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Solar prominence

  • Formation and Evolution of a Multi-Threaded Solar Prominence

    Formation and Evolution of a Multi-Threaded Solar Prominence

  • Multi-Spacecraft Analysis of the Solar Coronal Plasma

    Multi-Spacecraft Analysis of the Solar Coronal Plasma

  • Solar Prominence Magnetic Configurations Derived Numerically

    Solar Prominence Magnetic Configurations Derived Numerically

  • The Sun's Dynamic Atmosphere

    The Sun's Dynamic Atmosphere

  • Physics of Solar Prominences: I-Spectral Diagnostics and Non-LTE

    Physics of Solar Prominences: I-Spectral Diagnostics and Non-LTE

  • How Big? How Far?

    How Big? How Far?

  • Waves and Magnetism in the Solar Atmosphere (WAMIS)

    Waves and Magnetism in the Solar Atmosphere (WAMIS)

  • Total Solar Eclipses: Why I Observe Them and How You Can Too Martina B

    Total Solar Eclipses: Why I Observe Them and How You Can Too Martina B

  • 8-4 Asssessment 4. the Objects People Refer to As Shooting Stars Are Often Meteors Burning up in Earth's Atmosphere. If A

    8-4 Asssessment 4. the Objects People Refer to As Shooting Stars Are Often Meteors Burning up in Earth's Atmosphere. If A

  • The Standard Model of the Solar Flares

    The Standard Model of the Solar Flares

  • Prominence and Filament Eruptions Observed by the Solar Dynamics Observatory: Statistical Properties, Kinematics, and Online Catalog

    Prominence and Filament Eruptions Observed by the Solar Dynamics Observatory: Statistical Properties, Kinematics, and Online Catalog

  • Global Properties of Solar Flares

    Global Properties of Solar Flares

  • The History of Solar Prominence Research: Historical Introduction to IAU Colloquium No. 167

    The History of Solar Prominence Research: Historical Introduction to IAU Colloquium No. 167 "New Perspectives on Solar Prominences"

  • Spectro-Polarimetry of the Solar Chromosphere in the He I 10830 Å Lines

    Spectro-Polarimetry of the Solar Chromosphere in the He I 10830 Å Lines

  • Arxiv:2104.13564V1 [Astro-Ph.SR] 28 Apr 2021 with the Local Magnetic field [22]

    Arxiv:2104.13564V1 [Astro-Ph.SR] 28 Apr 2021 with the Local Magnetic field [22]

  • Sun Cookies Can You Make a Model of the Sun That’S Good Enough to Eat?

    Sun Cookies Can You Make a Model of the Sun That’S Good Enough to Eat?

  • Diagnosing the Prominence-Cavity Connection in the Solar Corona

    Diagnosing the Prominence-Cavity Connection in the Solar Corona

  • DYNAMICS of a SOLAR PROMINENCE TORNADO OBSERVED by SDO/AIA on 2012 NOVEMBER 7–8 Irakli Mghebrishvili1, Teimuraz V

    DYNAMICS of a SOLAR PROMINENCE TORNADO OBSERVED by SDO/AIA on 2012 NOVEMBER 7–8 Irakli Mghebrishvili1, Teimuraz V

Top View
  • 14.3 the Sun–Earth Connection
  • NASA/TM- ,,/ ,9 208270 Solar Prominence Eruption
  • Solar Cycle: Observations
  • Prominence Activity During the 2006 Total Solar Eclipse
  • Solar Dynamics Observatory
  • The Magnetic Field Configuration of a Solar Prominence
  • Abstract Book Conference Organizers
  • On the Solar Coronal Heat Problem
  • Solar Prominences: Theory and Models
  • What's the Difference Between Energy and Power?
  • The Role of Alfvén Wave Heating in Solar Prominences Roberto Soler1, 2, Jaume Terradas1, 2, Ramon Oliver1, 2, and Jose Luis Ballester1, 2
  • Observing the Sun
  • SJAC-Mike-Powell-The-Sun.Pdf
  • The Thermal Instability of Solar Prominence Threads
  • Causal Relationships Between Eruptive Prominences and Coronal Mass Ejections
  • Triggering of Twists in Solar Prominence Threads Y
  • Magnetic Helicity and Solar Prominence Formation
  • Module 2 – the Sun Lesson 1: Solar Prominences and Sunspots


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