气候:今天的太阳活动有多不寻常?
Raimund Muscheler1, Fortunat Joos, Simon A Müller
1National Center for Atmospheric Research, Climate and Global Dynamics Division, Paleoclimatology, Boulder, Colorado 80305-3000, USA. raimund@ucar.edu
Nature
|July 29, 2005
概括
最近几十年的太阳活动可能与过去8,000年相比没有特别高. 对放射性碳记录的扩展分析显示,在过去的几个世纪,太阳风的磁场强度相似或更高.
科学领域:
- 气候科学是气候科学.
- 太阳物理 太阳物理
- 古气候学 古气候学
背景情况:
- 了解全球变暖需要从过去的太阳活动和太阳在气候变化中的作用中了解背景.
- 以前的研究表明,最近的太阳活动在过去的8000年中异常高.
研究的目的:
- 通过分析长期太阳风磁场强度,重新评估最近太阳活动的特殊性.
- 为当前太阳活动及其对气候的潜在影响提供更准确的历史背景.
主要方法:
- 放射性碳记录的扩展分析.
- 过去几个世纪太阳风磁场强度的重建.
主要成果:
- 确定了过去几个世纪的几个时期,太阳风的磁场强度与最近的水平相比或超过.
- 质疑了最近太阳活动在过去8,000年中是前所未有的概念.
结论:
- 最近的太阳活动水平可能并不像以前提出的那样异常高.
- 太阳的磁场强度表现出变化,过去的时期与今天相似或高于今天.
相关概念视频
What is Weather?
17.2K
Overview
17.2K
What is Climate?
17.5K
Climate refers to the prevailing weather conditions in a specific area over an extended period. As the saying goes, “Climate is what you expect. Weather is what you get.” Climate is influenced by geographic factors, such as latitude, terrain, and proximity to bodies of water.
17.5K
Global Climate Change
24.4K
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.
24.4K
Nuclear Fusion
33.2K
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...
33.2K
Radiation: Applications
1.8K
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...
1.8K
Radiation Pressure: Problem Solving
1.0K
The radiation pressure applied by an electromagnetic wave on a perfectly absorbing surface equals the energy density of the wave. The wave's momentum also gets transferred to the surface when an electromagnetic wave is entirely absorbed by it. The rate at which momentum is transmitted to an absorbing surface perpendicular to the propagation direction equals the force on the surface.
The average value of the rate of momentum transfer divided by the absorbing area represents the average force...
The average value of the rate of momentum transfer divided by the absorbing area represents the average force...
1.0K


