Info

Vt, 2003 hour avg.

r «

1 A tognexmal

B^ = 0033nT (4600 hours)

Fig. 3.6.8. Statistical distributions of observed by Voyager 1 (V1) HMF in Heliosheath (A) in 2005 and in Solar Wind (B) in 2003. From Ness et al. (2005).

The hourly averaged Heliospheric magnetic field observations by Voyager 1 during 2004-2005, 61 days before and 76 days after the Terminal shock crossing on day 351, 2004 are shown in Fig. 3.6.9.

Voyager 1,2004/2005

Solar Wind TS .

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