High-Resolution Spectroscopy of Gamma-Ray Lines from the X-Class Solar Flare of 2002 July 23

2003 ◽  
Vol 595 (2) ◽  
pp. L81-L84 ◽  
Author(s):  
D. M. Smith ◽  
G. H. Share ◽  
R. J. Murphy ◽  
R. A. Schwartz ◽  
A. Y. Shih ◽  
...  
2000 ◽  
Vol 543 (1) ◽  
pp. 77-89 ◽  
Author(s):  
P. Kurczynski ◽  
D. Palmer ◽  
H. Seifert ◽  
B. J. Teegarden ◽  
N. Gehrels ◽  
...  

1981 ◽  
Vol 75 (1) ◽  
pp. 181-191 ◽  
Author(s):  
B. J. Teegarden ◽  
T. L. Cline

1998 ◽  
Vol 21 (1-2) ◽  
pp. 347-350 ◽  
Author(s):  
H.V Kladpor-Kleingrothaus ◽  
J Hellmig ◽  
A Mueller ◽  
H Strecker ◽  
S.I Svertilov ◽  
...  

2009 ◽  
Author(s):  
V. D’Elia ◽  
F. Fiore ◽  
F. Nicastro ◽  
R. Perna ◽  
Y. Krongold ◽  
...  

2005 ◽  
Vol 13 ◽  
pp. 784-786
Author(s):  
Jürgen Knödlseder

AbstractGamma-ray spectroscopy has made important progress with the observations of the OSSE and COMPTEL telescopes aboard CGRO, and has entered the domain of high-resolution spectroscopy with the launch of the SPI telescope aboard the INTEGRAL satellite. Recent science highlights in this field are presented, and an outlook is given to future promising projects.


2005 ◽  
Vol 624 (2) ◽  
pp. 853-867 ◽  
Author(s):  
F. Fiore ◽  
V. D’Elia ◽  
D. Lazzati ◽  
R. Perna ◽  
L. Sbordone ◽  
...  

1994 ◽  
Vol 144 ◽  
pp. 635-639
Author(s):  
J. Baláž ◽  
A. V. Dmitriev ◽  
M. A. Kovalevskaya ◽  
K. Kudela ◽  
S. N. Kuznetsov ◽  
...  

AbstractThe experiment SONG (SOlar Neutron and Gamma rays) for the low altitude satellite CORONAS-I is described. The instrument is capable to provide gamma-ray line and continuum detection in the energy range 0.1 – 100 MeV as well as detection of neutrons with energies above 30 MeV. As a by-product, the electrons in the range 11 – 108 MeV will be measured too. The pulse shape discrimination technique (PSD) is used.


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