まとめ
太陽活動が太陽の放射線量に影響する. 紫外線は,総エネルギーのわずかな部分ですが,太陽周期の移行時に太陽光照射量の総変化に大きく影響します.
科学分野:
- 宇宙物理学 宇宙物理学
- 太陽物理 太陽物理学
- 大気科学 大気科学
背景:
- 太陽のエネルギー出力,または太陽放射線量は,太陽活動サイクルによって変化します.
- これらの変動を理解することは,気候と宇宙天候の研究に不可欠です.
研究 の 目的:
- 合計と紫外線 (UV) の太陽照射の傾向を分析する.
- これらの傾向と太陽活動周期 (太陽周期21と22年) を相関させる.
主な方法:
- 1980年以降の衛星で測定された太陽光全照射量のデータを分析.
- 太陽の紫外線照射データ,特に200~300 nmの波長を分析した.
主要な成果:
- 総太陽光照射量は1980年から1985年半ばまで減少し,安定し,その後増加した.
- 紫外線照射は同様の傾向で,太陽のサイクル21の衰退中に減少し,サイクル22の始まりで増加しました.
- 紫外線照射量の減少 (1981年−1985年) は,その期間における全照射量の減少の19%を占めた.
結論:
- 太陽光照射量の変動は,太陽活動サイクルと密接に結びついています.
- 紫外線は,太陽の全照射量の変動において,不釣り合いの大きな役割を果たしている.
関連する概念動画
Mutations
Mutations are changes in the sequence of DNA. These changes can occur spontaneously or they can be induced by exposure to environmental factors. Mutations can be characterized in a number of different ways: whether and how they alter the amino acid sequence of the protein, whether they occur over a small or large area of DNA, and whether they occur in somatic cells or germline cells.
Chromosomal Alterations Are Large-Scale Mutations
While point mutations are changes in a single nucleotide in...
Chromosomal Alterations Are Large-Scale Mutations
While point mutations are changes in a single nucleotide in...
Ultraviolet and Visible (UV–Vis) Spectroscopy: Overview
Ultraviolet–visible (UV–visible or UV–Vis) spectroscopy is an analytical technique that investigates the interaction between matter and UV–Vis light within the electromagnetic spectrum. This method is widely used for its versatility, simplicity, and relatively quick data acquisition, making it valuable for both qualitative and quantitative analysis. When UV–Vis radiation passes through a material, molecules absorb light depending on the energy required for electronic transitions. As a result...
Radiation Pressure: Problem Solving
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 per...
The average value of the rate of momentum transfer divided by the absorbing area represents the average force per...
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...
Absorption of Radiation
The rate of heat transfer by emitted radiation is described by the Stefan-Boltzmann law of radiation:
Energy Transfer in Chemical Reactions
Chemical reactions require sufficient energy to cause the matter to collide with enough precision and force that old chemical bonds can be broken and new ones formed. In general, kinetic energy is the form of energy powering any type of matter in motion. Imagine a person building a brick wall. The energy it takes to lift and place one brick on top of another is the kinetic energy—the energy matter possesses because of its motion. Once the wall is in place, it stores potential energy. Potential...


