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                  <gco:CharacterString>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</gco:CharacterString>
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            <gco:CharacterString>We study the response of the thermosphere and ionosphere to gravity waves (GWs) excited by 6âh 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 Î»Hâ¼70â300âkm, periods of 10â60âmin, and phase speeds of cHâ¼50â225âm/s propagate well into the thermosphere. Their density perturbations are Æ¿âp ~15 â 25% at zâ¼150âkm and are negligible at z&gt;300âkm. The dissipation of these GWs creates spatially and temporally localized body forces with amplitudes of 0.2â 1.0 m/s2at zâ¼120â230âkm. These forces generate two counter-rotating circulation cells with horizontal velocities of 50â350âm/s. They also excite secondary GWs; those resolved by our global model have Î»Hâ¼4000â5000âkm and cHâ¼500â600âm/s. These secondary GWs propagate globally and have Æ¿âp ~10 â 25% and 5â15% at z=250 and 375âkm, respectively. These forces also create plasma perturbations of foF2â²â¼0.2â1.0âMHz, TECâ²â¼0.4â 1.5âTECU (total electron content unit, 1TECUâ =10Â¹â¶ elmâ»Â²), and hmF2â²â¼5â50âkm. The large-scale traveling ionospheric disturbances (LSTIDs) induced by the secondary GWs have amplitudes of foF2â²â¼0.2â0.5âMHz, TECâ²â¼0.2â 0.6 TECU, and hmF2â²â¼5â10âkm. In a companion paper, we discuss changes to the prereversal enhancement and plasma drift from these forces.</gco:CharacterString>
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