在太阳和地磁指数以及 SABER 热层红外功率测量中观测到的周期性现象

IF 1.8 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS
Nabil Nowak , Martin G. Mlynczak , Linda Hunt , B. Thomas Marshall , Christopher J. Mertens
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引用次数: 0

摘要

我们分析了 F10.7 厘米太阳射电通量和阿普地磁指数的周期性特征,以研究 100 公里以上地球大气中的日地耦合。在一氧化氮(NO)和二氧化碳(CO2)辐射的全球红外功率中观测到的周期性特征也表明了这种耦合。自 2002 年 1 月以来,NASA TIMED 卫星上的 SABER 仪器一直在测量红外功率数据。在所有数据集中都可以观察到太阳周期长度(≈11 年)的强烈主导特征。在不同的太阳周期中,这一周期的长度从 9.95 年到 12.25 年不等。在 F10.7 和 Ap 指数中也能观测到大于太阳周期长度的周期特征(≈22 年和≈44 年)。在 Ap 指数中可以观察到一个强烈的 180 天周期特征,这与著名的 Russell-McPherron 效应相对应。此外,NO 功率和 Ap 指数在较短周期(如 27 天、13.5 天和 9 天)内也表现出统计意义上的显著周期特征。这种相似性表明热大气层的红外能量预算与高层大气的地磁条件之间存在密切联系。
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Periodicities observed in the solar and geomagnetic indexes and in SABER thermospheric infrared power measurements

We analyze periodic features in the F10.7 cm solar radio flux and the Ap geomagnetic index to examine solar-terrestrial coupling in Earth's atmosphere above 100 km. The coupling is indicated by the same periodic features observed in the global infrared power radiated by Nitric Oxide (NO) and Carbon Dioxide (CO2). The infrared power data have been measured by the SABER instrument on the NASA TIMED satellite since January 2002. A strong dominant feature for the length of the solar cycle (≈11 years) can be observed in all the datasets. The length of this periodicity can vary from 9.95 years to 12.25 years for different solar cycles. Periodic features larger than the length of the solar cycle are also observed in the F10.7 and Ap index (≈22 years and ≈44 years). A strong 180-day periodic feature can be observed in the Ap index which corresponds to the well-known Russell-McPherron effect. Additionally, the NO power and the Ap index exhibit statistically significant periodic features for shorter periods (e.g., 27, 13.5 and 9 days). This similarity indicates a strong link between the thermosphere's infrared energy budget and the geomagnetic conditions of the upper atmosphere.

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来源期刊
Journal of Atmospheric and Solar-Terrestrial Physics
Journal of Atmospheric and Solar-Terrestrial Physics 地学-地球化学与地球物理
CiteScore
4.10
自引率
5.30%
发文量
95
审稿时长
6 months
期刊介绍: The Journal of Atmospheric and Solar-Terrestrial Physics (JASTP) is an international journal concerned with the inter-disciplinary science of the Earth''s atmospheric and space environment, especially the highly varied and highly variable physical phenomena that occur in this natural laboratory and the processes that couple them. The journal covers the physical processes operating in the troposphere, stratosphere, mesosphere, thermosphere, ionosphere, magnetosphere, the Sun, interplanetary medium, and heliosphere. Phenomena occurring in other "spheres", solar influences on climate, and supporting laboratory measurements are also considered. The journal deals especially with the coupling between the different regions. Solar flares, coronal mass ejections, and other energetic events on the Sun create interesting and important perturbations in the near-Earth space environment. The physics of such "space weather" is central to the Journal of Atmospheric and Solar-Terrestrial Physics and the journal welcomes papers that lead in the direction of a predictive understanding of the coupled system. Regarding the upper atmosphere, the subjects of aeronomy, geomagnetism and geoelectricity, auroral phenomena, radio wave propagation, and plasma instabilities, are examples within the broad field of solar-terrestrial physics which emphasise the energy exchange between the solar wind, the magnetospheric and ionospheric plasmas, and the neutral gas. In the lower atmosphere, topics covered range from mesoscale to global scale dynamics, to atmospheric electricity, lightning and its effects, and to anthropogenic changes.
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