UV Io footprint leading spot: A key feature for understanding the UV Io footprint multiplicity?
نویسندگان
چکیده
منابع مشابه
The Io UV footprint: Location, inter-spot distances and tail vertical extent
[1] The Io footprint (IFP) consists of one or several spots observed in both jovian hemispheres and is related to the electromagnetic interaction between Io and the magnetosphere. These spots are followed by an auroral curtain, called the tail, extending more than 90 longitude in the direction of planetary rotation. We use recent Hubble Space Telescope images of Jupiter to analyze the location ...
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[1] The Io footprint (IFP) is the auroral signature of the electromagnetic interaction between Io and Jupiter’s magnetosphere. It consists of several spots followed by an extended tail, which are located close to the feet of the magnetic field lines connecting Io to Jupiter. The size of the main spot is a controversial issue, and previously published values range from ∼400 to ∼8000 km. However,...
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ژورنال
عنوان ژورنال: Geophysical Research Letters
سال: 2008
ISSN: 0094-8276
DOI: 10.1029/2007gl032418