Chihiro Tao

TL;DR: In this paper, the response of the Jovian magnetosphere to solar wind dynamic pressure enhancements was investigated by simulating a one-dimensional magnetohydrodynamic propagation of the solar wind from the Earth.

TL;DR: In this article, the ionospheric response to auroral precipitation at the giant planets is reviewed, using models and observations The emission processes for aurorae at radio, infrared, visible, ultraviolet, and X-ray wavelengths are described, and exemplified using ground-and space-based observations Comparisons between the emissions at different wavelengths are made, where possible, and interpreted in terms of precipitating particle characteristics or atmospheric conditions.

TL;DR: In this article, the first comparison of Jupiter's auroral morphology with an extended, continuous and complete set of near-Jupiter interplanetary data was presented, revealing the response of the planet's auroras to the interplanar conditions.

TL;DR: In this paper, the authors presented evidence provided by the new Hisaki spacecraft and the Hubble Space Telescope that showed that such brightening of Jupiter's aurora can in fact be internally driven.

TL;DR: The relationship between electron energy flux and the characteristic energy of electron distributions in the main auroral loss cone has been inferred from remote sensing observations of the Jovian aurora, primarily from the Hubble Space Telescope, and also more recently from Hisaki as mentioned in this paper.