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#solarorbiter — Public Fediverse posts

Live and recent posts from across the Fediverse tagged #solarorbiter, aggregated by home.social.

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  1. NASA's Parker Solar Probe Flew In And Out Of The Solar Corona And Found A Source Of High-Energy Particles That No Existing Model Had Predicted
    (When NASA's Parker Solar Probe passed through the solar corona during perihelion encounters at the heliospheric current sheet, its instruments recorded energetic protons at energies far above what existing models of particle acceleration at that location could account for.)
    --
    spacedaily.com/n-nasas-parker- <-- shared technical article
    --
    doi.org/10.3847/2041-8213/ae3c <-- shared paper
    --
    space.com/high-energy-particle <-- shared technical article
    --
    youtu.be/Woo4yZby4BU?si=rzzND3 <-- shared space weather overview effects video, #AIslop notwithstanding 🙃 🫠 😉
    --
    “… A team… at the Southwest Research Institute… and… the University of Maryland’s Institute for Research in Electronics and Applied Physics has published an analysis of those measurements [link above]…, identifying magnetic reconnection at the heliospheric current sheet as the mechanism responsible. The proton energies detected were, in the study’s framing, approximately a thousand times greater than the available magnetic energy per particle that models of this process had predicted.
    The finding matters for two reasons: it identifies a source of energetic particles close to the Sun that was not anticipated, and it raises questions about how far the existing understanding of reconnection-driven particle acceleration extends…
    The Parker measurements suggest that picture needs revision. The magnetic island merging mechanism [the authors] identif[ied] can evidently produce proton populations at energies that challenge the boundary between what reconnection does and what shock acceleration does. Whether this source can explain a significant fraction of observed near-Earth energetic particle events, or whether it contributes mainly at energies and scales that remain confined close to the Sun, is a question the paper does not yet resolve…
    Solar Orbiter, the European Space Agency mission operating in coordination with Parker, offers complementary measurements at somewhat greater distances. Comparing what the two spacecraft measure of the same particle populations as they propagate outward from the Sun will help establish which features originate close to the source and which are modified by the intervening solar wind. The energetic particle observations that puzzled researchers in the pre-Parker era now have a candidate mechanism. Whether that mechanism accounts for a large or small fraction of what actually reaches Earth remains the open question…”
    #sun #solar #solarsystem #heliosphere #Parker #SolarOrbiter #spacecraft #research #monitoring #instrumentatin #spaceweather #solarflare #coronalmassejection #CME #NASA #ESA #magnetism #geomagnetism #proton #energy #particleacceleration #measurement #solarwind #risk #hazard #impacts #corona #perihelion #model #modeling
    @nasa @esa

  2. NASA's Parker Solar Probe Flew In And Out Of The Solar Corona And Found A Source Of High-Energy Particles That No Existing Model Had Predicted
    (When NASA's Parker Solar Probe passed through the solar corona during perihelion encounters at the heliospheric current sheet, its instruments recorded energetic protons at energies far above what existing models of particle acceleration at that location could account for.)
    --
    spacedaily.com/n-nasas-parker- <-- shared technical article
    --
    doi.org/10.3847/2041-8213/ae3c <-- shared paper
    --
    space.com/high-energy-particle <-- shared technical article
    --
    youtu.be/Woo4yZby4BU?si=rzzND3 <-- shared space weather overview effects video, #AIslop notwithstanding 🙃 🫠 😉
    --
    “… A team… at the Southwest Research Institute… and… the University of Maryland’s Institute for Research in Electronics and Applied Physics has published an analysis of those measurements [link above]…, identifying magnetic reconnection at the heliospheric current sheet as the mechanism responsible. The proton energies detected were, in the study’s framing, approximately a thousand times greater than the available magnetic energy per particle that models of this process had predicted.
    The finding matters for two reasons: it identifies a source of energetic particles close to the Sun that was not anticipated, and it raises questions about how far the existing understanding of reconnection-driven particle acceleration extends…
    The Parker measurements suggest that picture needs revision. The magnetic island merging mechanism [the authors] identif[ied] can evidently produce proton populations at energies that challenge the boundary between what reconnection does and what shock acceleration does. Whether this source can explain a significant fraction of observed near-Earth energetic particle events, or whether it contributes mainly at energies and scales that remain confined close to the Sun, is a question the paper does not yet resolve…
    Solar Orbiter, the European Space Agency mission operating in coordination with Parker, offers complementary measurements at somewhat greater distances. Comparing what the two spacecraft measure of the same particle populations as they propagate outward from the Sun will help establish which features originate close to the source and which are modified by the intervening solar wind. The energetic particle observations that puzzled researchers in the pre-Parker era now have a candidate mechanism. Whether that mechanism accounts for a large or small fraction of what actually reaches Earth remains the open question…”
    #sun #solar #solarsystem #heliosphere #Parker #SolarOrbiter #spacecraft #research #monitoring #instrumentatin #spaceweather #solarflare #coronalmassejection #CME #NASA #ESA #magnetism #geomagnetism #proton #energy #particleacceleration #measurement #solarwind #risk #hazard #impacts #corona #perihelion #model #modeling
    @nasa @esa

