No. 349, “Warm UV Loops Heated by Small-Scale Cancellation Events,” by S. Şahin and V. Yurchyshyn: Precisely locating warm coronal loops helps identify the source(s) of excitation.

No. 348, “Multiple Regions of Shock-accelerated Particles during a Solar Coronal Mass Ejection,” by D. Morosan: LOFAR identifies herringbone sources within the flank of the SOL2017-09-10 shock – no joke.

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