Physics
Scientific paper
Nov 1978
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978jgr....83.5167b&link_type=abstract
Journal of Geophysical Research, vol. 83, Nov. 1, 1978, p. 5167-5174. Research supported by the Consiglio Nazionale delle Recer
Physics
12
Coronal Holes, Helios 1, Interplanetary Magnetic Fields, Magnetic Properties, Magnetohydrodynamic Flow, Solar Wind, Boundary Layer Flow, Lines Of Force, Magnetic Effects, Magnetic Field Configurations
Scientific paper
Magnetic phenomena and coronal holes observed by Helios 1 during nearly four rotations of the sun are discussed. It is estimated that the magnetic field intensity of open field lines in some of the coronal holes (which changed in shape and latitude from one rotation to the next) was of the order of 10-20 G during the studied period, December 1974 to March 1975. Magnetic field polarity, cold magnetic enhancements, and longitudinal widths of the stream are described. It is concluded that between the sun and 0.3 AU there was a diverging stream surrounded by a thin boundary layer in which there was large velocity shear. There is evidence for compression of the magnetic field in the western boundary layer.
Bavassano Bruno
Burlaga Leonard Francis
Harvey Jack
Mariani Franco
Ness Norman F.
No associations
LandOfFree
Magnetic fields and flows between 1 and 0.3 AU during the primary mission of HELIOS 1 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 Magnetic fields and flows between 1 and 0.3 AU during the primary mission of HELIOS 1, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Magnetic fields and flows between 1 and 0.3 AU during the primary mission of HELIOS 1 will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1067534