immo est un podcast quotidien et indépendant, produit par MySweetImmo.com. Pour le soutenir, abonnez-vous et laissez des étoiles ou des commentaires sur votre plateforme de podcast préférée. 

durée : 00:02:30 - C'est mon boulot - par : Philippe DUPORT - Les mères de famille et les cadres sont les plus concernés, selon une étude. Six critères sont retenus pour évaluer cet indice de charge mentale comme les troubles du sommeil ou l'omniprésence du travail dans les pensées.

Mon Podcast Immo analyse la 2e vague du baromètre "Les Français et l'immobilier" avec Laurent Sabouret, cofondateur de l'agence en ligne Imop, qui a fait réaliser cette étude passionnante par Harris Interactive. Mon Podcast Immo est un podcast quotidien et indépendant, produit par MySweetImmo.com. Pour le soutenir, abonnez-vous et laissez des étoiles ou des commentaires sur votre plateforme de podcast préférée. 

En partenariat avec Expat Pro :https://www.expat-pro.com/ Catherine réalise sa première expatriation à l'âge de 5 mois aux Antilles étant donné que son père était géologue et voyageait beaucoup. Elle part donc en Italie, en Guadeloupe, en Guyane et à Madagascar. Elle est aujourd'hui expatriée en Allemagne à Berlin avec sa famille. Elle exerce la profession de coach en orientation scolaire notamment grâce à son expérience à la fois de parent d'enfants d'expatriés et d'enfant de parents expatriés.  https://www.instagram.com/chabincoaching/  ............................................   Vous avez aimé ce podcast ?   Soutenez et aidez la 1ère radio des Français dans le monde en faisant un don à notre association pour nous aider à nous développer. Nous préférons votre participation plutôt que de la pub, pas vous ?  http://association.stereochic.fr   Europe-Allemagne - enseigner enfants 

durée : 00:02:41 - C'est mon boulot - par : Philippe DUPORT - Selon une enquête menée par l'Ifop, 23% des personnes interrogées estiment avoir vécu des discriminations lors des entretiens d'embauche.

05  ...that always feels good to... 10  I just started seeing musicians out on the street 15  It's like an undefined thing 20  I like cool new stuff 25  It ends with the epilogue 30  It's a good TMD record 35  We drove and talked about it 40  F sharp was never really in it 45  ...amp out in the kitchen... 50  It's just a guideline for dumb people

05  The computer talked to LOGIC 10  Maybe I was overreaching 15  ...weekly or monthly... 20  I love you, Paul 25  Turn the dryer off because we're doing tracks 30  This is like a brand new fucking thing 35  That's a bummer 40  I haven't even looked at my notebooks 45  Strictly because I don't have a CD player anymore 50  Just barely get a mark on it 55  Dark chocolate, that's the way to go.

durée : 00:03:23 - Musique connectée du lundi 01 mars 2021 - par : Suzanne Gervais - Qui sont les pays les plus influents, musicalement parlant ? C’est ce que révèle une étude allemande, qui vient de paraître.

durée : 00:01:44 - Le vrai du faux - par : Antoine KREMPF - Maux de tête, troubles de l'apprentisage ou encore inconfort... Une infographie partagée plusieurs milliers de fois depuis quelques jours laisse entendre qu'une étude a mesuré "les répercussions" du port du masque chez les jeunes. C'est faux.

Ate onde k bo era kapaz de bai por kauza de fé, por causa de religião? E manera k bo tava sinti komo irm@ de famoso detetive Sherlock Holmes? Na episodio de aoje no te bem fala de doj film; O Diabo de cada Dia e Enola Holmes. No tem “Enola Homes”, ke irmã de Sherlock interpretod pa um jovem atriz em ascensão Milly B. Brown. E no tem “O Diabo de cada Dia” eh k tem komo ator principal jovem Tom Holland maj kunxid pa Homem Aranha. Filme Enola eh sobre um mnininha bastante corajosa e inteligente eh k te sei te expia se mãe eh k desaparece, e na procura pa se mãe el te kaba pa passa pa txeu koza e “encontra” se pessoa ness processo. O Diabo de cada dia eh um filme complexo, cheio de personagens interessantes eh k te gira a volta de noj jovem protagonista, e onde k linha pa separa amor, fé, e paranoia, eh quase inexistente. Tude ej 2 film eh de época, cheios de drama e um bokedin de mistério. No tem um elenco de atores supertalentosos, e Netflix te mostra maj um vez kel k te na brincadeira k sej produções. Ej filme te vale a pena, por iss ba oiaj e depois bo bem uvi ess episodio. Bom sessão!

Ate onde k bo era kapaz de bai por kauza de fé, por causa de religião? E manera k bo tava sinti komo irm@ de famoso detetive Sherlock Holmes? Na episodio de aoje no te bem fala de doj film; O Diabo de cada Dia e Enola Holmes. No tem “Enola Homes”, ke irmã de Sherlock interpretod pa um jovem atriz em ascensão Milly B. Brown. E no tem “O Diabo de cada Dia” eh k tem komo ator principal jovem Tom Holland maj kunxid pa Homem Aranha. Filme Enola eh sobre um mnininha bastante corajosa e inteligente eh k te sei te expia se mãe eh k desaparece, e na procura pa se mãe el te kaba pa passa pa txeu koza e “encontra” se pessoa ness processo. O Diabo de cada dia eh um filme complexo, cheio de personagens interessantes eh k te gira a volta de noj jovem protagonista, e onde k linha pa separa amor, fé, e paranoia, eh quase inexistente. Tude ej 2 film eh de época, cheios de drama e um bokedin de mistério. No tem um elenco de atores supertalentosos, e Netflix te mostra maj um vez kel k te na brincadeira k sej produções. Ej filme te vale a pena, por iss ba oiaj e depois bo bem uvi ess episodio. Bom sessão!

La recherche avance concernant la maladie pour trouver un traitement, de nouveaux médicaments mais aussi pour comprendre d'où vient cette maladie et comment l'éviter au maximum en comprenant quels facteurs peuvent être aggravants

No episódio de hoje você vai conhecer a coleção especial da Biblioteca Radiofônica Tude de Souza, criada pela rádio MEC e especializada na área de radialismo.

durée : 00:02:37 - Grand angle - Comment expliquer les cas de cancers pédiatriques à Saint-Rogatien, près de La Rochelle ? Après le signalement de plusieurs cas dans cette commune de près de 2 000 habitants, la communauté d'agglomération a lancé une étude atmosphérique pour trouver l'origine de ces maladies. Les familles sont dans l'attente.

