Astronomy and Astrophysics – Astrophysics
Scientific paper
Dec 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984a%26a...141...17b&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 141, no. 1, Dec. 1984, p. 17-24. Previously announced in STAR as N85-13761.
Astronomy and Astrophysics
Astrophysics
37
Interplanetary Space, Solar Storms, Solar Wind, Type 3 Bursts, Electron Density (Concentration), Helios Satellites, International Sun Earth Explorer 3, Plasma Density, Solar Wind Velocity
Scientific paper
Storms of interplanetary type III radio bursts (IP storms) are commonly observed in the interplanetary medium by the ISEE-3 radio instrument. This instrument has the capability of accurately determining the arrival direction of the radio emission. At each observing frequency, the storm radio sources are tracked as they cross the line-of-sight to the sun. Using a simple model, the emission levels are determined at a number of radio frequencies for four separate storms. The IP storm radiation is found to occur in regions of enhanced density at levels of 0.05 to 0.8 AU. The density in these enhancements falls off faster than R(-2). The solar wind speed in the storm region is also measured. The analysis is consistent with steady conditions in the storm region during a few days around the III storm burst radio emission at the harmonic of the local plasma frequency.
Bougeret Jean-Louis
Fainberg Joe
Stone Robert G.
No associations
LandOfFree
Interplanetary radio storms. II - Emission levels and solar wind speed in the range 0.05-0.8 AU 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 radio storms. II - Emission levels and solar wind speed in the range 0.05-0.8 AU, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Interplanetary radio storms. II - Emission levels and solar wind speed in the range 0.05-0.8 AU will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-732870