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Low-frequency waves in the solar wind near Neptune

Journal Article · · Geophysical Research Letters (American Geophysical Union); (United States)
DOI:https://doi.org/10.1029/91GL01050· OSTI ID:5316401
; ;  [1];  [2];  [3]; ;  [4]
  1. Massachusetts Inst. of Tech., Cambridge (USA)
  2. Max-Planck-Inst. for Aeronomie, Garching (West Germany)
  3. NASA Goddard Space Flight Center, Greenbelt, MD (USA)
  4. Univ. of Delaware, Newark (USA)
Plasma and magnetic field observations from the Voyager 2 spacecraft when it was outbound from Neptune reveal low-frequency waves in the solar wind which are clearly associated with the planet. The waves have frequencies below the proton cyclotron frequency f{sub cp}, which is about 10{sup {minus}3} Hz during the periods waves are observed. The waves are present when the interplanetary magnetic field is oriented such that the spacecraft is connected to the bow shock by the magnetic field lines. The authors have identified the waves to be Alfvenic waves propagating at {approximately}140 {degree} to the ambient magnetic field and away from the bow shock. As at the other planets, these downstream waves are thought to be generated in the upstream region, where energetic protons created near the nose of the bow shock excite waves as they stream along solar wind magnetic field lines.
OSTI ID:
5316401
Journal Information:
Geophysical Research Letters (American Geophysical Union); (United States), Journal Name: Geophysical Research Letters (American Geophysical Union); (United States) Vol. 18:6; ISSN 0094-8276; ISSN GPRLA
Country of Publication:
United States
Language:
English