Top 20 signs your small town is getting ready to be exploited in the same manner Ft Lauderdale is. 1. they will make your roads into highways 2. they will start making you pay for parking in new areas 3. they will start dredging more and more of your water ways. 4. you will start not recognize your local law enforcement 5. Cranes and condos will change your skylines 6. you will see personal water craft rental/ boat rental companies 7. Big corporations will start buying your marinas 8. you will start seeing boats that make no sense at all, 3 , 5 engines. Boats that draw more water than your ecosystem can handle 9. sea wall growth that will only benefit development  10. street signs that tell you can not to do. 11. increasing amount of storm drains that drain into your ecosystem. 12. tolerance for pollution in you water ways and parks etc... will change for the worst 13. Condos , condos, condos condos condominiums are the worst thing for your small town. 14. your small local restaurants / Tackle stores and hardware type stores will be replaced by huge companies 15. Traffic will increase to a point where is harshes your TUDE  16. Landscaping companies will over run your neighborhoods and the sound of lawn equipment like mowers will be normal. 17. new neighborhoods will be created in places you thought no one could live  18. your politicians will start coming from cities that have already been exploited 19. your politicians will try to sell you on growth and developement 20. Companies will come in to exploit your resources (example from Ft Lauderdale are cruise lines and water taxis. 42 Learn more about your ad choices. Visit megaphone.fm/adchoices

Tude bai yumi harim long Philipi 3:10, na lukim olsem ol Kristen tu bai i karim hevi-- hevi bilong Krais.

Episódio gravado ao vivo no estúdio na Rádio Comunitária CPA, 105,9 MHz em Cuiabá, Mato Grosso. Dia 12 de Outubro de 2019.TRACKLIST:Dj Snake, Cardi B, Selena Gomez & Ozuna vs. Mc Punjabi - Taki Taki vs. Mundian (Djs From Mars Bootleg)Eptic x Habstrakt - Lazor 3000Skrillex & Wolfgang Gartner - The Devil's DenKillsonik - Je Te VeuxRusko - Woo Boost (Skin Deep Remix)Jauz & Pegboard Nerds - Get On UpEptic - The End (Carnage & Breaux Remix)Jauz x San Holo - OK!Jauz - Feel The Volume (Joyryde 'Stick in Reverse' Mix)Getter & Ghastly - 666! (Getter VIP)Jauz x Crankdat - I Hold StillJauz x Megalodon - Shark AttackDestructo & YG - Party Up NONSENS - SabotageEminem vs. The Prodigy vs. TJR vs. Baauer vs. Nero - Ode To Harlem Bitch Up Without e Tude ON AIR:Rádio Comunitária CPA FM - 105,9 MHz - Cuiabá/MT Sexta, 22h | Sábado, 22h25 - GMT-4 (Horário da Amazônia) www.radiocpafm.amaisouvida.com.br/Rádio Trans BJ - 87,9 MHz - Bom Jardim de Minas/MG Sábado, 20h - GMT-3 (Horário de Brasília) http://radiotransbj.com Rádio FM Tibau - 104.9 MHz - Tibau/RNSábado, 19h - GMT-3 (Horário de Brasília) www.fmtibau.com.brRádio Comunitária Itaquera - 87,5 MHz - São Paulo/SPSábado, 21h | Domingo, 21h - GMT-3 (Horário de Brasília)http://rcitaquera.com.br/Rádio Ipanema Comunitária - 87,9 MHz - Porto Alegre/RSSábado, 21h - GMT-3 (Horário de Brasília) http://www.ipanemacomunitaria.com.brRádio Acácia - 87,9 MHz - Alvorada/RS Domingo, 20h - GMT-3 (Horário de Brasília) http://www.acaciafm.com.br/Beat Top Som Domingo, 05h - GMT-3 (Horário de Brasília) http://beattopsom.com/Rádio Cidade Paraíba Domingo, 18h | Terça, 21h - GMT-3 (Horário de Brasília) http://radiocidadeparaiba.radiostream123.com/Antena Web (Portugal) Quarta, 01h - GMT+1 (Horário da Europa Ocidental) http://www.antenaweb.infoPop Mix Sábado, 15h | Domingo, 14h - GMT-3 (Horário de Brasília) http://popmixradioweb.com/Agente Oficial: Marina Navarro Viagens e Turismo https://www.facebook.com/marinanavarroviagenseturismo

