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The beam driven chromospheric evaporation model of large solar flares: a model getting “no respect” from the sun

  • V. Heating and Flows in Flares
  • Conference paper
  • First Online:
Flare Physics in Solar Activity Maximum 22

Part of the book series: Lecture Notes in Physics ((LNP,volume 387))

  • 130 Accesses

Abstract

Since before the last solar maximum, theoretical and to some extent observational, flare physics were dominated by beam driven chromospheric evaporation models. Comparisons between theoretical predictions and observations from soft and hard X-ray radiations point to major model inconsistencies. An account of some of the inconsistencies as well as the requirements for a better soft X-ray model are presented.

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Authors and Affiliations

  1. E.O. Hulburt Center for Space Research, Naval Research Laboratory, 20375-5000, Washington, DC

    Uri Feldman

Authors
  1. Uri Feldman
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Editor information

Yutaka Uchida Richard C. Canfield Tetsuya Watanabe Eijiro Hiei

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© 1991 Springer-Verlag

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Feldman, U. (1991). The beam driven chromospheric evaporation model of large solar flares: a model getting “no respect” from the sun. In: Uchida, Y., Canfield, R.C., Watanabe, T., Hiei, E. (eds) Flare Physics in Solar Activity Maximum 22. Lecture Notes in Physics, vol 387. Springer, Berlin, Heidelberg. https://doi.org/10.1007/BFb0032630

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  • DOI: https://doi.org/10.1007/BFb0032630

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-54383-1

  • Online ISBN: 978-3-540-47596-5

  • eBook Packages: Springer Book Archive

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