Energy Release During Slow Long-Duration Flares Observed by RHESSI

6Citations
Citations of this article
9Readers
Mendeley users who have this article in their library.

This article is free to access.

Abstract

Slow long-duration events (SLDEs) are flares characterized by the long duration of their rising phase. In many such cases the impulsive phase is weak without typical short-lasting pulses. Instead, smooth, long-lasting hard X-ray (HXR) emission is observed. We analyzed hard X-ray emission and morphology of six selected SLDEs. In our analysis we utilized data from the RHESSI and GOES satellites. The physical parameters of HXR sources were obtained from imaging spectroscopy and were used for the energy balance analysis. The characteristic decay time of the heating rate, after reaching its maximum value, is very long, which explains the long rising phase of these flares. © 2011 The Author(s).

Author supplied keywords

Cite

CITATION STYLE

APA

Ba̧k-Stȩślicka, U., Mrozek, T., & Kołomański, S. (2011). Energy Release During Slow Long-Duration Flares Observed by RHESSI. Solar Physics, 271(1), 75–89. https://doi.org/10.1007/s11207-011-9803-9

Register to see more suggestions

Mendeley helps you to discover research relevant for your work.

Already have an account?

Save time finding and organizing research with Mendeley

Sign up for free