Premium
Dynamics Explorer observations of the production of electron conics
Author(s) -
Burch J. L.
Publication year - 1995
Publication title -
geophysical research letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.007
H-Index - 273
eISSN - 1944-8007
pISSN - 0094-8276
DOI - 10.1029/95gl02817
Subject(s) - conic section , physics , electron , tilt (camera) , magnetic field , electric field , pitch angle , computational physics , acceleration , particle acceleration , range (aeronautics) , optics , geophysics , classical mechanics , geometry , materials science , nuclear physics , mathematics , quantum mechanics , composite material
Several mechanisms have been proposed as the cause of electron conics, including perpendicular, oblique, and parallel heating, as well as acceleration by both stochastic and oscillating parallel electric fields. While the conic distributions and various wave modes have been observed together, no measurements have been made of the actual acceleration mechanism while it is in progress. This study reports on data obtained by DE‐1, which measured conies at high altitudes (≥ 10,000 km) over the auroral oval, and DE‐2, which simultaneously measured electron distributions at low altitudes (∼900 km) in the same latitude/local time region. The DE‐2 electron distributions often show the low‐altitude signature of a downward field‐aligned beam, which has spread to pitch angles of about 55° as a result of the magnetic mirror force, along with an upward‐moving electron conic distribution localized in the same pitch‐angle range. Even though the electron conies observed by DE‐2 have energies of only several hundred eV, compared to the several keV conics observed by DE‐1, these observations nevertheless support models in which field‐aligned bursts and electron conics occur on the same field line, with the conic being the result of the magnetic mirroring of the part of the downward electron beam that lies just outside the loss cone.