Nitric oxide cooling emission during geomagnetic storm: Case studies

被引：0
|
作者：
Bag, Tikemani [1 ]
Barman, Rahul [2 ]
Das, Sukanya A. [2 ]
Sivakumar, V. [3 ,4 ]
Singh, Vir [5 ]
机构：
[1] Natl Inst Polar Res, 10-3 Midori Cho, Tachikawa, Tokyo 1908518, Japan
[2] CV Raman Global Univ, Dept Phys, Bhubaneswar 752054, India
[3] Univ KwaZulu Natal, Discipline Phys, Westville, Durban, South Africa
[4] Univ KwaZulu Natal, Natl Inst Theoret & Computat Sci, Westville, Durban, South Africa
[5] Indian Inst Technol Roorkee, Dept Phys, Roorkee 247667, India
来源：
ADVANCES IN SPACE RESEARCH | 2024年 / 73卷 / 01期
基金：
日本学术振兴会;
关键词：
Mesosphere-Thermosphere Energetics and Dynamics; Geomagnetic storm; Infrared Radiative emission; Diurnal variation; TIMED-SABER satellite; TIMED/SABER MEASUREMENTS; TIME-VARIATION; NO; THERMOSPHERE; IONOSPHERE; SABER; MODEL;
D O I：
10.1016/j.asr.2023.09.064
中图分类号：
V [航空、航天];
学科分类号：
08 ; 0825 ;
摘要：
The Nitric Oxide (NO) emission at 5.3 mm is the dominating thermospheric coolant in the altitude above - 100 km. It effectively regulates the thermospheric temperature during space weather events. We studied the diurnal response of the Nitric Oxide at 5.3 mm emission to the geomagnetic storms of different intensities by using the NO emission data from the Sounding of Atmosphere using Broadband Emission Radiometry (SABER) instrument onboard NASA's Thermosphere-Ionosphere-Mesosphere Energetics and Dynamics (TIMED) satellite. We selected eight CME-driven geomagnetic storms with |SYM-H| index ranging from 0 to 500 nT. One of the storms that occurred during 19-22 November 2003 is investigated in details. Other events are used for comparison. The NO flux and the NO power during different phases of the geomagnetic storms are calculated with 24 h-time bins from the storm's onset. The NO cooling and the cooling power are always higher during the daytime. Although the NO cooling flux and the cooling power increase with the storm (c) 2023 COSPAR. Published by Elsevier B.V. All rights reserved.
引用
收藏
页码：747 / 757
页数：11
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