The Sun in Time: Activity and Environment

IF 23 1区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS Living Reviews in Solar Physics Pub Date : 2007-12-20 DOI:10.12942/lrsp-2007-3
Manuel Güdel
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引用次数: 168

Abstract

The Sun’s magnetic activity has steadily declined during its main-sequence life. While the solar photospheric luminosity was about 30% lower 4.6 Gyr ago when the Sun arrived on the main sequence compared to present-day levels, its faster rotation generated enhanced magnetic activity; magnetic heating processes in the chromosphere, the transition region, and the corona induced ultraviolet, extreme-ultraviolet, and X-ray emission about 10, 100, and 1000 times, respectively, the present-day levels, as inferred from young solar-analog stars. Also, the production rate of accelerated, high-energy particles was orders of magnitude higher than in present-day solar flares, and a much stronger wind escaped from the Sun, permeating the entire solar system. The consequences of the enhanced radiation and particle fluxes from the young Sun were potentially severe for the evolution of solar-system planets and moons. Interactions of high-energy radiation and the solar wind with upper planetary atmospheres may have led to the escape of important amounts of atmospheric constituents. The present dry atmosphere of Venus and the thin atmosphere of Mars may be a product of early irradiation and heating by solar high-energy radiation. High levels of magnetic activity are also inferred for the pre-main sequence Sun. At those stages, interactions of high-energy radiation and particles with the circumsolar disk in which planets eventually formed were important. Traces left in meteorites by energetic particles and anomalous isotopic abundance ratios in meteoritic inclusions may provide evidence for a highly active pre-main sequence Sun. The present article reviews these various issues related to the magnetic activity of the young Sun and the consequent interactions with its environment. The emphasis is on the phenomenology related to the production of high-energy photons and particles. Apart from the activity on the young Sun, systematic trends applicable to the entire main-sequence life of a solar analog are discussed.

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及时的太阳:活动与环境
太阳的磁活动在其主序层生命期间稳步下降。4.6 Gyr以前,当太阳到达主序层时,太阳光球的亮度比现在的水平低30%左右,但它更快的自转产生了增强的磁场活动;从年轻的类似太阳的恒星中推断,色球层、过渡区和日冕的磁加热过程分别诱导紫外线、极紫外线和x射线的发射,大约是现在水平的10倍、100倍和1000倍。此外,加速高能粒子的产生速度比现在的太阳耀斑要高几个数量级,而且从太阳逸出的风更强,渗透到整个太阳系。来自年轻太阳的增强辐射和粒子通量的后果对太阳系行星和卫星的演化可能是严重的。高能辐射和太阳风与上层行星大气的相互作用可能导致了大量大气成分的逃逸。金星目前的干燥大气和火星的稀薄大气可能是早期太阳高能辐射照射和加热的产物。高水平的磁活动也被推断为前主序太阳。在这些阶段,高能辐射和粒子与行星最终形成的日环盘的相互作用非常重要。高能粒子在陨石中留下的痕迹和陨石包裹体中异常的同位素丰度比值可能为高度活跃的前主序太阳提供证据。本文回顾了这些与年轻太阳的磁活动及其与环境的相互作用有关的各种问题。重点是与高能光子和粒子的产生有关的现象学。除了在年轻太阳上的活动外,还讨论了适用于太阳类似物的整个主序生命的系统趋势。
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来源期刊
Living Reviews in Solar Physics
Living Reviews in Solar Physics Earth and Planetary Sciences-Space and Planetary Science
CiteScore
41.90
自引率
1.40%
发文量
3
审稿时长
20 weeks
期刊介绍: Living Reviews in Solar Physics is a peer-reviewed, full open access, and exclusively online journal, publishing freely available reviews of research in all areas of solar and heliospheric physics. Articles are solicited from leading authorities and are directed towards the scientific community at or above the graduate-student level. The articles in Living Reviews provide critical reviews of the current state of research in the fields they cover. They evaluate existing work, place it in a meaningful context, and suggest areas where more work and new results are needed. Articles also offer annotated insights into the key literature and describe other available resources. Living Reviews is unique in maintaining a suite of high-quality reviews, which are kept up-to-date by the authors. This is the meaning of the word "living" in the journal''s title.
期刊最新文献
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