The SolarNuggets continue the earlier series of RHESSI Nuggets, and are now located at
https://heliowiki.smce.nasa.gov/wiki/index.php/SolarNuggets
No. 516, “A fine-scale bright kernel captured by Hi-C 3 in the post-maximum phase of an M-class solar flare,” by Sanjiv TIWARI: An extremely compact brightening in late-phase flare ribbon development.
No. 517, “Observational Evidence Linking Loop Length and Thermal/Nonthermal Peak Timing in Solar Flares,” by Solomon PERRIYIL: Clear evidence for the universality of the physics behind the Neupert effect.
No. 518, "When Magnetic Field Lines Stretch, Snap, and Expand: A New Look at Solar Flares with L-maps,” by Maria KAZACHENKO et al: A clever new tool tracks magnetic connectivity (and energy) during flare/CME occurrence.
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 news-oriented text and 2-3 nice figures.
mmscience@solar.physics.montana.edu