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PROBLEMS OF GEOCOSMOS

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Proceedings of the 7th International Conference "Problems of Geocosmos" (St. Petersburg, Russia, 26-30 May 2008)<br />

Fig 5. Radial profiles measured by CORONAS-F spectrometer from October 27 to 30, 2003. Channels 1-5 MeV (left) and<br />

14-26 MeV (right)<br />

Fig 6 Storm-time variation during magnetic storms, July<br />

2004<br />

Fig. 7 Radial profiles of the 1.2 MeV protons,<br />

SERVIS-1. All profiles were taken at the same<br />

longitude over BMA.<br />

25.07.04 Important changes of the radial profiles were registered after the main phase of the second magnetic<br />

storm. Previously created proton belt disappeared because it was occupied by the region of the direct SCR<br />

penetration, the quasitrapping region. What was the fate of this trapped protons – do they escaped from the<br />

magnetopause into the solar wind or were lost by diffusion into the loss cone, or they survive due to the<br />

radial diffusion from L=3.7 to L=3.2? Anyway, new proton belt was created during the initial part of the<br />

recovery phase of the second storm.<br />

26.07.04 Before the beginning of the last magnetic storm one can see that intensity of the proton belt<br />

increased and maximum shifted a little earthward. That we can ascribe to the action of the recovery phase.<br />

27.07.04 It seems that this new (solar) proton belt was too close to the Earth to be affected by the PB motion<br />

during the main phase of the third magnetic storm. As was mentioned previously, there were no effects<br />

indicating on the particle SC injection (see Fig. 2).<br />

28-29.07.04 During the recovery phase of the third magnetic storm one can see an increase of the intensity<br />

and earthward shift of the proton belt maximum.<br />

It is evident from the radial profile transformation discussed above, that it was created and accelerated at the<br />

recovery phase of the magnetic storm, not by the SC-injection.<br />

6. DISCUSSION AND CONCLUSION<br />

Process of the solar proton capture to the proton belt at L=2-3 was confirmed by the observation during<br />

several magnetic storms, there are no doubts on the reality of this process. But there are different opinions on<br />

the mechanisms of this process. We analyzed here two models which were discussed in publications.<br />

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