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Many of us have calibrated Noise source generators to estimate Background Temperature vs Jovian & Solar radio bursts. But when comparision of results with other radio observatories temperature differences are noted due to equipment. The tempatures are different but the flux density (power landing on square meter per hertz of bandwidth) will be the same. This simple program calculates the flux density of Solar and Jovian storms,as a function of the measured temperatures.
Excellent for NASA JOVE participants and Amateur Radio astronomers.
