太阳旋转对火星和地球热层的影响
Jeffrey M Forbes1, Sean Bruinsma, Frank G Lemoine
1Department of Aerospace Engineering Sciences, University of Colorado, Boulder, CO 80309, USA. forbes@colorado.edu
概括
地球 地球 地球 地球 地球 地球
科学领域:
- 行星科学 行星科学
- 大气物理学 大气物理学
- 太阳与地球的关系
背景情况:
- 热层是一个重要的大气层,受到太阳活动的影响.
- 了解热层对太阳流量变化的反应是大气建模的关键.
- 以前的研究表明,行星的太阳反应不同.
研究的目的:
- 为了比较地球和火星对太阳流变化的热层温度反应.
- 为验证和改进比较热层模拟提供观测数据.
- 调查太阳旋转驱动的流量变化在行星大气热平衡中的作用.
主要方法:
- 当代测量地球和火星上的热层反应.
- 使用10.7厘米的无线电流量作为极端紫外线 (EUV) 流量的代理.
- 分析温度变化,以应对典型的20个单位的太阳流量变化.
主要成果:
- 地球的热层显示,每20个单位的太阳流量变化,温度增加42.0±8.0K.
- 火星的热层表现出较小的反应,温度增加了19.2 ± 3.6 K.
- 金星数据表明3.6 ± 0.6 K的反应甚至更小.
结论:
- 地球的热层对太阳流变化的反应是火星的两倍.
- 这些发现为比较行星热层模型提供了关键的观测约束.
- 结果可能有助于解决行星热平衡的不确定性,特别是关于二氧化碳冷却.
相关概念视频
The Carbon Cycle
Carbon is the basis of all organic matter on Earth, and is recycled through the ecosystem in two primary processes: one in which carbon is exchanged among living organisms, and one in which carbon is cycled over long periods of time through fossilized organic remains, weathering of rocks, and volcanic activity. Human activities, including increased agricultural practices and the burning of fossil fuels, has greatly affected the balance of the natural carbon cycle.
Global Climate Change
Throughout its ~4.5 billion year history, the Earth has experienced periods of warming and cooling. However, the current drastic increase in global temperatures is well outside of the Earth’s cyclic norms, and evidence for human-caused global climate change is compelling. Paleoclimatology, the study of ancient climate conditions, provides ample evidence for human-caused global climate change by comparing recent conditions with those in the past.
Nuclear Fusion
The process of converting very light nuclei into heavier nuclei is also accompanied by the conversion of mass into large amounts of energy, a process called fusion. The principal source of energy in the sun is a net fusion reaction in which four hydrogen nuclei fuse and ultimately produce one helium nucleus and two positrons.
A helium nucleus has a mass that is 0.7% less than that of four hydrogen nuclei; this lost mass is converted into energy during the fusion. This reaction produces about...
A helium nucleus has a mass that is 0.7% less than that of four hydrogen nuclei; this lost mass is converted into energy during the fusion. This reaction produces about...
Mechanisms of Heat Transfer I
Just as interesting as the effects of heat transfer on a system are the methods by which the heat transfer occur. Whenever there is a temperature difference, heat transfer occurs. It may occur rapidly, such as through a cooking pan, or slowly, such as through the walls of a picnic ice box. So many processes involve heat transfer that it is hard to imagine a situation where no heat transfer occurs. Yet, every heat transfer takes place by only three methods: conduction, convection, and radiation.
Mechanisms of Heat Transfer II
In convection, thermal energy is carried by the large-scale flow of matter. Ocean currents and large-scale atmospheric circulation, which result from the buoyancy of warm air and water, transfer hot air from the tropics toward the poles and cold air from the poles toward the tropics. The Earth’s rotation interacts with those flows, causing the observed eastward flow of air in the temperate zones. Convection dominates heat transfer by air, and the amount of available space for the airflow...
Radiation: Applications
The average temperature of Earth is the subject of much current discussion. Earth is in radiative contact with both the Sun and dark space; it receives almost all its energy from the radiation of the Sun and reflects some of it into outer space. Dark space is very cold, about 3 K, so Earth radiates energy into it. For instance, heat transfer occurs from soil and grasses, the rate of which can be so rapid that frost can occur on clear summer evenings, even in warm latitudes.
The average...
The average...


