Computer Science
Scientific paper
May 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009adspr..43.1575r&link_type=abstract
Advances in Space Research, Volume 43, Issue 10, p. 1575-1587.
Computer Science
Scientific paper
The variations in the horizontal and declination components of the geomagnetic field in response to the interplanetary shocks driven by fast halo coronal mass ejections, fast solar wind streams from the coronal hole regions and the dynamic pressure pulses associated with these events are studied. Close association between the field-aligned current density (j∥) and the fluctuations in the declination component (ΔDABG) at Alibag is found for intense storm conditions. Increase in the dawn-dusk interplanetary electric field (Ey) and ΔDABG are generally in phase. However, when the magnetospheric electric field is directed from dusk to dawn direction, a prominent scatter occurs between the two. It is suggested that low-latitude ground magnetic data may serve as a proxy for the interplanetary conditions in the solar wind.
Alex Shobana
Lakhina Gurbax S.
Rawat Rahul
No associations
LandOfFree
Low-latitude geomagnetic response to the interplanetary conditions during very intense magnetic storms 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 Low-latitude geomagnetic response to the interplanetary conditions during very intense magnetic storms, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Low-latitude geomagnetic response to the interplanetary conditions during very intense magnetic storms will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1107845