磁层-电离层电风暴对地圈相互作用的影响

IF 0.7 4区 物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS
L. F. Chernogor
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引用次数: 0

摘要

定量分析强地磁风暴触发的电场-电离层-电流-大气-电离层和电场-大气-岩石圈两个子系统的过程是一个相关的任务。本研究旨在评估磁层-电离层电风暴对内外地圈相互作用的影响。该研究定量地评估了这种电风暴在SIMMIAE系统内部和外部地球圈相互作用中的作用。由于电离层电流在电场作用下的耗散,在120-350公里高度的大气温度在白天增加几十到几百开尔文,在夜间增加一个单位到几百开尔文。已经证明,被加热的大气气体以每秒几十米到几百米不等的速度上升,这取决于海拔高度。被加热的大气气体上升的特征时间随海拔高度的增加而减少,白天从大约10分钟减少到4分钟,夜间从40分钟减少到8-9分钟。热通量密度在海拔150 km左右达到最大值,白天达到20 mW/m2,夜间达到0.1 ~ 0.2 mW/m2。焦耳在大气中加热的最大功率白天为200gw,夜间为1 - 2gw。大气中的焦耳热量白天可达200 TJ,夜间可达5-6 TJ。起源于磁层-电离层的电风暴也会在岩石圈引起电风暴。在这种情况下,岩石圈内的电场强度可达到约10-100µV/m,焦耳加热功率范围为1 ~ 1000 MW,能量范围为1 ~ 40000 GJ。大气和岩石圈的焦耳加热作为电场响应的触发过程。热层触发系数为1010 ~ 1011,岩石圈触发系数为1012 ~ 1013。提出了大气和岩石圈电风暴的七分制分类。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Impact of Electrical Storms of Magnetospheric-Ionospheric Origin on Geosphere Interactions

The quantitative analysis of processes in the subsystems electric field–ionospheric current–atmosphere–ionosphere and electric field–atmosphere–lithosphere, triggered by powerful geomagnetic storms, is a relevant task. The study aims to assess the impact of the electrical storms of magnetospheric-ionospheric origin on the interaction between the external and internal geospheres. The study quantitatively evaluates the role of such electrical storms in the interaction between the external and internal geospheres within the SIMMIAE system. Due to the dissipation of ionospheric current under the action of the electric field, the atmospheric temperature at altitudes of 120–350 km increases by tens to hundreds of Kelvins during the day and by units to hundreds of Kelvins during the night. It has been shown that the heated atmospheric gas rises with a speed varying from tens to hundreds of meters per second depending on altitude. The characteristic time for the ascent of heated atmospheric gas decreases with altitude, from approximately 10 to 4 min during the day and from 40 to 8–9 min during the night. The heat flux density is maximal at an altitude of around 150 km, reaching 20 mW/m2 during the day and 0.1–0.2 mW/m2 during the night. The maximum power of Joule heating in the atmosphere is 200 GW during the day and 1–2 GW during the night. The quantity of Joule heat in the atmosphere reaches 200 TJ during the day and 5–6 TJ during the night. An electrical storm of magnetospheric-ionospheric origin also induces an electrical storm in the lithosphere. In this case, the electric field strength in the lithosphere can reach approximately 10–100 µV/m, the power of Joule heating ranges from 1 to 1000 MW, and the energy spans 1–40 000 GJ. Joule heating of the atmosphere and lithosphere acts as a triggering process in response to the electric field. The triggering coefficient ranges from 1010 to 1011 for the thermosphere and from 1012 to 1013 for the lithosphere. Seven-point scales for classifying electrical storms in the atmosphere and lithosphere are proposed.

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来源期刊
Kinematics and Physics of Celestial Bodies
Kinematics and Physics of Celestial Bodies ASTRONOMY & ASTROPHYSICS-
CiteScore
0.90
自引率
40.00%
发文量
24
审稿时长
>12 weeks
期刊介绍: Kinematics and Physics of Celestial Bodies is an international peer reviewed journal that publishes original regular and review papers on positional and theoretical astronomy, Earth’s rotation and geodynamics, dynamics and physics of bodies of the Solar System, solar physics, physics of stars and interstellar medium, structure and dynamics of the Galaxy, extragalactic astronomy, atmospheric optics and astronomical climate, instruments and devices, and mathematical processing of astronomical information. The journal welcomes manuscripts from all countries in the English or Russian language.
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