  3. NASA's Parker Solar Probe Flew In And Out Of The Solar Corona And Found A Source Of High-Energy Particles That No Existing Model Had Predicted
    (When NASA's Parker Solar Probe passed through the solar corona during perihelion encounters at the heliospheric current sheet, its instruments recorded energetic protons at energies far above what existing models of particle acceleration at that location could account for.)
    --
    spacedaily.com/n-nasas-parker- <-- shared technical article
    --
    doi.org/10.3847/2041-8213/ae3c <-- shared paper
    --
    space.com/high-energy-particle <-- shared technical article
    --
    youtu.be/Woo4yZby4BU?si=rzzND3 <-- shared space weather overview effects video, #AIslop notwithstanding 🙃 🫠 😉
    --
    “… A team… at the Southwest Research Institute… and… the University of Maryland’s Institute for Research in Electronics and Applied Physics has published an analysis of those measurements [link above]…, identifying magnetic reconnection at the heliospheric current sheet as the mechanism responsible. The proton energies detected were, in the study’s framing, approximately a thousand times greater than the available magnetic energy per particle that models of this process had predicted.
    The finding matters for two reasons: it identifies a source of energetic particles close to the Sun that was not anticipated, and it raises questions about how far the existing understanding of reconnection-driven particle acceleration extends…
    The Parker measurements suggest that picture needs revision. The magnetic island merging mechanism [the authors] identif[ied] can evidently produce proton populations at energies that challenge the boundary between what reconnection does and what shock acceleration does. Whether this source can explain a significant fraction of observed near-Earth energetic particle events, or whether it contributes mainly at energies and scales that remain confined close to the Sun, is a question the paper does not yet resolve…
    Solar Orbiter, the European Space Agency mission operating in coordination with Parker, offers complementary measurements at somewhat greater distances. Comparing what the two spacecraft measure of the same particle populations as they propagate outward from the Sun will help establish which features originate close to the source and which are modified by the intervening solar wind. The energetic particle observations that puzzled researchers in the pre-Parker era now have a candidate mechanism. Whether that mechanism accounts for a large or small fraction of what actually reaches Earth remains the open question…”
    #sun #solar #solarsystem #heliosphere #Parker #SolarOrbiter #spacecraft #research #monitoring #instrumentatin #spaceweather #solarflare #coronalmassejection #CME #NASA #ESA #magnetism #geomagnetism #proton #energy #particleacceleration #measurement #solarwind #risk #hazard #impacts #corona #perihelion #model #modeling
    @nasa @esa

