Interplanetary coronal mass ejections during the descending cycle 23: Sheath and ejecta properties comparison

Details Interplanetary coronal mass ejections during the descending cycle 23: Sheath and ejecta properties comparison Interplanetary coronal mass ejections during the descending cycle 23: Sheath and ejecta properties comparison

Feb 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009adspr..43..495m&link_type=abstract

Advances in Space Research, Volume 43, Issue 4, p. 495-498.

Computer Science

1

Scientific paper

We have used Omniweb data in order to identify the sheath and the ejecta boundaries of 67 shock-driving interplanetary coronal mass ejections during the time period 2003-2006. We examine and compare their statistical properties (speed, magnetic field strength, proton density and temperature, proton plasma beta), with those of the typical solar wind. We also calculate their passage time and radial width. We study the correlation between the ejecta and sheath characteristics.

Affiliated with

Also associated with

No associations

Rating

Interplanetary coronal mass ejections during the descending cycle 23: Sheath and ejecta properties comparison 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 Interplanetary coronal mass ejections during the descending cycle 23: Sheath and ejecta properties comparison, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Interplanetary coronal mass ejections during the descending cycle 23: Sheath and ejecta properties comparison will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-835321