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ИСТИНА ЦЭМИ РАН |
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The Model I was proposed to explain the LP effect of neutron flux suppression at lunar poles. For using this model, one postulates that epi-thermal neutron flux at polar regions outside PSRs is about the same as at moderate latitudes of the Moon, but spots of PSRs have very strong suppression of epi-thermal neutron emission. This resolution scale of LP measurements is much larger than size of an individual PSR (about 10 – 30 km or smaller). Therefore, one cannot use the LP neutron data for direct test of the presence of local neutron suppressions at individual PSRs.