  4. NASA's Parker Solar Probe Flew In And Out Of The Solar Corona And Found A Source Of High-Energy Particles That No Existing Model Had Predicted
    (When NASA's Parker Solar Probe passed through the solar corona during perihelion encounters at the heliospheric current sheet, its instruments recorded energetic protons at energies far above what existing models of particle acceleration at that location could account for.)
    --
    spacedaily.com/n-nasas-parker- <-- shared technical article
    --
    doi.org/10.3847/2041-8213/ae3c <-- shared paper
    --
    space.com/high-energy-particle <-- shared technical article
    --
    youtu.be/Woo4yZby4BU?si=rzzND3 <-- shared space weather overview effects video, #AIslop notwithstanding 🙃 🫠 😉
    --
    “… A team… at the Southwest Research Institute… and… the University of Maryland’s Institute for Research in Electronics and Applied Physics has published an analysis of those measurements [link above]…, identifying magnetic reconnection at the heliospheric current sheet as the mechanism responsible. The proton energies detected were, in the study’s framing, approximately a thousand times greater than the available magnetic energy per particle that models of this process had predicted.
    The finding matters for two reasons: it identifies a source of energetic particles close to the Sun that was not anticipated, and it raises questions about how far the existing understanding of reconnection-driven particle acceleration extends…
    The Parker measurements suggest that picture needs revision. The magnetic island merging mechanism [the authors] identif[ied] can evidently produce proton populations at energies that challenge the boundary between what reconnection does and what shock acceleration does. Whether this source can explain a significant fraction of observed near-Earth energetic particle events, or whether it contributes mainly at energies and scales that remain confined close to the Sun, is a question the paper does not yet resolve…
    Solar Orbiter, the European Space Agency mission operating in coordination with Parker, offers complementary measurements at somewhat greater distances. Comparing what the two spacecraft measure of the same particle populations as they propagate outward from the Sun will help establish which features originate close to the source and which are modified by the intervening solar wind. The energetic particle observations that puzzled researchers in the pre-Parker era now have a candidate mechanism. Whether that mechanism accounts for a large or small fraction of what actually reaches Earth remains the open question…”
    #sun #solar #solarsystem #heliosphere #Parker #SolarOrbiter #spacecraft #research #monitoring #instrumentatin #spaceweather #solarflare #coronalmassejection #CME #NASA #ESA #magnetism #geomagnetism #proton #energy #particleacceleration #measurement #solarwind #risk #hazard #impacts #corona #perihelion #model #modeling
    @nasa @esa

  5. NASA's Parker Solar Probe Flew In And Out Of The Solar Corona And Found A Source Of High-Energy Particles That No Existing Model Had Predicted
    (When NASA's Parker Solar Probe passed through the solar corona during perihelion encounters at the heliospheric current sheet, its instruments recorded energetic protons at energies far above what existing models of particle acceleration at that location could account for.)
    --
    spacedaily.com/n-nasas-parker- <-- shared technical article
    --
    doi.org/10.3847/2041-8213/ae3c <-- shared paper
    --
    space.com/high-energy-particle <-- shared technical article
    --
    youtu.be/Woo4yZby4BU?si=rzzND3 <-- shared space weather overview effects video, notwithstanding 🙃 🫠 😉
    --
    “… A team… at the Southwest Research Institute… and… the University of Maryland’s Institute for Research in Electronics and Applied Physics has published an analysis of those measurements [link above]…, identifying magnetic reconnection at the heliospheric current sheet as the mechanism responsible. The proton energies detected were, in the study’s framing, approximately a thousand times greater than the available magnetic energy per particle that models of this process had predicted.
    The finding matters for two reasons: it identifies a source of energetic particles close to the Sun that was not anticipated, and it raises questions about how far the existing understanding of reconnection-driven particle acceleration extends…
    The Parker measurements suggest that picture needs revision. The magnetic island merging mechanism [the authors] identif[ied] can evidently produce proton populations at energies that challenge the boundary between what reconnection does and what shock acceleration does. Whether this source can explain a significant fraction of observed near-Earth energetic particle events, or whether it contributes mainly at energies and scales that remain confined close to the Sun, is a question the paper does not yet resolve…
    Solar Orbiter, the European Space Agency mission operating in coordination with Parker, offers complementary measurements at somewhat greater distances. Comparing what the two spacecraft measure of the same particle populations as they propagate outward from the Sun will help establish which features originate close to the source and which are modified by the intervening solar wind. The energetic particle observations that puzzled researchers in the pre-Parker era now have a candidate mechanism. Whether that mechanism accounts for a large or small fraction of what actually reaches Earth remains the open question…”

