No. 156,
X-ray, EUV & WL emission heights observed by RHESSI & SDO
, by Marina Battaglia and Eduard Kontar
High resolution allows us to determine source heights for the first time. See
http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/X-ray,_EUV_%26_WL_emission_heights_observed_by_RHESSI_%26_SDO
Older Nuggets are available at
http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/RHESSI_Science_Nuggets
(the new series), and at
http://sprg.ssl.berkeley.edu/~tohban/nuggets/
(the original series).
We publish these at roughly two-week intervals and welcome
contributions, which should be at least loosely related to RHESSI
science.