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  2. Atmospheric radiative transfer codes - Wikipedia

    en.wikipedia.org/wiki/Atmospheric_radiative...

    The radiative transfer equation is a monochromatic equation to calculate radiance in a single layer of the Earth's atmosphere. To calculate the radiance for a spectral region with a finite width (e.g., to estimate the Earth's energy budget or simulate an instrument response), one has to integrate this over a band of frequencies (or wavelengths ...

  3. Lunar water - Wikipedia

    en.wikipedia.org/wiki/Lunar_water

    The hypothetical mechanism of water transport / trapping (if any) remains unknown: indeed lunar surfaces directly exposed to the solar wind where water production occurs are too hot to allow trapping by water condensation (and solar radiation also continuously decomposes water), while no (or much less) water production is expected in the cold ...

  4. Solar constant - Wikipedia

    en.wikipedia.org/wiki/Solar_constant

    The solar constant is an average of a varying value. In the past 400 years it has varied less than 0.2 percent. [2] Billions of years ago, it was significantly lower. This constant is used in the calculation of radiation pressure, which aids in the calculation of a force on a solar sail.

  5. Solar irradiance - Wikipedia

    en.wikipedia.org/wiki/Solar_irradiance

    This integrated solar irradiance is called solar irradiation, solar radiation, solar exposure, solar insolation, or insolation. Irradiance may be measured in space or at the Earth's surface after atmospheric absorption and scattering. Irradiance in space is a function of distance from the Sun, the solar cycle, and cross-cycle changes. [2]

  6. Radiative flux - Wikipedia

    en.wikipedia.org/wiki/Radiative_flux

    In geophysics, shortwave flux is a result of specular and diffuse reflection of incident shortwave radiation by the underlying surface. [3] This shortwave radiation, as solar radiation, can have a profound impact on certain biophysical processes of vegetation, such as canopy photosynthesis and land surface energy budgets, by being absorbed into the soil and canopies. [4]

  7. Faint young Sun paradox - Wikipedia

    en.wikipedia.org/wiki/Faint_young_Sun_paradox

    Records of ion implantation from meteorites and lunar samples show that the elevated rate of solar wind flux only lasted for a period of 100 million years. Observations of the young Sun-like star π 1 Ursae Majoris match this rate of decline in the stellar wind output, suggesting that a higher mass loss rate cannot by itself resolve the paradox.

  8. Chinese scientists use lunar soil to produce water, state ...

    www.aol.com/news/chinese-scientists-lunar-soil...

    Chinese scientists have discovered a "brand-new method" of producing large quantities of water using lunar soil brought back from a 2020 expedition, state broadcaster CCTV reported on Thursday. In ...

  9. Simple Model of the Atmospheric Radiative Transfer of Sunshine

    en.wikipedia.org/wiki/Simple_Model_of_the...

    The first versions of SMARTS were developed by Dr. Gueymard while he was at the Florida Solar Energy Center. [2] [3] [4] The model employed a structure similar to the earlier SPCTRAL2 model, still offered by the National Renewable Energy Laboratory (), but with finer spectral resolution, as well as updated extraterrestrial spectrum and transmittance functions.