27 Jul
2011
27 Jul
'11
1:30 p.m.
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_emissi...
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.