Published September 18, 2020
| Version v1
Working paper
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Solar Flare Energy Partitioning and Transport -- the Impulsive Phase (a Heliophysics 2050 White Paper)
Creators
- 1. Catholic University of America/NASA GSFC
- 2. NASA GSFC
- 3. Western Kentucky University
- 4. University of Glasgow / University of Oslo
- 5. American University
- 6. USRA/ NASA GSFC
- 7. NASA GSFC (Emeritus)
- 8. University of Glasgow
- 9. University of Colorado / National Solar Observatory
- 10. Queens University Belfast
- 11. BAERI / LMSAL
- 12. Montana State University
- 13. American University / NASA GSFC
Description
This white paper, submitted to the Heliophysics 2050 Workshop, discusses the solar flare impulsive phase, setting out the questions that need addressing via a combination of theoretical, modelling, and observational research. In short, by 2050 we must determine the mechanisms of particle acceleration and propagation, and must push beyond the paradigm of energy transport via nonthermal electron beams, to also account for accelerated protons & ions and downward directed Alfven waves.
Notes
Submitted to the Heliophysics 2050 Workshop
Files
Helio2050_ImpulsivePhase_GSKerr_arxiv.pdf
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Additional details
Related works
- Is identical to
- Working paper: arXiv:2009.08400 (arXiv)