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Table 3 Table 2

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

 

V (km/s)

α(hr)

δ(°)

\(V_{HMS}^{S}\) of HMS relative to Stars

19.65

18.04

29.2

\(V_{HMS}^{C}\) of HMS observed by CRs

 

18

24

\(V_{HMS}^{CS}\) of HMS relative to Stars

(∼20)

18

24

Vnp between np and HMS

 

16.8

−15∼−17

\(V_{np}^{HMS}\) of np relative to HMS

26

4.8

15 ∼ 17

\(V_{IGM}^{S}\) of IGM relative to Stars

17.5

0

66.5