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Global Climate Change01:50

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.
Kepler's Second Law of Planetary Motion01:29

Kepler's Second Law of Planetary Motion

In the early 17th century, German astronomer and mathematician Johannes Kepler postulated three laws for the motion of planets in the solar system. His first law states that all planets orbit the Sun in an elliptical orbit, with the Sun at one of the ellipse's foci. Therefore, the distance of a planet from the Sun varies throughout its revolution around the Sun.
While in an elliptical orbit, the total energy of the planet is conserved. Therefore, the planet slows down when it is at apogee and...
Kepler's First Law of Planetary Motion01:10

Kepler's First Law of Planetary Motion

In the early 17th century, German astronomer and mathematician Johannes Kepler postulated three laws for the motion of planets in the solar system. He formulated his first two laws based on the observations of his forebears, Nikolaus Copernicus and Tycho Brahe.
Polish astronomer Nikolaus Copernicus put forth a theory that stated a heliocentric model for the solar system. According to this heliocentric theory, all the planets, including Earth, orbit the Sun in circular orbits.
On the other hand,...
What is Climate?01:16

What is Climate?

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.
Radiation: Applications01:17

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...
Kepler's Third Law of Planetary Motion01:18

Kepler's Third Law of Planetary Motion

In the early 17th century, German astronomer and mathematician Johannes Kepler postulated three laws for the motion of planets in the solar system. In 1909, he formulated his first two laws based on the observations of his forebears, Nikolaus Copernicus and Tycho Brahe. However, in 1918, he published his third law of planetary motion, which gives a precise mathematical relationship between a planet's average distance from the Sun and the amount of time it takes to revolve around the Sun. It...

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相关实验视频

Updated: Jul 12, 2026

Scattering And Absorption of Light in Planetary Regoliths
11:34

Scattering And Absorption of Light in Planetary Regoliths

Published on: July 1, 2019

由于气溶引起的行星白度变化.

M A Atwater

    Science (New York, N.Y.)
    |October 2, 1970
    PubMed
    概括

    气溶会影响地球的白度,导致大气加热或冷却. 气溶吸收与散射的微妙变化可以扭转这些气候趋势.

    科学领域:

    • 大气科学 大气科学
    • 气候科学是气候科学.
    • 辐射转移是一种辐射转移.

    背景情况:

    • 气溶通过与太阳辐射相互作用,显著影响地球的能量平衡.
    • 气溶对行星白度 (升温或降温) 的净影响取决于它们的光学特性和表面反射率.
    • 了解这些相互作用对于准确的气候建模至关重要.

    研究的目的:

    • 研究气溶特性如何影响行星的白度和随后的大气温度变化.
    • 确定气候趋势对气溶吸收和散射比率变化的敏感性.
    • 突出气溶光学特征在气候动态中的关键作用.

    主要方法:

    • 对控制气溶与表面相互作用的辐射转移原理的分析.
    • 基于不同的气溶光学性能的行星白度变化的建模.
    • 检查气溶吸收和散射比率的时间变化.

    主要成果:

    • 由于气溶引起的行星白度变化的标志是由气溶吸收/散射和表面反射率之间的相互作用决定的.
    • 行星白度的变化直接导致大气的升温或降温.
    • 气溶吸收与散射比率的微小变化可能会导致已建立的加热或冷却趋势的逆转.

    更多相关视频

    Measurement of Aerosols Optical Thickness of the Atmosphere using the GLOBE Handheld Sun Photometer
    06:27

    Measurement of Aerosols Optical Thickness of the Atmosphere using the GLOBE Handheld Sun Photometer

    Published on: May 29, 2019

    Split Point Analysis and Uncertainty Quantification of Thermal-Optical Organic/Elemental Carbon Measurements
    10:22

    Split Point Analysis and Uncertainty Quantification of Thermal-Optical Organic/Elemental Carbon Measurements

    Published on: September 7, 2019

    相关实验视频

    Last Updated: Jul 12, 2026

    Scattering And Absorption of Light in Planetary Regoliths
    11:34

    Scattering And Absorption of Light in Planetary Regoliths

    Published on: July 1, 2019

    Measurement of Aerosols Optical Thickness of the Atmosphere using the GLOBE Handheld Sun Photometer
    06:27

    Measurement of Aerosols Optical Thickness of the Atmosphere using the GLOBE Handheld Sun Photometer

    Published on: May 29, 2019

    Split Point Analysis and Uncertainty Quantification of Thermal-Optical Organic/Elemental Carbon Measurements
    10:22

    Split Point Analysis and Uncertainty Quantification of Thermal-Optical Organic/Elemental Carbon Measurements

    Published on: September 7, 2019

    结论:

    • 气溶辐射效应是地球气候系统的一个关键因素.
    • 气溶吸收和散射之间的平衡是气候强迫的一个关键决定因素.
    • 监测和准确地表示气溶光学特性对于预测未来气候变化至关重要.