Modeling of an interplanetary disturbance event tracked by the interplanetary scintillation method

Details Modeling of an interplanetary disturbance event tracked by the interplanetary scintillation method Modeling of an interplanetary disturbance event tracked by the interplanetary scintillation method

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989p%26ss...37...73a&link_type=abstract

Planetary and Space Science (ISSN 0032-0633), vol. 37, Jan. 1989, p. 73-83.

Physics

10

Interplanetary Space, Scintillation, Solar Activity Effects, Coronal Holes, Shock Waves, Solar Wind Velocity

Scientific paper

The interplanetary disturbance event of August 25-29, 1978 was modeled in an attempt to reproduce the corresponding interplanetary scintillation observations and simultaneous ISEE-3 satellite data. A shock wave generated from the region of a disappearing filament on August 23 is shown to account for the observed shock wave structure, but not the broad high-speed stream behind the shock wave. A shock wave generated by the sudden activation of the coronal hole on the same day is able to account for the high-speed stream.

Affiliated with

Also associated with

No associations

Rating

Modeling of an interplanetary disturbance event tracked by the interplanetary scintillation method 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 Modeling of an interplanetary disturbance event tracked by the interplanetary scintillation method, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Modeling of an interplanetary disturbance event tracked by the interplanetary scintillation method will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-828211