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Record #144638:
Modeling the high-latitude equinoctial asymmetry / Anasuya L. Aruliah, J. Schoendorf, A.D. Aylward, M.N. Wild.
Title: | Modeling the high-latitude equinoctial asymmetry / Anasuya L. Aruliah, J. Schoendorf, A.D. Aylward, M.N. Wild. |
Author(s): | Aruliah, Anasuya L. Schoendorf, J. Aylward, A. D. Wild, M. N. |
Date: | 1997. |
In: | Journal of Geophysical Research. (1997.), Vol. 102(A12) (1997) |
Abstract: | Interferometer measurements of neutral winds and radar measurements of plasma velocities have shown significant equinoctial asymmetry in average behaviour of thermosphere and ionosphere above northern Scandinavia. It is suggested that asymmetry arises from diurnal variation in cross polar cap potential difference, because there is 12 hour phase difference between variations at March and September equinoxes. Effect is Russell-McPherron Effect, which has been simulated in laboratories, and implies that auroral oval may be unexpectedly smaller at solar minimum. |
Notes: | Journal of Geophysical Research. Vol. 102(A12) :27, 027-27, 216 (1997). |
Keywords: | 551.510.5 -- Atmosphere, structure. 551.510.535 -- Ionosphere. 551.594.51 -- Aurora, physics and technical analysis. 551.594.52 -- Aurora, height and geographical distribution. A -- Geophysical sciences (general). (*3) -- Arctic regions. (*571.1) -- Norrbottens lan. |
SPRI record no.: | 144638 |
LDR 01665naa#a2200000#a#4500 001 SPRI-144638 005 20231207112330.0 007 ta 008 231207s1997####xx#a##|##|###|0||#0|eng#d 035 ## ‡aSPRI-144638 040 ## ‡aUkCU-P‡beng‡eaacr 245 00 ‡aModeling the high-latitude equinoctial asymmetry /‡cAnasuya L. Aruliah, J. Schoendorf, A.D. Aylward, M.N. Wild. 260 ## ‡a[S.l.] :‡b[s.n.],‡c1997. 300 ## ‡ap. 27, 027-27, 216 :‡bdiags. 500 ## ‡aJournal of Geophysical Research. Vol. 102(A12) :27, 027-27, 216 (1997). 520 3# ‡aInterferometer measurements of neutral winds and radar measurements of plasma velocities have shown significant equinoctial asymmetry in average behaviour of thermosphere and ionosphere above northern Scandinavia. It is suggested that asymmetry arises from diurnal variation in cross polar cap potential difference, because there is 12 hour phase difference between variations at March and September equinoxes. Effect is Russell-McPherron Effect, which has been simulated in laboratories, and implies that auroral oval may be unexpectedly smaller at solar minimum. 650 07 ‡a551.510.5 -- Atmosphere, structure.‡2udc 650 07 ‡a551.510.535 -- Ionosphere.‡2udc 650 07 ‡a551.594.51 -- Aurora, physics and technical analysis.‡2udc 650 07 ‡a551.594.52 -- Aurora, height and geographical distribution.‡2udc 650 07 ‡aA -- Geophysical sciences (general).‡2local 651 #7 ‡a(*3) -- Arctic regions.‡2udc 651 #7 ‡a(*571.1) -- Norrbottens lan.‡2udc 700 1# ‡aAruliah, Anasuya L. 700 1# ‡aSchoendorf, J. 700 1# ‡aAylward, A. D. 700 1# ‡aWild, M. N. 773 0# ‡7nnas ‡tJournal of Geophysical Research. ‡gVol. 102(A12) (1997) ‡wSPRI-35252 916 ## ‡a118157 -- 1998/08/13 917 ## ‡aUnenhanced record from Muscat, imported 2019 948 3# ‡a20231207