Nowhere Ones Essay 5 September 2019 This is convoluted, but then again so is everything. Fuck. Here is an immediate existential digression. Follow it? Why the fuck not. Maybe go stream of consciousness. That always feels like a cop out. Who fucking knows. The thing with stream of consciousness is that it's the amalgamation of everything one's little pea brain is sorting through. Just because the words come tumbling out doesn't imply a lack of preparation. That's the biggest thing that pisses me off about motherfuckers who can't grasp the complexities of improvisation. Improvisation is the exact OPPOSITE of lack of preparation. It's living one's life constantly in the state of immediate creation. It's just that when improvising the artists shines the artist's spotlight on the shit purging itself from the soul of the vessel-artist. Then again artist as vessel is another hoary cliche. Anything that smacks of "otherness" is annoying. Like there are different "things." Things? Really? Is there ONE thing. Is one infinite. Of course it is, dildo head. As for the Nowhere Ones it's all there. It all fits. I always think of the movie YELLOW SUBMARINE where the psychedelic words spell out "nowhere" then they desperate into "now here." It's there. It's here. Initially this song was called "Nowhere Son" and it kicked off A BRIDE A DAY, the cassette I did between Forgotten Sons and Tude and Doom Cookie. It served as a reset there and it serves as a reset here. A lot of these initial bits are from that period, riffs wise, probably because Andy is drumming and he drummed Love & Hate and Forgotten Sons. It's amazing how much I have stayed on point in terms of large lyrical concepts. Anyhoo, the story continues. This is concurrent with 1993. There the mundanity of existence bumps up against the harsh realities of young adults finding out that fucking up has consequences. Here though? Pure fantasy, baby, and yes I say "baby" too. It's not that there are no consequences in THE SAGA OF REMOTE CONTROL as much as it's an attempt to apply improvisational techniques to long form storytelling and seeing where the story goes. There is an outline of 30 something records for THE SAGA OF REMOTE CONTROL. That's the backdrop. That's the fabric of existence. That's the land upon which we stand as we set forth into by the minute story telling recreated in a studio and brought to YOU, you brilliant motherfucker. I have to give all due props to Matt Besser and his podcast IMPROV4HUMANS. They make it up, duh, with even less preparation than my absolute holy grail of improv podcasts Scott Aukerman's motherfucking brilliant COMEDY BAND BANG. I bring up Besser, though, because I consider him a peer simply in that we're the same age and grew up punk as fuck. Of course he fulfilled his artistic dreams and I'm still slogging through. When he has on musical guests, mostly alt-country (natch), he asks what a certain lyric meant. I imagine he's asking me about a certain lyric from, say, Meltdown Shuffle from ACT 9 ATLANTIS and replying along the lines of "I'm really not sure what it means. It was just improvised in the larger story, like when you guys make shit up. Later you can go back and figure it out. In the moment it was stream of consciousness - in so much that every thought is stream of consciousness." I've quoted it a million times because it's perfection: "turn off your minds relax and float downstream." "Nowhere Ones" is an attempt to bring lonesomeness into a universal realm, to try to include all the people who feel out of focus and invite them all to the party. To me that was always the great promise of rock and roll. Everyone is invited and everyone is accepted. That's pretty much a good way to approach existence. At any rate, friend, 7.

1993 Essay May 2, 2019 When I was in my twenties I decided to conduct an experiment meant to test randomness and if randomness led to any noticeable patterns. I took all of my t-shirts and threw them into a gigantic pile in the middle of the cedar closet at my Mom's house. She was gracious enough to let me stay there after I stopped going to college. Every day I would close my eyes and root around the pile of literally hundreds of shirts and that'd be my shirt for the day. Once at a party my random shirt happened to be an old hospital shirt. A friend said something along the lines of "look at Tude. Most people go to the hospital and wear a shirt out. When they get home they throw it away or use it as a rag. Tude wears it to a party." That still gives me a chuckle.  What did I learn? Randomness is random. It led down a deconstructionist path that was essential in putting together the pieces for the never ending opera. Everything is arbitrary if you go back far enough. When I was a kid I read rock and roll biographies. Dave Marsh was my favorite. Later Lester Bangs was a god to me. Leg's McNeil writing for Spin was a golden age of magazine journalism. But I realized eventually, tracing the music I love back further and further, that rock and roll itself was a lie shouted by narcissistic Baby Boomers who had the good fortune of never having to face down an existential threat to their comfort. The 'Nam draftees  are not included in my vitriol. They faced two enemies, Ho Chi Minn and Nixon. Hah! Where was I? Rock and roll was, is, and always will be a lie. The fact of the matter is that it's the same stuff that folk musicians had been doing for millennia. It wasn't special. Nothing is special. When you are born is arbitrary. The music of your youth is not special. You are not special. What's this got to do with the song 1993? Wouldn't YOU like to know! I'll tell you. Remember a while back when the Hubble telescope was pointed at empty space and eventually it photographed a gazillion galaxies? That's the existential angst of arbitrary randomness right there. I fixed point in time and space, unassuming, nothing special about it (just like you) and yet, focus on it for an instant and it's the most spectacular thing ever in the cosmos. Just a tiny instant of focus and that specific reality is transformed, nothing into everything. Did it lose it's tag of nothingness when the discovery of everything was made? Does the discovery define that point in space? Did it even exist before the Hubble pointed at it? Deconstruct it further. To paraphrase Sam Kinison "we've hit another vein, mine deeper."  1993 is an arbitrary year picked at random with the specific idea of deconstructing it month by month and season by season to see what stories are told. The song birthed the concept with this'n. I wrote it for Doom Cookie. As a matter of fact the only reason this entry into the Never Ending Opera isn't under the name of Doom Cookie is that I made Brian promise that he would never let me stray from the Society Fringe Player name with future projects. He said it was smarter to be like my buddy Andrew Grimm, aka June Star, and keep the name forever whilst changing up the players. Musically this song, through Paul's mixing, really accentuates the riff. In me pea-brain I always heard a fiddle playing the riff. I even borrowed one with the intent that I'd learn it enough to play the part when we recorded it but ALAS nyet! I really want to hammer home the arbitrary underpinnings of all existence. It's arbitrary where you are born. It's arbitrary to what nation you owe allegiance. It's arbitrary which god was foisted upon you as a child. It's arbitrary if you dig your own gender. It's arbitrary if you get cancer. It's arbitrary if you have fun playing the guitar. Nothing is according to any plan. Keep deconstructing everything, eventually you'll get to a point of vacant nothingness and in a moment of mental anti-obliteration you'll realize that the entire everything was there the whole fucking time.

In conversation with Gene Seymour, contributor to The Nation and former film critic and jazz columnist for Newsday. He has written for Bookforum, CNN.com, and The Washington Post. Author and spoken-word artist Darius James's 1992 masterpiece, the William S. Burroughs meets Thomas Pynchon meets Ishmael Reed fever-dream Negrophobia, is a raunchy, raucous, headlong dive into the many faces of American racism. With other works including That's Blaxploitation: Roots of the Baadassssss 'Tude, Voodoo Stew, and Froggy Chocolate's Christmas Eve, James is the cowriter and narrator of the of 2013 film The United States of Hoodoo. With a new introduction by film scholar Amy Abugo Ongiri and a new preface by the author, the multi-genre Negrophobia is dire, darkly comic, and more relevant than ever. (recorded 3/12/2019)

