Physics
Scientific paper
Mar 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992georl..19..429c&link_type=abstract
Geophysical Research Letters (ISSN 0094-8276), vol. 19, March 3, 1992, p. 429-432. Research supported by USAF.
Physics
40
Annual Variations, Ejecta, Magnetic Storms, Magnetic Variations, Solar Corona, Solar Terrestrial Interactions, Equinoxes, Geomagnetism, Interplanetary Magnetic Fields, Shock Waves, Stellar Mass Ejection
Scientific paper
Recent results indicate that the intense southward interplanetary magnetic fields (IMFs) responsible for great storms can reside in the postshock plasma preceding the driver gas of coronal mass ejections (CMEs) as well as in the driver gas itself. It is proposed here that strong southward fields in the postshock flow result from a major increase in the Russell-McPherron polarity effect through a systematic pattern of compression and draping within the ecliptic plane. Differential compression at the shock increases the Parker spiral angle and, consequently, the azimuthal field component that projects as a southward component onto earth's dipole axis. The resulting prediction is that southward fields in the postshock plasma maximize at the spring (fall) equinox in CMEs emerging from toward (away) sectors. This pattern produces a strong semiannual variation in postshock IMF orientation and may account at least in part for the observed semiannual variation of the occurrence of great geomagnetic storms.
Cliver Edward W.
Crooker Nancy U.
Tsurutani Bruce T.
No associations
LandOfFree
The semiannual variation of great geomagnetic storms and the postshock Russell-Mcpherron effect preceding coronal mass ejecta 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 semiannual variation of great geomagnetic storms and the postshock Russell-Mcpherron effect preceding coronal mass ejecta, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The semiannual variation of great geomagnetic storms and the postshock Russell-Mcpherron effect preceding coronal mass ejecta will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1217576