Multi-wavelength fine structure and mass flows in solar microflares

Details Multi-wavelength fine structure and mass flows in solar microflares Multi-wavelength fine structure and mass flows in solar microflares

Oct 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009a%26a...505..811b&link_type=abstract

Astronomy and Astrophysics, Volume 505, Issue 2, 2009, pp.811-823

Astronomy and Astrophysics

Astrophysics

4

Sun: Flares, Sun: Chromosphere, Sun: Corona

Scientific paper

Aims: We study the multi-wavelength characteristics at high spatial resolution, as well as chromospheric evaporation signatures of solar microflares. To this end, we analyze the fine structure and mass flow dynamics in the chromosphere, transition region and corona of three homologous microflares (GOES class Appendix A and the movie are only available in electronic form at http://www.aanda.org

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