Praying with a “Tude”John 15; Revelation 3February 17, 2019 MVCIntroduction:A. Dear Lord, So far, today I’ve done all right. I haven’t gossiped, lusted, lost mytemper, haven’t been greedy, grumpy, nasty, selfish, or over-indulgent. I’m verythankful for that. But in a few minutes, Lord, I’m going to get out of bed. Fromthen on as I face the world, the devil and my flesh, I desperately need you to do amiracle of not letting my flesh control me but your Spirit. In Jesus Name, Amen.B. Let me ask you – Is that your attitude when you go to prayer – a humble desperatedependence upon God?1. Is this the disposition of our hearts? Is this the posture of the heart?2. When we do not have this attitude, it becomes one of the main reasons “whywe do not pray!”C. Attitudes are “heart things”. Often we are not even aware of our attitude. But it iswhat drives our prayer life and makes it either a hot prayer life or a lukewarmprayer life or even one that is nonexistent!• Do you know what attitude is driving your prayer life? First, let’s take a look at the…I. The “Tude” of a Hot Prayer Life – humble desperationA. We see the need for this attitude revealed in the teachings of Jesus in John 15.1. This a parable about the vine and branches, Jesus is the vine and we believersare the branches.2. We learn here and from the agricultural world that the vine is the source oflife and the branch is for the purpose of holding the fruit the vine produces.a) Jesus taught that a branch cannot bear fruit of itself apart from the vine.Read v4b) He also taught that apart from Him they cannot bear fruit.(1) Read v5(2) What is true of the vine and branches is true of our relationshipwith Jesusc) Then we learn in v8 that God is glorified when we bear much fruit!3. By the way, fruit is more of Jesus in our life!a) A grape vine produces grapes so a Jesus vine produces Jesus.b) The fruit is more and more of Jesus in our life, character, attitudes,thinking and in our ministry to others so that it is Jesus working throughus Bringing People to Jesus and Helping Believers Become more likeJesus!4. Anybody here feel the need more of Jesus in their life? Marriage, parenting,job, school, character, tough times, big decisions, ministry to others, etc.?5. Then he said in v7 that what they cannot do for themselves God would do forthem in the context of prayer. Read v7.B. Jesus was telling his disciples that they were in an impossible, hopeless,unattainable, desperate situation. They were called to bear much fruit but theywere unable, “can - speaks of ability” apart from Him!1. This is the heart of the Christian life. The true Biblical Christian life is notdifficult to do, it is impossible.2. What God asks of us is beyond man’s ability. No matter how hard you try orto figure it out what God asks of us is bigger than we are strong and smarterthan we are smart on our own!3. Fruit bearing is a work of God not manC. Humility is the disposition of heart that recognizes that all is of and from God andnothing is of or from self!• Jesus even said that He does nothing “of” Himself. He does not do it of Hisown initiative, but rather it is the Father doing it in and through Him.1. Humility is recognizing that God is the source, He is the cause, He is thereason, all of my Christian life and ministry is of and from Him and not of orfrom myself.D. When we fully grasp this with our hearts, not just our minds, we cannot help butbe desperate and humble, “God, I cannot pull off what you want me to do, I needyou to do this!”1. When we have this attitude, we cannot help but pray!2. Prayer that is fervent – (on fire and intense), focused - not a wandering mind,and full of faith and finally prayer from your heart rather than recited orformal prayers!3. On the one hand, it recognizes that apart from Jesus it is impossible to be anddo what God asks us to be and do. On the other hand, it recognizes that Jesusdoes in and through us, what God asks us to be and do.4. I saw a saying that said this – “May I never forget that on my best day I stillneed God as desperately as I did on my worst day!”• The natural response of a heart like this is to call out to Jesus because God does forus, through prayer, what we cannot do for ourselves. Now let’s take a look at the…II. “Tude” of a Lukewarm Prayer Life. – contentment/self sufficiencyA. By lukewarm I do not mean that there is no prayer in that person’s life but rather Imean a prayer life that has no fire and intensity to it. They pray but their mind isalways wandering, there is no faith and it feels like they are just speaking tothemselves. It is more duty and responsibility than a humble desperation.B. Let me say this “It is possible to have the right theology about prayer and evenhumility, but a wrong attitude in your heart”1. That is when our heads and our hearts have not been wired together by theSpirit of God.2. Right theology does not produce a hot prayer life!3. The need is for a heart surgery performed by the Holy Spirit of God.C. Turn to Revelation 3 where we see this kind of heart.1. In this passage, we see in v15-17 the condition of the church; in v18-19Jesus’ counsel to the church; in v20 Jesus’ call to the church.2. Note in v14 that this passage is written to the church, a group of believers.D. V 15-17 reveals their condition of self-sufficiency, a condition that blinded themto their spiritual poverty.1. He starts by saying they are lukewarm. Read v15-16.2. In v17, he gives us a further glimpse into this condition. Read v17a) They had a mixture of material wealth and spiritual poverty.b) Their basic attitude was that “I have need of nothing” self-sufficiency;just the opposite of the humble desperation that says, “I can do nothing.”One says, “I can do nothing” the other says, “I have need of nothing.”One says, “God, I need you for this” the other says, “I can handle this”c) Jesus says there is a spiritual deception going on. “You do not know”that you are spiritually in deep trouble.3. Doesn’t this sound like the modern church in North America and like manyof us? On the outside and by North American standards things look great butthe way God sees it can be a completely different thing!a) We want to see God do miraculous things like we hear He does at aplace like the Brooklyn Tabernacle where drug addicts, prostitutes, andgang member’s lives are turned upside down by Jesus and marriages arerestored and families healed!b) They do not have the resources there like we do in the suburbs so theirfirst resort is prayer to God! We go to prayer as a last resort as we say,“I guess all we can do now is pray”c) We are just as desperate for God in the suburbs as they are in the middleof Brooklyn, New York or Chicago, IL. Yes, right here in the suburbs,we have our addicts to drugs, drink and porn; we have our troubledmarriages and wayward kids who are not walking with the Lord. Wehave habits, hurts and hang-ups we cannot shake; we have the “ds” -depression, death, divorce, divisions, diseases and dollar strugglesdemons, on and on.d) We are lulled to sleep and deceived by the “resources” we have (money,credit cards, contacts, education, experts, fancy vacations, etc.) that weare trusting in to fix these problems, things that can only superficiallyand temporarily fix us! We need Jesus just as desperately as those in thecity do for these problems to find the deep, transformational, andpermanent healing only Jesus can give do!E. Listen to Jesus’ counsel regarding this situation.1. Read v18 - Come to mea) Buy the true riches, not material but the spiritual riches of God.b) Allow Jesus to change your soiled life and put a clean garment on you.c) You need spiritual medication for your eyes. You have been blind. Youneed the healing of your spiritual eyes that only Jesus can give. Youneed to see yourself, your situation and your God as they really are.2. You see in God’s kingdom you do not buy things from Him with money.God’s currency is faith. The entrance door into “God’s market” to get ourspiritual clothing and medicine is prayer.a) Listen to Isa 64:7 - “There is no one who calls on Thy name, whoarouses himself to take hold of Thee.”b) Prayer is the means by which we take hold of God. We put a hand onHim and a hand on our hearts and circumstances so God transforms us.3. Read v19 - Be zealous and repent. If your heart is being confronted today bywhat I am saying, it is because Jesus loves you. Whom He loves Hereproves.a) Zealous - be hot, be ferventb) Repent - change of mind, heart and deeds.F. We have seen that our prayer life reveals our heart attitude. If it is a lukewarmprayer life then we have an attitude of self-sufficiency.1. The key to a hot prayer life is not to commit or try to pray more or changeyour prayer habits. The key is to change your heart, to change your attitude.Then a hot prayer life will be the fruit of a heart of humble desperation.2. Jesus is calling us this morning to repent of a heart attitude of selfsufficiency.G. Listen to the call. Read v201. Remember this verse was written to Christians who have a self-sufficientattitude.2. The key to this is the eye salve that Jesus offers!3. The picture that Jesus gives us is that self-sufficiency in the church and thelife of a believer puts Jesus on the outside, longing to come in and share lifewith you on a moment-by-moment basis.H. Invite and pray.

