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Multi-wavelength fine structure and mass flows in solar microflares

Astronomy and Astrophysics (2009) 505(2) 811-823
DOI: 10.1051/0004-6361/200912100
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Abstract

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

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Berkebile-Stoiser, S., Gömöry, P., Veronig, A. M., Rybák, J., & Sütterlin, P. (2009). Multi-wavelength fine structure and mass flows in solar microflares. Astronomy and Astrophysics, 505(2), 811–823. https://doi.org/10.1051/0004-6361/200912100

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