Документ взят из кэша поисковой машины. Адрес оригинального документа : http://xray.sai.msu.ru/~mystery/html/latex/rotating.ps Дата изменения: Thu Sep 10 19:50:24 1998 Дата индексирования: Tue Oct 2 12:19:51 2012 Кодировка:

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The galactic binary GW noisewill be modulated by the LISA orbital motion,
whereas the extragalactic one will not. If the latter is comparable with galactic
values at some galactic latitudes, it can impede detection by LISA of some inter­
esting relic cosmological GW backgrounds, and specific statistical features of the
relic GW should be used to separate them against the noise from astrophysical
sources.
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