Dr. Thomas Immel is Assistant Research Physicist at SSL at UC Berkeley. His expertise is interpretation of remote-sensing data and modeling of physical processes in the upper atmosphere & ionosphere. His work includes UV imaging observations from 4 NASA missions. ICON.TranscriptSpeaker 1: Spectrum's next. Speaker 2: Okay. [inaudible]. Speaker 1: Welcome to spectrum the science and technology show on k a l x Berkeley, a biweekly 30 minute program bringing you interviews [00:00:30] featuring bay area scientists and technologists as well as a calendar of local events and news. Speaker 3: Good afternoon. My name is Brad Swift. I'm the host of today's show. Today's interview is part one of two interviews with Thomas Emmel and assistant research physicist at the space sciences laboratory at UC Berkeley. In April, 2013 NASA selected the Ayana spheric connection explorer or icon to be the next Helio physics [00:01:00] explorer satellite mission. The icon mission is to be led by the space sciences laboratory at UC Berkeley. Thomas Emal is the principal investigator of the icon mission icon will provide NASA's heliophysics division with a powerful new capability to determine the conditions in space modified by weather on earth and to understand the way space weather events grow to envelop regions of our planet with dense ionospheric plasma. In today's interview, Dr Emel talks [00:01:30] about Helio physics, the space sciences lab, and small cube sets, which are small satellites being built at universities. Here's that interview, Thomas Ml. Welcome to spectrum. Speaker 4: Thank you. Brad, would you give us a short description of heliophysics? Sure. Here's your physics is sort of a new term and it's used at NASA to describe in shorthand the disciplines of solar and space physics. [00:02:00] Together. It's a little controversial because it means solar physics, obviously space physicists and people who studied the upper atmosphere have sort of felt the shift with changing it to solar physics. A lot of focus went to solar physics. I think icon is icon. Our mission that talking about today is shows a, another view of heliophysics or another focus. Can you describe starting at the earth's surface, the concentric layers of the atmosphere and out to [00:02:30] the ionosphere and beyond? Sure, and how do you define a layer of the atmosphere is sort of where you start. What's the answer? The answer is we defined layers of the atmosphere by their temperature profile or how the temperature changes with altitude. Speaker 4: It's as simple as that and so there are specific layers that on average have a temperature profile, one direction or the other. That means as you go up in altitude, does the temperature drop or increase as you leave the surface of the planet and go up and you're [00:03:00] in the troposphere and as you go higher in altitude, the temperature drops. And that has to do with just basic atmospheric physics. And also the fact that the surface of the planet is what absorbs most of the solar radiation. So it's hot and as you move away from that in an atmosphere that gets thinner without the Tude, the temperature drops. So you go all the way up to the top of the troposphere and you end up with the tropopause. So there's fears and pauses and once you cross the tropopause, you're in the stratosphere, [00:03:30] you know the next sphere and there you've know you've crossed it because temperature start to increase with altitude. Speaker 4: And they increased because of the fact that solar radiation is being actively absorbed in that region of space. That's not happening in the troposphere. The troposphere is transparent of visible light, but the stratosphere is starting to absorb solar radiation that is harmful to life, UV. And so the heating that occurs, the ozone that's in the stratosphere absorbs that [00:04:00] radiation and basically cause the cause of that place being much warmer. So when you're in the stratosphere though, you've already above about 90% of the atmosphere. It's all on a troposphere the stuff we breathe. So the stratosphere warms up all the way to the top. You hit the strata pause and then things turn around again. The chemistry that supports ozone does not work in the mesosphere and so you end up starting to drop in temperature again. So just like in the troposphere, the base of the mesosphere is the warm [00:04:30] straddle pause and it gets cold from that point. Speaker 4: And the coldest place in the vicinity of earth is the top of the menopause where those temperatures have been dropping all the way up to the boundary of space up to about 95 kilometers. At that point, you've reached just about the boundary of space and the temperatures turn around again and and warm all the way up into your in space and the, the atmosphere that's left up there, it's called the thermosphere because it's very hot and it's hot again because it's absorbing a different region [00:05:00] of solar radiation, extreme on fire ultraviolet. So again, protecting life on the earth as part of our atmosphere does that in a number of ways. So the thermosphere in that case is also where we find the ionosphere. The thermosphere is hot because the solar radiation is very energetic at that altitude. So energetic that ionizes the gas and that's where you find the ionosphere, you find a layer of plasma density, so ions and electrons [00:05:30] living together in the same place as plasma and that plasma becomes very dense, about 200 to 300 kilometers above the earth. Speaker 4: That's the dentist plasma between here in the sun. It's why you can hear at night radio tear ran from your ham radio set up if people still do that anymore because you're bouncing radio waves off of that and it's why you can hear, you know, I am stations over a long distance too in the daytime, but it's at night. That layer is all by itself hanging around and you can bounce [00:06:00] radio signals off of it. So then you keep going into space and the plasma density is actually dropped, but you are protected still. You don't enter into interplanetary space until you get out of the magnetosphere. And that's where Earth's magnetic field controls the motion of the plasma. And this is all the way out to 30,000 kilometers. And then you hit the bow shock and the end of the magnetosphere at the magneto pause. Everything has to end and you end up in the solar wind. Speaker 4: And that's interplanetary [00:06:30] space to interstellar space. And interplanetary space are two different things. We've never been to interstellar space. We're working on that. Voyager is on its way and there's a constant argument over whether or not it's out there. So the sun constitutes the helio sphere. It constructs the heliosphere by its energy and blowing out, and that's the sphere around our planetary system that we're part of. That's right. And that's where voyagers headed out of. Right, right out of the heliosphere. It's leaving and it's not coming back. [00:07:00] And I forget what star it's headed off to. So Helio physics is the study of plasmas and space plasmas and how they interact with bodies, uh, and interact with important things such as planetary