    @nasa @esa

  6. #MPS:
    "
    Wenn die Sonne ernst macht

    Die Folgen stürmischen Sonnenwetters: zwischen farbenfrohen Polarlichtern und funkensprühenden Telegrafenmasten
    "
    ".. nicht nur Polarlichter auslösen, sondern auch erhebliche Schäden an technischer Infra-struktur verursachen .."

    mps.mpg.de/8758108/news_public

    16.6.2026

    #Erde #Göttingen #Magnetfeld #Plasma #Polarlichter #Raumfahrt #Raumsonde #SolarOrbiter #Sonne #Sonnensturm #Sonnenwetter #Sonnenzyklus #Sunrise #Viigil #Weltraumwetter

  7. #MPS:
    "
    Wenn die Sonne ernst macht

    Die Folgen stürmischen Sonnenwetters: zwischen farbenfrohen Polarlichtern und funkensprühenden Telegrafenmasten
    "
    ".. nicht nur Polarlichter auslösen, sondern auch erhebliche Schäden an technischer Infra-struktur verursachen .."

    mps.mpg.de/8758108/news_public

    16.6.2026

    #Erde #Göttingen #Magnetfeld #Plasma #Polarlichter #Raumfahrt #Raumsonde #SolarOrbiter #Sonne #Sonnensturm #Sonnenwetter #Sonnenzyklus #Sunrise #Viigil #Weltraumwetter

  8. #MPS:
    "
    Wenn die Sonne ernst macht

    Die Folgen stürmischen Sonnenwetters: zwischen farbenfrohen Polarlichtern und funkensprühenden Telegrafenmasten
    "
    ".. nicht nur Polarlichter auslösen, sondern auch erhebliche Schäden an technischer Infra-struktur verursachen .."

    mps.mpg.de/8758108/news_public

    16.6.2026

    #Erde #Göttingen #Magnetfeld #Plasma #Polarlichter #Raumfahrt #Raumsonde #SolarOrbiter #Sonne #Sonnensturm #Sonnenwetter #Sonnenzyklus #Sunrise #Viigil #Weltraumwetter

  9. #MPS:
    "
    Wenn die Sonne ernst macht

    Die Folgen stürmischen Sonnenwetters: zwischen farbenfrohen Polarlichtern und funkensprühenden Telegrafenmasten
    "
    ".. nicht nur Polarlichter auslösen, sondern auch erhebliche Schäden an technischer Infra-struktur verursachen .."

    mps.mpg.de/8758108/news_public

    16.6.2026

    #Erde #Göttingen #Magnetfeld #Plasma #Polarlichter #Raumfahrt #Raumsonde #SolarOrbiter #Sonne #Sonnensturm #Sonnenwetter #Sonnenzyklus #Sunrise #Viigil #Weltraumwetter

  10. #MPS:
    "
    Wenn die Sonne ernst macht

    Die Folgen stürmischen Sonnenwetters: zwischen farbenfrohen Polarlichtern und funkensprühenden Telegrafenmasten
    "
    ".. nicht nur Polarlichter auslösen, sondern auch erhebliche Schäden an technischer Infra-struktur verursachen .."

    mps.mpg.de/8758108/news_public

    16.6.2026

    #Erde #Göttingen #Magnetfeld #Plasma #Polarlichter #Raumfahrt #Raumsonde #SolarOrbiter #Sonne #Sonnensturm #Sonnenwetter #Sonnenzyklus #Sunrise #Viigil #Weltraumwetter

  11. Sun Suddenly Blasts Powerful Radio Transmission for 19 Continuous Days

    The Sun has broken a new record for continuous radio wave transmissions, blasting a powerful signal four times…
    #NewsBeep #News #US #USA #UnitedStates #UnitedStatesOfAmerica #Space #radioblast #radiowave #Science #SolarOrbiter #Sun
    newsbeep.com/us/663787/

