Numerical modeling of the large-scale neutral and plasma responses to the body forces created by the dissipation of gravity waves from 6 h of deep convection in Brazil
We study the response of the thermosphere and ionosphere to gravity waves (GWs) excited by 6âh of deep convection in Brazil on the evening of 01 October 2005 via the use of convective plume, ray trace, and global models. We find that primary GWs excited by convection having horizontal wavelengths of λHâ¼70â300âkm, periods of 10â60âmin, and phase speeds of cHâ¼50â225âm/s propagate well into the thermosphere. Their density perturbations are Æ¿âp ~15 â 25% at zâ¼150âkm and are negligible at z>300âkm. The dissipation of these GWs creates spatially and temporally localized body forces with amplitudes of 0.2â 1.0 m/s2at zâ¼120â230âkm. These forces generate two counter-rotating circulation cells with horizontal velocities of 50â350âm/s. They also excite secondary GWs; those resolved by our global model have λHâ¼4000â5000âkm and cHâ¼500â600âm/s. These secondary GWs propagate globally and have Æ¿âp ~10 â 25% and 5â15% at z=250 and 375âkm, respectively. These forces also create plasma perturbations of foF2â²â¼0.2â1.0âMHz, TECâ²â¼0.4â 1.5âTECU (total electron content unit, 1TECUâ =10¹ⶠelmâ»Â²), and hmF2â²â¼5â50âkm. The large-scale traveling ionospheric disturbances (LSTIDs) induced by the secondary GWs have amplitudes of foF2â²â¼0.2â0.5âMHz, TECâ²â¼0.2â 0.6 TECU, and hmF2â²â¼5â10âkm. In a companion paper, we discuss changes to the prereversal enhancement and plasma drift from these forces.
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https://n2t.org/ark:/85065/d7xw4kp0
eng
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2016-01-01T00:00:00Z
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2013-05-21T00:00:00Z
Copyright 2013 American Geophysical Union.
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