atmospheres. Basically anywhere our star is an influence that can influence the processes that occur there. Speaker 3: Our guest today is Thomas Animal. In the next segment, Thomas Talks about heliophysics discoveries. [00:07:30] This is KALX Berkley. And what have been the big revelation trends Speaker 4: in heliophysics? Well, the first discovery and Helio physics was the fact that we had radiation belts. It was our first forays into space carried instrumentation. And the first few explorers, which we're still part of that line icon mission, is part of the explore line. But the first ones carried Geiger counters out of University of Iowa where Jim van Allen was in [00:08:00] charge of that department. And where they built those uh, experiments that discovered what we call the van Allen belts now. So that was the first discovery was that we had an environment around us in space that was hazardous and we didn't know where that radiation came from. It fill a Geiger counter just to see what was there. And when you found us a lot more radiation than they thought. The solar cycle has influences throughout the heliosphere. A solar storm for instance, can launch a coronal mass ejection. Speaker 4: They say these are the words [00:08:30] that are starting to show up in the common discussion of space, whether it was coronal mass ejections had come with a solar flare and we've timed these things. We see a coronal mass ejection, a very large one cause a massive magnetic storm at earth. And a good time later it flies by voyage here and it hits the heliopause and radio waves are admitted from the helio pause, the boundary of interstellar space and voyager picks them up. And those were some of the first studies of void. You're trying to figure out how close [00:09:00] it was to the heliopause. Where we are now in the past 10 years is what we understand more now than ever. That the forcing of plasma in near a space is controlled to a much larger degree than we ever suspected or dare to think or dare to discuss. Speaker 4: Really it's controlled by conditions in the lower atmosphere and that the atmospheric layers that we've talked about and talked to all the temperature variations that occur, there's processes that carry energy and momentum beyond past [00:09:30] all those pauses and layers straight from the surface to space. And it's actually biggest discovery in Helio physics in the last decade is that this coupling of the terrestrial atmosphere to spaces stronger than we thought. And what is your focus at the space sciences lab? Well, it has been in the upper atmosphere, in the atmosphere, looking at how solar wind energy propagates through the system. Solar Wind, [00:10:00] it impacts or it effects the MAG Nitas fear and the number of ways creates a shape, stretches it out. The magnetosphere is what processes also learned energy that produces the Aurora. The Aurora is energized by the solar wind. All that energy has to get through the magnetosphere and then down into our atmosphere in a number of ways. Speaker 4: So we're interested in how that energy propagates through the system and how it's eventually deposited in our atmosphere. And then also how our atmosphere and the [inaudible] sphere as you energize them and [00:10:30] make them more conductive through ionization by Aurora, how it feeds back through the system. So magnetosphere occurrence is a current system, electrical current that heats the atmosphere and how you turn that current on and off during a magnetic storm. The timing and how processes work together as sort of as an engineering problem is something I've been focused on for the past 10 years. That's changed over the years too. I've been sliding to lower latitudes where the plasma density is actually highest [00:11:00] and it's highest for two reasons. One because the sun is overhead more often at low latitudes and I NYSE in the atmosphere more actively or more strongly, but also because there's magnetic field tends to trap the plasma at low latitudes. Speaker 4: And when I say that the plasma is densest in the atmosphere between here in the sun, it's actually the low latitude ionosphere which has the dense plasma that interacts most strongly with the earth's atmosphere. Um, and we know now that the [00:11:30] energy and momentum that propagates up from the lower atmosphere that a lot of that energy is coming up from low latitudes as well. Cause that's where a lot of the energy goes in and tropical rainforest and in the tropical weather systems that curved from day to day with interesting periodicities. The reason you end up with large coupling from the little atmosphere to the upper atmosphere is because the atmosphere can be caused to move a wave like manner and we call it a tide, just like tides in the ocean. The atmosphere tends to have some [00:12:00] 12 hour, 24 hour period of city. Say you have a planet with the Brazilian rainforest on it and that fires up at two in the afternoon every day, day after day you start moving the atmosphere in a periodic manner and you end up growing these really, really large waves in the atmosphere that propagate up into space. Speaker 4: And so it's the combination of the tropical forcing and the tropical ion sphere, which is dense and captured by the magnetic field really creates this interesting environment and we're a great laboratory [00:12:30] for understanding atmosphere, space coupling. Speaker 3: Yeah. Listening to spectrum, I am k a l x Berkeley. Our guest today is Thomas Emma. In the next segment he talks about solar energy interacting with Earth's magnetosphere,Speaker 4: the Aurora [inaudible]. Can you just describe the Aurora for us? The Aurora is a feature of the planet [00:13:00] at high latitudes in the north and the south, the Aurora Borealis of North Aurora Australis down south. What it is, it is light coming from the energization of our atmosphere by space plasma. The Sun obviously has a lot of energy and solar atmosphere is constantly moving out and it's carrying a lot of energy with it. But so that energy arrives at earth as solar plasma blowing past the planet. So those are the energies we're talking about. The magnetosphere as sort of a, [00:13:30] it energizes all of the solar wind particles to higher energies and dumps them into our atmosphere. And the Aurora is what you see when you go out on your deck and Alaska and look up. It's the signature of that process occurring. And when the Aurora's very active, that means that process is very active and there's a lot of energy coming into our atmosphere from the solar wind. Speaker 4: What's great is a Nikon camera has great red response, so you can point your camera to the sky and you can put it to a two second exposure and it will see things [00:14:00] that you can't see with your eyes. Many people now have great auroral imagers in their mitts. They may not even know that they've got that capability. So the waves that are created around the equator in the low latitudes, in thinking about waves on the ocean, they're moving in a specific direction. Are these waves also moving in the specific direction? Are they sort of emanating everywhere? And that's a good