Radio evidence for interplanetary streamers in the range 10-170 solar radii

Details Radio evidence for interplanetary streamers in the range 10-170 solar radii Radio evidence for interplanetary streamers in the range 10-170 solar radii

Nov 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983nascp.2280.469f&link_type=abstract

In JPL Solar Wind Five p 469-474 (SEE N84-13067 03-92)

Physics

1

International Sun Earth Explorer 3, Interplanetary Medium, Solar Radio Bursts, Solar Storms, Electrons, Radio Frequencies, Solar Corona

Scientific paper

Type III radio storms are observed by the radio experiment on board the International Sun Earth Explorer 3 out to 0.5-0.8 AU from the Sun, at a rate of 2 to 3 storms per solar rotation near solar maximum. They correlate with the type I and type III radio storms observed at higher frequencies, originating closer to the Sun. They are associated with an almost continuous injection of suprathermal electrons into the interplanetary medium. Some of the properties of the regions where the particles propagate are discussed, using the radio emission as a tracer.

Affiliated with

Also associated with

No associations

Rating

Radio evidence for interplanetary streamers in the range 10-170 solar radii 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 Radio evidence for interplanetary streamers in the range 10-170 solar radii, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Radio evidence for interplanetary streamers in the range 10-170 solar radii will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1487797