Hydrogen-alpha auroral activity on Jupiter

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Astronomical Photography, Auroras, H Alpha Line, Jupiter Atmosphere, Planetary Radiation, Doppler Effect, Nonthermal Radiation, Planetary Magnetic Fields, Radio Emission, Solar Activity Effects

Scientific paper

This paper deals with an attempt to observe H-alpha auroral activity on Jupiter. Photographs in H-alpha light were taken of the planet in the spring and summer of 1972 in Tampa, Florida, utilizing a 26-inch Schmidt-Cassegrain telescope. This investigation and many others have been undertaken because Jupiter has been shown to have a strong magnetic field and to emit nonthermal radiation at various radio wavelengths; these properties seem to be related to magnetic fields and solar activity.

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