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Hydromagnetic emissions, X-ray bursts, and electron bunches: 2. Theoretical interpretation

Journal Article · · Journal of Geophysical Research
The existence of bunches of monoenergetic electrons oscillating back and forth along field lines in the magnetosphere has been suggested by a number of workers to explain various geophysical phenomena. The simultaneous occurrence of x-ray and hydromagnetic emission bursts (regular oscillatory micropulsations at frequencies in the range 1-2 cps) immediately after sudden commencements and during magnetically disturbed periods, as discussed in part 1, raises the possibility that hm emissions could be generated by such electron bunches. A model is presented that considers certain aspects of the motion of geomagnetically trapped electrons relevant to the production of hm emissions by electron bunches. A new result is the calculation of electron motion in a dipole field confined to the interior of a sphere (as a first approximation to the solar wind cavity). The model calculations are applied to experimental results discussed in part 1, and it is shown that the electrons responsible for the x-ray burst after the sudden commencement of June 27, 1960, could have produced the hm emission burst at that time, and that the maximum observed hm emission frequency as a function of geomagnetic latitude is consistent with the calculated value. Hydromagnetic emissions during magnetically quiet times are characterized by a fine structure containing overlapping bands of rapidly increasing frequency. This is tentatively interpreted as indicating rapid acceleration of electron bunches; hence, if the model is correct, hm emissions will provide a powerful tool for studying the acceleration mechanism for electrons in the magnetosphere.
Research Organization:
Lockheed Aircraft Corp., Palo Alto, Calif.
Sponsoring Organization:
USDOE
NSA Number:
NSA-17-003924
OSTI ID:
4761500
Journal Information:
Journal of Geophysical Research, Journal Name: Journal of Geophysical Research Journal Issue: 9 Vol. 67; ISSN 0148-0227
Publisher:
American Geophysical Union
Country of Publication:
Country unknown/Code not available
Language:
English

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