question. So the really large scale waves in [00:14:30] the atmosphere, the first thing is to realize that once you've got a wave moving in the atmosphere, there's nothing really to stop it. The waves aren't going to crash on the shore somewhere. They're going to go up and they're going to grow with altitude, their waves, storms derive, and I am talking about the large scale continental scale waves that the wavelength is as large as a continent, at least horizontally, vertically. Speaker 4: There's about 2030 kilometers, but 2030 kilometers is a quarter or a third of the way to space. So they're still large even [00:15:00] though 2030 kilometers doesn't sound that far. In any case, those waves grow with altitude and by the time you get to the edge of space, a wave that might have had a half degree centigrade or Celsius variability to it in amplitude, by the time it gets to the boundary of space and crosses it, it can have an amplitude of 20 or 30 degrees Kelvin or our Celsius. It's the same thing. Uh, it's one way to measure the size of that wave. With that wave also comes a large wind component. The winds, the [00:15:30] motion of the atmosphere is going to go with it. It's this sloshing and the temperature comes from the compression and the expansion of the gas. As the wave moves around the planet, do they go in different directions? Speaker 4: Yeah, we talk about them. We see there's a number of technical terms for the waves. There's eastward and westward traveling waves and some of them are larger than others. This atmosphere supports a couple of waves eastward at a couple of ways, westward more than others. Some of these waves are excited [00:16:00] more naturally than others just because of the source of the excitation, the source of the excitation of the continents. If you look at a map of the earth where lightning occurs on earth, for instance, it's always over the continents because the solar energy is really just being deposited right there at the surface and the atmosphere starts to be put in a motion and the water vapor starts to condense. As the atmosphere rises and you get storms, a tropical rainforest and Africa, tropical rainforests in South America and also a third really large [00:16:30] region of tropical forcing to Southeast Asia. Speaker 4: Those three places on the earth firing off two in the afternoon in the South East Asia than two in the afternoon, Africa, then South American and do that over again every day. It's like a drum head problem, if you know what I mean. If you put a little sand on a drum and you start tapping it in one position, you can form a pattern. You would see where else you could tap it at the same time to reinforce that pattern. Now the rainy seasons of of those different places changes throughout the year. [00:17:00] That's one of the reasons we know it's from the lower atmosphere because we've observed conditions in space that changed with the rainy seasons and there's no reason to have rainy seasons in space. But we do and so we look immediately to where we do have a rainy season, which is in the troposphere. And so the recent developments and numerical model supports the idea that there's a strong connection between the tropic sun conditions and space. Speaker 4: Have you been involved in a lot of past satellite projects at the space science lab or a few [00:17:30] of them? I've been involved in too. Recently icon, which I'm leading and a small satellite re recently completed a flue called cinema that was a student led cubes hat, so a 10 by 10 by 30 centimeter satellite that we built at the lab designed and built. Before that I was analyzing data. I've been spending 10 years analyzing data from missions that we've supported or built and so combining data from a number of [00:18:00] different instruments that space sciences lab has built or satellites that space sciences lab has built. It's been something I've done at the lab, but this is my first time leading a mission. Speaker 5: This is k a l x Berkeley. The show is spectrum. Our guest is Thomas Emma, a physicist at UC Berkeley's space sciences lab. Speaker 4: How has the [00:18:30] cube sat changed the way satellite measurements are made? Well, in some respects that remains to be seen. There's been a number of advances in the capabilities that cubes hats can carry in terms of pointing and power and the instruments have all had to shrink in size as well. But there's a number of capabilities that have grown over the years that allow us to do that. Cell phones have been a big driver and shrinking small processors and getting [00:19:00] into low power processors and communications gear as well. And what's been nice is working with the students here at Berkeley actually. They've had a lot of experience in designing and programming processors for the purposes that we need to fly in space. So there's a number of universities working in this area now and I think they're just getting better. Cinema has been a good experiment for us. Speaker 4: We have four of them in the works this year. There's two Korean cinema. It's going up. [00:19:30] Kate, you young, he university was our partner. There's a lot of interest in supporting keeps that launches at NASA and throughout different government agencies and so you know, we went on a national reconnaissance vehicle, but a, it didn't cost us much. It was fantastic that we had that opportunity and NASA has worked with NRO and other agencies to make this possible for universities to do these. There were a number of university keeps that's on that launch. So these cubes hats that NASA embraces, I guess [00:20:00] that's the only way to get up is NASA says, yeah, this is worth putting up there, or are there now independent ways to get to space? I think NASA is where we'd like to start and that's who we've gone to before. NSF is really the organization that was the first to support a cube type program per se. Speaker 4: And National Science Foundation doesn't have a launch service, but NASA does. So there was a close collaboration early on and some key individuals at NASA Kennedy have taken a remarkable interest [00:20:30] in fostering that program and develop basically what they call a educational launch. Alana was, uh, is the acronym that we went on. Alana. Alana supports a number of, keeps getting into space. You propose to Atlanta, NSF sends them $20,000 or that's it was for us and you get your slot and you get your orbit and you're on orbit for many years. So it's really a great opportunity. So right now it's really good to work with NASA on this, on the cinema [00:21:00] projects. There's quite a bit of student involvement in those. I understand. Can you talk about that? Right. So National Science Foundation supported Space Sciences Labs, cinema project, which is a cube set for high ions, magnetic fields, c I n electrons, it went on it. Speaker 4: It's a great acronym for a very tough thing, but it's a base whether mission, it's to measure the particle environment in space and the magnetic fields. So that was great. You know, we [00:21:30] miss dearly, Bob Lynne, who was the former head of space sciences lab for more than a decade and