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Fig. 18 | Earth, Planets and Space

Fig. 18

From: The existence of cosmic ray sidereal anisotropies of galactic and solar origins with energies lower than 104 GeV and their modulation caused by the presumed behavior pattern of the heliomagnetosphere and of its neighboring gaseous matter in interstellar magnetic field

Fig. 18

The distribution of the tail-in (TA) and galactic (GA) anisotropies on the equatorial coordinate grid (Ref. 3). The excess cone of TA, within which all the directional excess flux is confined, is shown bounded by the thick line including the south pole. A thinner line bounds the deficit cone of GA, in which all the directional deficit flux is confined (cf. Nagashima et al., 1989). PM, direction of proper motion of the solar system; RM, direction of relative motion of the system to the neutral gas; (thin line), galactic equator.

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