A possible observation of a cometary bow shock

Details A possible observation of a cometary bow shock A possible observation of a cometary bow shock

Oct 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984georl..11.1022r&link_type=abstract

Geophysical Research Letters (ISSN 0094-8276), vol. 11, Oct. 1984, p. 1022-1025. Research supported by Lockheed Independent Rese

Astronomy and Astrophysics

Astronomy

11

Bow Waves, Comets, Plasma Interactions, Shock Wave Propagation, Solar Wind, Interplanetary Magnetic Fields, Pioneer Venus 1 Spacecraft, Shock Discontinuity, Space Plasmas, Venus (Planet), Comets, Bowshock, Observations, Astronomy, Density, Temperature, Thermal Properties, Velocity, Magnetic Properties, Structure, Hypotheses

Scientific paper

In February, 1982, an unusual enhancement of the IMF was observed by the Pioneer Venus orbiter at 0.72 AU. The three discontinuities within this large disturbance, previously suggested to be due to the possible passage of a comet, are examined in view of the alternative possibility of their representing the first observation to date of a cometary shock. It is noted that number density, temperature, and velocity changes, as well as the magnetic structure of the discontinuities, are consistent with this hypothesis.

Affiliated with

Also associated with

No associations

Rating

A possible observation of a cometary bow shock 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 A possible observation of a cometary bow shock, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A possible observation of a cometary bow shock will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1227697