the principal investigator on one of our explorers Hesi and the principal investigator on cinema, he put that international team together between CUNY University where he was an adjunct professor. We worked with imperial college as well on that mission and they provided the smallest magnetometer have ever seen for a space instrument. It was a high quality, high precision magnetometer, way better than even your iPhone if you can imagine. Also [00:22:00] we had a detector group at LBL and a group providing an electronic part and aces from France. So it was an unbelievable confluence of people and scientific interests that built cinema. Speaker 4: The student aspect was, there were students, uh, from the start in mechanical engineering who really came up with the initial design of a cube sat and it was a couple of masters students, one of whom is still a space sciences lab, David Glaser. And it was great working with the Mechanical Engineering Department [00:22:30] because it was that department of which took the controls problem of how you spin a spacecraft based on inputs from space, the Sun Sensor, we had the magnetometer measurements that you're making. So that was a remarkable achievement. I thought on the mechanical engineering side and working with the electrical engineers, we had a number of cs IEC students as well and really had a good team. They're working on interfacing with the mechanical engineering students who were working on the attitude control or working [00:23:00] with the imperial college students and researchers who were providing magnetometer those a number of difficult tasks that we had some great students come through and everyone got their chance to save cinema. It was a seat of your pants operation. The thing flew and it's functional. We are going to fly the next one with some updates that's gonna work better, so we need more students. The wonderful problem with students is that they graduate to go onto great careers and other places and so we'd like to have those people back. They're not coming [00:23:30] back, so we need to get a new crop of ex students and mechanical engineers and we'll probably be flyering at soda again. Speaker 5: That concludes part one of our two part interview with Thomas Emmylou. Part two will air on 14 in that interview, Dr Hamill discusses icon mission process start to finish. The icon explorer mission website is icon dot s s l. Dot. berkeley.edu [00:24:00] now a few of the science and technology events happening locally over the next two weeks. Rick Karnofsky and Renee route Speaker 6: present the calendar this Tuesday, June 4th the San Francisco ASCA scientists lecture series. We'll be hosting a talk by two sides. Officers at the California Institute for Regenerative Medicine. You Know Greg Shamor and Kevin Wilson will speak about the potential of stem cell research to help in diseases such as diabetes, spinal cord injury, [00:24:30] heart night disease, and neurological disorders. They will also address the recent restrictions on research and where it is heading today. This June 4th event will be held that the Soma Street food park in San Francisco, the city's first permanent food truck pod. It will begin at 7:00 PM biological anthropologist, Helen Fisher of Rutgers. We'll speak with KQ eds, Michael Krasney about the science of love and attraction. On Tuesday, June 4th [00:25:00] at 7:30 PM at the North Theater in San Francisco, Fisher has written five books on the evolution and future of human sexuality, monogamy, adultery, and divorce, gender differences in the brain, the chemistry of romantic love and human personality types. Speaker 6: And why are we fall in love with one person rather than another? Tickets start at $20 and are available at cal academy. Dot. O. R. G. On Monday, June 10th Brian Day [00:25:30] deleted Lunar Science Institute director at NASA will give a talk about the latest lunar discoveries as litter robotics continue to advance. Our understanding of the moon continues to change. Well, the lunar surface has been previously viewed as a static desert environment. New evidence points to a far more dynamic moonscape than expected. Dr. David will discuss these new discoveries and elaborate on some of NASA's more recent and lunar exploration missions. The event will be held on Monday, June 10th at 7:30 PM in the California [00:26:00] Academy of Sciences. Planetarium. Tuesday we have tickets for the event. Visit the Academy website@calacademy.org the Computer History Museum at 1401 north shoreline boulevard in mountain view is hosting senior vice president and director of IBM Research John Kelly on June 11th at 7:00 PM Museum CEO John Holler, well moderate a conversation with Kelly on topics ranging from his background and the path that led him to IBM. [00:26:30] The history of research there, IBM's Watson and cognitive computing to the newest IBM lab in Nairobi, Kenya. IBM says that Africa is destined to become an important growth market. The company admission is free. register@computerhistory.org Speaker 7: [inaudible]Speaker 6: [00:27:00] spectrum is to present news stories we find interesting. Rick Karnofsky and Renee arou present. The news engineers at UC Berkeley have created a new hydro gel that can be manipulated by exposure to light alone. The team inspired by plant's ability to grow towards light sources [00:27:30] created their gel by combining synthetic elastic proteins with one cell thick sheets of graphite known as graphene. Graphene generates heat when exposed to light, which can cause synthetic proteins to release water. The two materials are combined to form of hydrogen with one side that is more porous than the other. This allows the material to mimic the way plant cells shrink and expand unevenly in response to light. This hydrogen also shrinks and evenly, albeit more precisely allowing to bend and move solely in response [00:28:00] to light. Create or speculate that the shape changing Gel could have applications in drug delivery and tissue engineering. Speaker 6: Mathematician Tang Jang of the University of New Hampshire in Durham published unimportant number theory proof and this week's issue of angels of mathematics. Yang proved a weak form of the twin prime conjecture and as the first to establish the existence of a finite bound four prime gaps. Prime numbers are natural numbers greater [00:28:30] than one that I have no positive divisors other than one and themselves. Interestingly, many come in pairs that have a difference of two for example, three and five 17 and 19 or 101 and 103 Jang showed that for some integer n that is at most 70 million. There are infinitely many pairs of primes that differ by n. Speaker 2: [inaudible]Speaker 5: [00:29:00] spectrum is archive on iTunes university. Our special link is tiny url.com/k a l ex spectrum. The music heard during the show was written and produced by Alex Simon. Thank you for listening to spectrum. If you have comments about the show, please send them to us via email. [00:29:30] Our email address is spectrum dot kalx@yahoo.com join us in two weeks at this same time. [inaudible]. See acast.com/privacy for privacy and opt-out information.