RHESSI Science Nuggets in September 2019September 29, 2019, from Hugh Hudson
No. 356: “EVE-RHESSI DEM Models and the Low-Energy Cutoff for Non-thermal Electrons”, by Jim McTiernan. Characterizing flare temperature distributions helps to define the non-thermal energy release.
No. 357: “Dynamic Processes of the Moreton Wave on 2014 March 29”, by Denis Cabezas and the FMT team. A beautiful chromospheric wave was excited by the best-observed flare ever.
No. 358: “The Last Best Flares”, by Hugh Hudson, Ed Cliver, and Brian Dennis. Major flares tend to happen at the very ends of sunspot cycles.
No. 359: “Submillimeter Radiation as the Thermal Component of the Neupert Effect.” Flare emission at the highest radio frequencies can be bremsstrahlung.
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 be found by searching for their SOLyyyy-mm-dd identifier from this home page.