The relative abundances and energy spectra of solar-flare-accelerated deuterium, tritium, and helium-3

1975 ◽  
Vol 198 ◽  
pp. 733 ◽  
Author(s):  
J. D. Anglin
1981 ◽  
Vol 1 (3) ◽  
pp. 73-76 ◽  
Author(s):  
E.I. Daibog ◽  
E.A. Devicheva ◽  
S.V. Golenetskii ◽  
Yu.A. Guryan ◽  
V.G. Kurt ◽  
...  

2011 ◽  
Vol 55 (4) ◽  
pp. 374-381 ◽  
Author(s):  
M. A. Zel’dovich ◽  
Yu. I. Logachev ◽  
G. M. Surova

1992 ◽  
Vol 401 ◽  
pp. 398 ◽  
Author(s):  
J. E. Mazur ◽  
G. M. Mason ◽  
B. Klecker ◽  
R. E. McGuire

1998 ◽  
Vol 498 (2) ◽  
pp. 779-789 ◽  
Author(s):  
S. W. Barwick ◽  
J. J. Beatty ◽  
C. R. Bower ◽  
C. J. Chaput ◽  
S. Coutu ◽  
...  

1989 ◽  
Vol 104 (2) ◽  
pp. 255-258 ◽  
Author(s):  
V.V. Kasinsky ◽  
R.T. Sotnikova

AbstractBased on X-ray (1-8 Å) flux data for 1977-1987, the integral spectra of solar flare energy were computed. The energy spectra were approximated by a power law N(E) α; E~n, with N being the number of flares with energy in excess of E. It is shown that the spectral index (β) varies systematically with the 11-year cycle phase.


Sign in / Sign up

Export Citation Format

Share Document