Physics
Scientific paper
Dec 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004agufmsa13b..01t&link_type=abstract
American Geophysical Union, Fall Meeting 2004, abstract #SA13B-01
Physics
7536 Solar Activity Cycle (2162), 7538 Solar Irradiance, 7549 Ultraviolet Emissions, 2479 Solar Radiation And Cosmic Ray Effects, 0358 Thermosphere: Energy Deposition
Scientific paper
Solar soft X-ray (XUV) and Vacuum Ultraviolet (VUV) spectral irradiances are particularly important for space system engineering, aeronomy, and climate change research since these wavelengths deposit their energy in the thermosphere, mesosphere, and stratosphere as well as create the ionosphere. Because solar spectral irradiances are a foundation for understanding scattering and photoabsorption processes in atmospheres and ionospheres, it is important to provide user communities with accurate, precise and time-resolved solar irradiance products. We present an overview of the solar irradiance community's recent space-based measurements and empirical as well as physics-based modeling for short (minutes to hours), medium (hours to days), and long (weeks to months) time scale irradiance variations as related to energy deposition processes for the thermosphere and ionosphere. In addition, we describe the ISO 21348 standard which provides a common process for determining solar irradiances.
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