The data currently available includes solar radio emission measurements and activity measurement at a wavelength of 10.7 cm. This is an optimum wavelength for monitoring the level of solar activity, and
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NOAA NCEI has solar radio legacy datasets from multiple sources over many decades, including the United States Air Force (USAF) Radio Solar Telescope Network (RSTN) stations.
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Solar radio emission refers to radio waves that are naturally produced by the Sun, primarily from the lower and upper layers of the atmosphere called the chromosphere and corona, respectively.
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The solar radio flux at 10.7 cm (2800 MHz) is an excellent indicator of solar activity. Often called the F10.7 index, it is one of the longest running records of solar activity. The F10.7 radio
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The solar radio flux at 10.7 cm (2800 MHz) is an excellent indicator of solar activity. Often called the F10.7 index, it is one of the longest running records of solar activity.
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A serially complete collection of hourly and half-hourly values of meteorological data and the three most common measurements of solar radiation: global horizontal, direct normal and diffuse horizontal
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Radio JOVE is a NASA education and outreach project involving high school and college students in solar and planetary radio astronomy.
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These results will provide a helpful reference for colleagues to make full use of the latest and future observation data obtained from the above solar radio telescopes.
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