Interplanetary conditions during 3-kHz radio-wave detections in the outer heliosphere

Details Interplanetary conditions during 3-kHz radio-wave detections in the outer heliosphere Interplanetary conditions during 3-kHz radio-wave detections in the outer heliosphere

Jul 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985natur.316..243l&link_type=abstract

Nature (ISSN 0028-0836), vol. 316, July 18, 1985, p. 243, 244. NASA-supported research.

Physics

Plasma Physics

5

Heliosphere, Interplanetary Medium, Plasma Waves, Radio Waves, Plasma Diagnostics, Shock Wave Propagation

Scientific paper

A very important observation regarding the plasma physics of the outer heliosphere has been that plasma-wave instruments on both the Voyager 1 and 2 spacecraft beyond ≡12 AU detected, during the same interval of time, plasma waves (frequency ≡3 kHz) that could possibly be associated with the turbulence expected at the heliopause. The authors draw attention to the low-energy charged-particle environment in the outer heliosphere during the observations of the unusual plasma-wave signals. These particle data suggest that the outer heliosphere was unusually stable and free of transient shock and particle events for the ≡8 months during the wave observations.

Affiliated with

Also associated with

No associations

Rating

Interplanetary conditions during 3-kHz radio-wave detections in the outer heliosphere 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 conditions during 3-kHz radio-wave detections in the outer heliosphere, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Interplanetary conditions during 3-kHz radio-wave detections in the outer heliosphere will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1232744