  12. Sun Suddenly Blasts Powerful Radio Transmission for 19 Continuous Days

    The Sun has broken a new record for continuous radio wave transmissions, blasting a powerful signal four times…
    #NewsBeep #News #US #USA #UnitedStates #UnitedStatesOfAmerica #Space #radioblast #radiowave #Science #SolarOrbiter #Sun
    newsbeep.com/us/663787/

  13. Sun Suddenly Blasts Powerful Radio Transmission for 19 Continuous Days

    The Sun has broken a new record for continuous radio wave transmissions, blasting a powerful signal four times…
    #NewsBeep #News #Space #AU #Australia #radioblast #radiowave #Science #SolarOrbiter #Sun
    newsbeep.com/au/693039/

  14. Sun Suddenly Blasts Powerful Radio Transmission for 19 Continuous Days

    The Sun has broken a new record for continuous radio wave transmissions, blasting a powerful signal four times…
    #NewsBeep #News #Space #AU #Australia #radioblast #radiowave #Science #SolarOrbiter #Sun
    newsbeep.com/au/693039/

  15. Sun Suddenly Blasts Powerful Radio Transmission for 19 Continuous Days

    The Sun has broken a new record for continuous radio wave transmissions, blasting a powerful signal four times…
    #NewsBeep #News #Space #radioblast #radiowave #Science #SolarOrbiter #Sun #UK #UnitedKingdom
    newsbeep.com/uk/601953/

  16. A look into the “GREGOR Observations Center” GOC at MPS Göttingen during this month’s remote campaign at the GREGOR Solar Telescope, located on Tenerife. Many great active regions and sunspots, but unfortunately clouds obstructed our view. Hoping for better conditions for our August campaign together with Solar Orbiter 🛰️ 🔭🤞

    #Sun #SolarPhysics #ActiveRegions #Sunspots #GREGORSolarTelescope #SolarOrbiter #MPSGoettingen

  17. A look into the “GREGOR Observations Center” GOC at MPS Göttingen during this month’s remote campaign at the GREGOR Solar Telescope, located on Tenerife. Many great active regions and sunspots, but unfortunately clouds obstructed our view. Hoping for better conditions for our August campaign together with Solar Orbiter 🛰️ 🔭🤞

    #Sun #SolarPhysics #ActiveRegions #Sunspots #GREGORSolarTelescope #SolarOrbiter #MPSGoettingen

  18. A look into the “GREGOR Observations Center” GOC at MPS Göttingen during this month’s remote campaign at the GREGOR Solar Telescope, located on Tenerife. Many great active regions and sunspots, but unfortunately clouds obstructed our view. Hoping for better conditions for our August campaign together with Solar Orbiter 🛰️ 🔭🤞

    #Sun #SolarPhysics #ActiveRegions #Sunspots #GREGORSolarTelescope #SolarOrbiter #MPSGoettingen

  19. A look into the “GREGOR Observations Center” GOC at MPS Göttingen during this month’s remote campaign at the GREGOR Solar Telescope, located on Tenerife. Many great active regions and sunspots, but unfortunately clouds obstructed our view. Hoping for better conditions for our August campaign together with Solar Orbiter 🛰️ 🔭🤞

    #Sun #SolarPhysics #ActiveRegions #Sunspots #GREGORSolarTelescope #SolarOrbiter #MPSGoettingen

  20. A look into the “GREGOR Observations Center” GOC at MPS Göttingen during this month’s remote campaign at the GREGOR Solar Telescope, located on Tenerife. Many great active regions and sunspots, but unfortunately clouds obstructed our view. Hoping for better conditions for our August campaign together with Solar Orbiter 🛰️ 🔭🤞

    #Sun #SolarPhysics #ActiveRegions #Sunspots #GREGORSolarTelescope #SolarOrbiter #MPSGoettingen

  21. A look into the “GREGOR Observations Center” at #mpsgoettingen during this month’s remote campaign at #GREGORSolarTelescope. Many great #activeregions and #sunspots, but unfortunately clouds obstructed our view. Hoping for better conditions for our August campaign together with #SolarOrbiter.

  22. A look into the “GREGOR Observations Center” at #mpsgoettingen during this month’s remote campaign at #GREGORSolarTelescope. Many great #activeregions and #sunspots, but unfortunately clouds obstructed our view. Hoping for better conditions for our August campaign together with #SolarOrbiter.

