RHESSI Nuggets in November 2020

November 24, 2020, from Hugh Hudson

No. 393, “Self-Consistent Flare Model”, by Wwnzhi RUAN and Rony KEPPENS: Energy transport by fast particles made self-consistent with MHD flare modeling.

No. 394, “Probing the solar coronal heating function with slow magnetoacoustic waves,” by Dmitriii KOLOTKOV et al.: Coronal heating models meet damped slow magnetoacoustic waves.

No. 395. “What drives impulsive coronal heating?” by Pradeep CHITTA et al.: Impulsive footpoint emissions suggest magnetic reconnection in the chromosphere.

We welcome contributions to the RHESSI Nuggets, and the topics may wander some distance away from specifically RHESSI results if they are generally interesting. See http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/RHESSI_Science_Nuggets for these and others. Comments about specific flares can often be found by searching for their SOLyyyy-mm-dd identifier from this home page.

http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/RHESSI_Science_Nuggets


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