No. 167, Flare Observations of the EUV Continua, by Ryan Milligan: SDO/EVE now routinely observes the EUV continua for major flares. This Nugget evaluates their energy content for the first X-class flare of Cycle 24, SOL2011-02-24.

See http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/Flare_Observations_of_th... ,

Older Nuggets are available at http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/RHESSI_Science_Nuggets (the current series, 2008-present), and at http://sprg.ssl.berkeley.edu/~tohban/nuggets/ (the original series, 2005-2008).

We publish these at roughly two-week intervals and welcome contributions, which should be related, at least loosely, to RHESSI science.