The global structure of the solar wind in June 1991

Details The global structure of the solar wind in June 1991 The global structure of the solar wind in June 1991

Dec 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993soph..148..371u&link_type=abstract

Solar Physics, Volume 148, Issue 2, pp.371-382

Physics

14

Scientific paper

A numerical simulation of the global solar wind structure for Carrington rotation 1843 (31 May 28 June, 1991) is performed based on a fully three-dimensional, steady-state MHD model of the solar wind (Usmanov, 1993b). A self-consistent solution for 3-D MHD equations is constructed for the spherical shell extending from the solar photosphere up to 10 AU. Solar magnetic field observations are used to prescribe boundary conditions. The computed distribution of the magnetic field is compared with coronal hole observations and with the IMF measurements made by IMP-8 spacecraft at the Earth's orbit.

Affiliated with

Also associated with

No associations

Rating

The global structure of the solar wind in June 1991 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The global structure of the solar wind in June 1991, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The global structure of the solar wind in June 1991 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1302385