Note to users. If you're seeing this message, it means that your browser cannot find this page's style/presentation instructions -- or possibly that you are using a browser that does not support current Web standards. Find out more about why this message is appearing, and what you can do to make your experience of our site the best it can be.

Site Tools

  • AAAS
  • Subscribe
  • Feedback

Site Search

Search Advanced

Science 9 December 1994:
Vol. 266. no. 5191, pp. 1675 - 1678
DOI: 10.1126/science.266.5191.1675
Prev | Table of Contents | Next

Articles

A Remarkable Auroral Event on Jupiter Observed in the Ultraviolet with the Hubble Space Telescope

J. C. Gérard 1, D. Grodent 1, V. Dols 1, R. Prangé 2, J. H. Waite 3, G. R. Gladstone 3, K. A. Franke 3, F. Paresce 4, A. Storrs 4, and L. Ben Jaffel 5

1 Laboratoire de Physique Atmosphérique et Planétaire, Institut d'Astrophysique, Université de Liége, Belgium
2 Institut d'Astrophysique Spatiale and Institut d'Astrophysique de Paris, Université de Paris Sud, Orsay, France
3 Southwest Research Institute, San Antonio, TX, 78228-0570, USA.
4 Space Telescope Science Institute, Baltimore, MD 21218, USA.
5 Institut d'Astrophysique de Paris, France

Two sets of ultraviolet images of the Jovian north aurora were obtained with the Faint Object Camera on board the Hubble Space Telescope. The first series shows an intense discrete arc in near corotation with the planet. The maximum apparent molecular hydrogen emission rate corresponds to an electron precipitation of sim1 watt per square meter, which is about 30,000 times larger than the solar heating by extreme ultraviolet radiation. Such a particle heating rate of the auroral upper atmosphere of Jupiter should cause a large transient temperature increase and generate strong thermospheric winds. Twenty hours after initial observation, the discrete arc had decreased in brightness by more than one order of magnitude. The time scale and magnitude of the change in the ultraviolet aurora leads us to suggest that the discrete Jovian auroral precipitation is related to large-scale variations in the current system, as is the case for Earth's discrete aurorae.

Submitted on July 11, 1994
Accepted on September 27, 1994


THIS ARTICLE HAS BEEN CITED BY OTHER ARTICLES:
Dark Auroral Oval on Saturn Discovered in Hubble Space Telescope Ultraviolet Images.
L. B. Jaffel, V. Leers, and B. R. Sandel (1995)
Science 269, 951-953
   Abstract »    PDF »
ROSAT Observations of X-ray Emissions from Jupiter During the Impact of Comet Shoemaker-Levy 9.
J. H. Waite Jr., G. R. Gladstone, K. Franke, W. S. Lewis, A. C. Fabian, W. N. Brandt, C. Na, F. Haberl, J. T. Clarke, K. C. Hurley, et al. (1995)
Science 268, 1598-1601
   Abstract »    PDF »


ADVERTISEMENT
Click Me!

ADVERTISEMENT
Click Me!

To Advertise     Find Products

Science. ISSN 0036-8075 (print), 1095-9203 (online)