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

No. 414, “Confined or Eruptive?”, by Ting LI, Anqin CHEN, Yijun HOU, Astrid M. VERONIG, Shuhong YANG, and Jun ZHANG: Increased magnetic flux reduces the eruptivity of a solar active region.

No. 415, “Do Hot Onsets Predict Flare Magnitudes”? by Hugh HUDSON: Maybe we can tell how big a flare is going to be from its initial development.

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.