Physics
Scientific paper
Jul 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002jgra..107.1121h&link_type=abstract
Journal of Geophysical Research (Space Physics), Volume 107, Issue A7, pp. SMP 20-1, CiteID 1121, DOI 10.1029/2001JA900171
Physics
26
Interplanetary Physics: Ejecta, Driver Gases, And Magnetic Clouds, Interplanetary Physics: Interplanetary Shocks, Magnetospheric Physics: Ring Current, Magnetospheric Physics: Storms And Substorms
Scientific paper
We have investigated the solar wind drivers of magnetic storms during the rising phase of solar cycle 23 from January 1996 to December 1999. We used observations of coronal mass ejections (CMEs) by the Large Angle and Spectrometric Coronagraph instrument on SOHO and in situ solar wind observations by Wind, IMP 8, and ACE spacecraft. The storms were determined from both the Dst and Kp indices, and the study was limited to storms with Dst <= -50 nT or Kp >= 5. We show examples of different behavior of Dst and Kp indices during magnetic storms caused by different types of solar wind drivers. Furthermore, we have investigated cross-correlation between peak Dst and Kp values of storms organized according to the associated solar wind driver. It makes a difference whether a sheath region or the following ejecta causes the storm. We found that almost all intense and stronger magnetic storms (Dst <= -100 nT, or Kp >= 7-) were associated with shocks and CMEs, but for moderate storms, driver statistics were different in different phases of the solar cycle. We found different behavior of the Kp and Dst indices during different types of solar wind drivers. Intense and short-time disturbances, like postshock streams and sheath regions, generated more Kp storms, and ejecta generated more Dst storms. Thus one should be careful when comparing studies based on any single activity index.
Huttunen Emilia J. K.
Koskinen Hannu E. J.
Schwenn Rainer
No associations
LandOfFree
Variability of magnetospheric storms driven by different solar wind perturbations 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 Variability of magnetospheric storms driven by different solar wind perturbations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Variability of magnetospheric storms driven by different solar wind perturbations will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-734788