木星半球活动因子的季节变化及其与太阳活动和轨道运动的关系

IF 0.7 4区 物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS
A. P. Vidmachenko
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引用次数: 0

摘要

为了研究季节变化和太阳活动的影响,作者分析了木星大气反射特性的长期变化。木星有一个非常活跃的大气层,主要由氢和氦组成。微量的氨、甲烷和其他化合物形成了可见的云层和云层上方的雾霾。地球强大的磁层在观测到的现象的形成中起着重要作用。木星轨道的显著偏心率(e≈0.0485)导致太阳输入到行星大气的能量在近日点和远日点之间变化21%。北半球接收到的能量明显更多,因为夏至发生在地球经过近日点的时候。这引起大气物理特性的变化,并表明季节变化的存在。为了量化这些变化,采用热带和温带南北地区的亮度比AJ = BN/BS作为大气过程光度活度的因子。对1960-2025年期间的这些数据进行分析,发现AJ变化具有明显的周期性,周期约为11.87年,与木星的轨道周期相对应,表明了季节性大气重构过程。分析了轨道偏心率(日照变化21%)和太阳活动(特别是22年的黑尔周期和紫外线辐射)对木星各层大气的影响。在轨道强迫和太阳强迫协调的时间间隔内,木星大气的特征辐射松弛时间约为3.4年(τR≈1.07 × 108 s)。记录了1995年至2012年的不平衡阶段及其随后的恢复,同时有效辐射常数下降至约2.5年(τR≈0.79 × 108 s),这可能反映了太阳活动对高层大气的影响增强。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Seasonal Changes in the Activity Factor of Jupiter’s Hemispheres and Their Relationship with Solar Activity and Orbital Motion

Seasonal Changes in the Activity Factor of Jupiter’s Hemispheres and Their Relationship with Solar Activity and Orbital Motion

Seasonal Changes in the Activity Factor of Jupiter’s Hemispheres and Their Relationship with Solar Activity and Orbital Motion

The authors analyze the long-term changes in the reflective properties of Jupiter’s atmosphere in order to study seasonal variations and the influence of solar activity. Jupiter has a very dynamic atmosphere consisting primarily of hydrogen and helium. Trace amounts of ammonia, methane, and other compounds form the visible cloud layers and haze above the clouds. The planet’s powerful magnetosphere plays an important role in the formation of the observed phenomena. The significant eccentricity of Jupiter’s orbit (e ≈ 0.0485) causes the solar energy input to the planet’s atmosphere to vary by 21% between perihelion and aphelion. The Northern Hemisphere receives significantly more energy because its summer solstice occurs during the planet’s passage through perihelion. This causes variations in the physical characteristics of the atmosphere and indicates the presence of seasonal changes. In order to quantify these changes, the brightness ratio of the northern and southern tropical and temperate regions AJ = BN/BS as a factor of photometric activity of atmospheric processes were used. Analysis of these data for the period 1960–2025 has revealed a clear periodicity in AJ changes with a period of approximately 11.87 years, which corresponds to Jupiter’s orbital period and indicates seasonal atmospheric restructuring processes. The effects of orbital eccentricity (a 21% variation in insolation) and solar activity (notably the 22-year Hale cycle and UV radiation) on Jupiter’s various atmospheric layers are analyzed. The characteristic radiative relaxation time of Jupiter’s atmosphere is found to be approximately 3.4 years (τR ≈ 1.07 × 108 s) during intervals of coordinated orbital and solar forcings. A phase of imbalance from 1995 to 2012 and its subsequent recovery have been documented, accompanied by a decrease in the effective radiative constant to approximately 2.5 years (τR ≈ 0.79 × 108 s), likely reflecting an enhanced influence of solar activity on the upper atmosphere.

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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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