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DTIC ADA210522: The Auroral Energy Deposition Over the Polar Ionosp...
by Defense Technical Information Center
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The global Joule heating distributions are estimated
through the magnetogram inversion method. This study
employs instantaneous ionospheric conductance
distributions deduced from the DMSP-F6 bremsstrahlung
Xray image data. Also estimated from the Xray data are
instantaneous global particle heating distributions. The
two heating distributions thus obtained allow us to
investigate various aspects of heat energy processes over
the polar ionosphere on an instantaneous basis. A special
emphasis is placed on their spatial and temporal
behaviors. Several important results of this study are
summarized as follows: (1) Regions of significant Joule
heating are closely associated with the auroral
electrojets prominently in the dawn and dusk sectors. (2)
The major Joule heating usually occurs poleward of the
major particle heating region, particularly in the
morning sector. On the other hand, the two heating
patterns are complementary in the longitudinal direction.
(3) There is a higher correlation between the global
Joule heating rate (U Sub J) and AE(12) than between the
global particle heating rate (U Sub A) and AE(12). (4)
The particle heating rate tends to be more prominent
during the maximum phase of substorms and afterward than
during the pre-expansion phase. (5) The U Sub J/U Sub A
ratio varies by more than a factor of 10, suggesting the
wide variability in the relative importance of the two
heating rates. On the average, however, U Sub J is larger
than U Sub A by a factor of 6.
Date Published: 2018-02-22 22:41:15
Identifier: DTIC_ADA210522
Item Size: 24910970
Language: english
Media Type: texts
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