Longitude dependences of Saturn's ultraviolet aurora
نویسندگان
چکیده
منابع مشابه
Electron and proton aurora observed spectroscopically in the far ultraviolet
[1] The only way to get a global, instantaneous picture of the energetic particle input over the auroral oval is through spectral imaging. The major driver of auroral emissions in the high-latitude ionosphere is overall electron precipitation. However, for certain locations and times, such as the equatorial edge of the evening auroral oval, proton precipitation can be the major energy source an...
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ژورنال
عنوان ژورنال: Geophysical Research Letters
سال: 2013
ISSN: 0094-8276
DOI: 10.1002/grl.50430