Please find the new SolarNuggets, extending our old RHESSI Nuggets, at

https://heliowiki.smce.nasa.gov/wiki/index.php/SolarNuggets.

Entries for October and November 2024:

No. 479, "Remarkable NUV Spectrum of an M-star Megaflare,” by Adam KOWALSKI

No. 478, "Revised Point-Spread Functions of AIA and their effect on DEM analyses,” by Stefan HOFMEISTER, Daniel Wolf SAVIN, and Michael HAHN

No. 477, "How much of the energy in flare-accelerated electrons reaches the chromosphere?” by Meriem ALAOUI and Gordon HOLMAN

No. 476, "Spatially resolved plasma composition evolution in a solar flare,” by Andy S. H. To

No. 475, “HOPE during high activity,” by Hugh HUDSON and Alphonse STERLING

No. 474, "Simulated heliospheric electron spectra show sensitivity to plasma properties of a source region in the flaring corona,” by Ross PALLISTER and Natasha JEFFREY

No. 473, "An extremely complex active region with very strong non-neutralized electric currents," by Ioannis KONTOGIANNIS

No. 472, “An X9 flare and its huge crochet (SFE)” by Hugh HUDSON

We apologize for the interruption of service and thank Damian Barrous and Steven Christe for major help in getting re-started. As always, we welcome new items and encourage opinion pieces and news items as well as descriptions of new discoveries. Just email Hugh Hudson with a page of text and 2-3 nice figures.