  23. ☀️ La mission #SolarOrbiter a observé pour la première fois une cascade de reconnexions du champ magnétique dans l’atmosphère solaire. Ces « avalanches magnétiques » pourraient expliquer comment naissent certaines éruptions solaires.

    🔎 cnes.fr/actualites/solar-orbit

  24. ☀️ La mission #SolarOrbiter a observé pour la première fois une cascade de reconnexions du champ magnétique dans l’atmosphère solaire. Ces « avalanches magnétiques » pourraient expliquer comment naissent certaines éruptions solaires.

    🔎 cnes.fr/actualites/solar-orbit

  25. ☀️ La mission #SolarOrbiter a observé pour la première fois une cascade de reconnexions du champ magnétique dans l’atmosphère solaire. Ces « avalanches magnétiques » pourraient expliquer comment naissent certaines éruptions solaires.

    🔎 cnes.fr/actualites/solar-orbit

  26. ☀️ La mission #SolarOrbiter a observé pour la première fois une cascade de reconnexions du champ magnétique dans l’atmosphère solaire. Ces « avalanches magnétiques » pourraient expliquer comment naissent certaines éruptions solaires.

    🔎 cnes.fr/actualites/solar-orbit

  27. ☀️ La mission #SolarOrbiter a observé pour la première fois une cascade de reconnexions du champ magnétique dans l’atmosphère solaire. Ces « avalanches magnétiques » pourraient expliquer comment naissent certaines éruptions solaires.

    🔎 cnes.fr/actualites/solar-orbit

  28. Detalles de la calibración radiométrica del telescopio HRIEUV de la Solar Orbiter. Datos técnicos, rendimiento óptico y resultados del instrumento que observa la corona solar.

    #SolarOrbiter #NASA #ESA #Tutiempo

    tutiempo.net/noticias/solar-or

  29. Detalles de la calibración radiométrica del telescopio HRIEUV de la Solar Orbiter. Datos técnicos, rendimiento óptico y resultados del instrumento que observa la corona solar.

    #SolarOrbiter #NASA #ESA #Tutiempo

    tutiempo.net/noticias/solar-or

  30. Detalles de la calibración radiométrica del telescopio HRIEUV de la Solar Orbiter. Datos técnicos, rendimiento óptico y resultados del instrumento que observa la corona solar.

    #SolarOrbiter #NASA #ESA #Tutiempo

    tutiempo.net/noticias/solar-or

  31. Detalles de la calibración radiométrica del telescopio HRIEUV de la Solar Orbiter. Datos técnicos, rendimiento óptico y resultados del instrumento que observa la corona solar.

    #SolarOrbiter #NASA #ESA #Tutiempo

    tutiempo.net/noticias/solar-or

  32. Detalles de la calibración radiométrica del telescopio HRIEUV de la Solar Orbiter. Datos técnicos, rendimiento óptico y resultados del instrumento que observa la corona solar.

    #SolarOrbiter #NASA #ESA #Tutiempo

    tutiempo.net/noticias/solar-or

  33. In recent years, the #ParkerSolarProbe and #SolarOrbiter probes have delivered a wealth of data about our #Sun, its surface—precisely where the #SolarWind originates. The ubiquitous presence of #plasma jets and magnetic field reversals suggests that a significant portion of the wind forms through dynamic processes involving magnetic #reconnection and transient energy releases.

    This Thursday, Alexis Rouillard will review recent research on the dynamics of the solar wind: irap.omp.eu/event/the-tempestu

  34. In recent years, the #ParkerSolarProbe and #SolarOrbiter probes have delivered a wealth of data about our #Sun, its surface—precisely where the #SolarWind originates. The ubiquitous presence of #plasma jets and magnetic field reversals suggests that a significant portion of the wind forms through dynamic processes involving magnetic #reconnection and transient energy releases.

