Effect of magnetospheric convection on the energy distribution of protons from the Earth radiation belts

2010 ◽  
Vol 50 (3) ◽  
pp. 298-302 ◽  
Author(s):  
S. V. Smolin
Author(s):  
S. N. Kuznetsov ◽  
Yu. I. Denisov ◽  
L. L. Lazutin ◽  
I. N. Myagkova ◽  
E. A. Muravieva ◽  
...  

1998 ◽  
Vol 21 (12) ◽  
pp. 1801-1804 ◽  
Author(s):  
A.V. Bogomolov ◽  
A.V. Dmitriev ◽  
I.N. Myagkova ◽  
S.P. Ryumin ◽  
O.N. Smirnova ◽  
...  

2008 ◽  
Vol 4 (S257) ◽  
pp. 57-59
Author(s):  
I. Dorotovič ◽  
K. Kudela ◽  
M. Lorenc ◽  
T. Pintér ◽  
M. Rybanský

AbstractIn our recent paper (Dorotovič et al. 2008a) we focused on a study of the Forbush decrease (FD) of January 17–18 and 21–22, 2005. It was shown that the corresponding recovery time can depend on the density of high-energy protons in the CME matter. In this paper we identified several additional events in the period between 1995 and 2007. We found that the majority of FDs studied is accompanied by an abrupt count increase in the proton channel P1 and by a simultaneous decrease in the channel P7 (GOES). However, the analysis of temporal evolution of all FDs did not confirm the hypothesis on different recovery time after FD as a function of the energy distribution of the particles penetrating into radiation belts of the Earth.


2007 ◽  
Vol 41 (4) ◽  
pp. 338-347 ◽  
Author(s):  
S. N. Kuznetsov ◽  
I. N. Myagkova ◽  
B. Yu. Yushkov ◽  
Yu. I. Denisov ◽  
E. A. Murav’eva ◽  
...  

1990 ◽  
Author(s):  
Jack Paden ◽  
Dhirendra K. Pandey ◽  
Robert S. Wilson ◽  
Susan Thomas ◽  
Michael A. Gibson ◽  
...  

1994 ◽  
Vol 12 (2/3) ◽  
pp. 240-253 ◽  
Author(s):  
F. Parol ◽  
J. C. Buriez ◽  
D. Crétel ◽  
Y. Fouquart

Abstract. Through their multiple interactions with radiation, clouds have an important impact on the climate. Nonetheless, the simulation of clouds in climate models is still coarse. The present evolution of modeling tends to a more realistic representation of the liquid water content; thus the problem of its subgrid scale distribution is crucial. For a convective cloud field observed during ICE 89, Landsat TM data (resolution: 30m) have been analyzed in order to quantify the respective influences of both the horizontal distribution of liquid water content and cloud shape on the Earth radiation budget. The cloud field was found to be rather well-represented by a stochastic distribution of hemi-ellipsoidal clouds whose horizontal aspect ratio is close to 2 and whose vertical aspect ratio decreases as the cloud cell area increases. For that particular cloud field, neglecting the influence of the cloud shape leads to an over-estimate of the outgoing longwave flux; in the shortwave, it leads to an over-estimate of the reflected flux for high solar elevations but strongly depends on cloud cell orientations for low elevations. On the other hand, neglecting the influence of cloud size distribution leads to systematic over-estimate of their impact on the shortwave radiation whereas the effect is close to zero in the thermal range. The overall effect of the heterogeneities is estimated to be of the order of 10 W m-2 for the conditions of that Landsat picture (solar zenith angle 65°, cloud cover 70%); it might reach 40 W m-2 for an overhead sun and overcast cloud conditions.


1986 ◽  
Vol 24 (2) ◽  
pp. 357 ◽  
Author(s):  
Frederick B. House ◽  
Arnold Gruber ◽  
Garry E. Hunt ◽  
Ann T. Mecherikunnel

Sign in / Sign up

Export Citation Format

Share Document