Energetic charged particle angular distributions near (r less than or equal to 2 Neptune radii) and over the pole of Neptune

Details Energetic charged particle angular distributions near (r less than or equal to 2 Neptune radii) and over the pole of Neptune Energetic charged particle angular distributions near (r less than or equal to 2 Neptune radii) and over the pole of Neptune

Sep 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990georl..17.1701m&link_type=abstract

Geophysical Research Letters (ISSN 0094-8276), vol. 17, Sept. 1990, p. 1701-1704.

Physics

13

Angular Distribution, Charged Particles, Neptune (Planet), Polar Regions, Voyager 2 Spacecraft, Auroras, Pitch (Inclination), Planetary Magnetic Fields, Voyager Project

Scientific paper

Energetic ion (greater than 28 keV) and electron (greater than 22 keV) pitch angle distributions very close to (r less than or equal to 2 Neptune radii) and over the north planetary pole of Neptune are presented using data from the Low Energy Charged Particle and magnetometer Experiments on the Voyager 2 spacecraft. The particle data are temporally structured and spectrally soft; a similarity with earth-like auroral signatures has previously been noted. However, the pitch angle distributions (showing trapped distributions at high magnetic latitudes) do not support an earth-like auroral interpretation, and alternative explanations for the temporal dynamics must be sought. Between r of about 1.6 and 2.0 Neptune radii and in the vicinity of the magnetic equator, the higher energy ion and electron pitch angle distributions (E greater than or equal to 80 keV) display dramatic 'bite-outs' at 90 deg. This bite-out feature could be caused by interactions with the newly discovered ring 1989N3R.

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