    This Thursday, Alexis Rouillard will review recent research on the dynamics of the solar wind: irap.omp.eu/event/the-tempestu

  35. In recent years, the #ParkerSolarProbe and #SolarOrbiter probes have delivered a wealth of data about our #Sun, its surface—precisely where the #SolarWind originates. The ubiquitous presence of #plasma jets and magnetic field reversals suggests that a significant portion of the wind forms through dynamic processes involving magnetic #reconnection and transient energy releases.

    This Thursday, Alexis Rouillard will review recent research on the dynamics of the solar wind: irap.omp.eu/event/the-tempestu

  36. In recent years, the #ParkerSolarProbe and #SolarOrbiter probes have delivered a wealth of data about our #Sun, its surface—precisely where the #SolarWind originates. The ubiquitous presence of #plasma jets and magnetic field reversals suggests that a significant portion of the wind forms through dynamic processes involving magnetic #reconnection and transient energy releases.

    This Thursday, Alexis Rouillard will review recent research on the dynamics of the solar wind: irap.omp.eu/event/the-tempestu

  37. In recent years, the #ParkerSolarProbe and #SolarOrbiter probes have delivered a wealth of data about our #Sun, its surface—precisely where the #SolarWind originates. The ubiquitous presence of #plasma jets and magnetic field reversals suggests that a significant portion of the wind forms through dynamic processes involving magnetic #reconnection and transient energy releases.

    This Thursday, Alexis Rouillard will review recent research on the dynamics of the solar wind: irap.omp.eu/event/the-tempestu

  38. Les sondes #ParkerSolarProbe et #SolarOrbiter ont livré quantité de données relatives à notre #Soleil, sa surface - là où naît le #VentSolaire. L'omniprésence de jets de #plasma et d'inversions de champ magnétique suggère qu'une partie importante du vent se forme à travers des processus dynamiques impliquant la #reconnexion magnétique et des libérations d'énergie transitoires.

    Ce jeudi, Alexis Rouillard exposera les recherches récentes sur le dynamisme du vent solaire : irap.omp.eu/event/the-tempestu

  39. Les sondes #ParkerSolarProbe et #SolarOrbiter ont livré quantité de données relatives à notre #Soleil, sa surface - là où naît le #VentSolaire. L'omniprésence de jets de #plasma et d'inversions de champ magnétique suggère qu'une partie importante du vent se forme à travers des processus dynamiques impliquant la #reconnexion magnétique et des libérations d'énergie transitoires.

    Ce jeudi, Alexis Rouillard exposera les recherches récentes sur le dynamisme du vent solaire : irap.omp.eu/event/the-tempestu

  40. Les sondes #ParkerSolarProbe et #SolarOrbiter ont livré quantité de données relatives à notre #Soleil, sa surface - là où naît le #VentSolaire. L'omniprésence de jets de #plasma et d'inversions de champ magnétique suggère qu'une partie importante du vent se forme à travers des processus dynamiques impliquant la #reconnexion magnétique et des libérations d'énergie transitoires.

    Ce jeudi, Alexis Rouillard exposera les recherches récentes sur le dynamisme du vent solaire : irap.omp.eu/event/the-tempestu

  41. Les sondes #ParkerSolarProbe et #SolarOrbiter ont livré quantité de données relatives à notre #Soleil, sa surface - là où naît le #VentSolaire. L'omniprésence de jets de #plasma et d'inversions de champ magnétique suggère qu'une partie importante du vent se forme à travers des processus dynamiques impliquant la #reconnexion magnétique et des libérations d'énergie transitoires.

    Ce jeudi, Alexis Rouillard exposera les recherches récentes sur le dynamisme du vent solaire : irap.omp.eu/event/the-tempestu

  42. Les sondes #ParkerSolarProbe et #SolarOrbiter ont livré quantité de données relatives à notre #Soleil, sa surface - là où naît le #VentSolaire. L'omniprésence de jets de #plasma et d'inversions de champ magnétique suggère qu'une partie importante du vent se forme à travers des processus dynamiques impliquant la #reconnexion magnétique et des libérations d'énergie transitoires.

    Ce jeudi, Alexis Rouillard exposera les recherches récentes sur le dynamisme du vent solaire : irap.omp.eu/event/the-tempestu