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.

Science 27 September 1991:
Vol. 253. no. 5027, pp. 1528 - 1531
DOI: 10.1126/science.253.5027.1528
Prev | Table of Contents | Next

Articles

Plasma Observations at Venus with Galileo

L. A. FRANK 1, W. R. PATERSON 1, K. L. ACKERSON 1, F. V. CORONITI 2, and V. M. VASYLIUNAS 3

1 Department of Physics and Astronomy, University of Iowa, Iowa City, IA 52242
2 Departments of Physics and Astronomy, University of California, Los Angeles, CA 90024
3 Max-Planck-Institut für Aeronomie, Postfach 20, W-3411 Katlenburg-Lindau, Germany

Plasma measurements were obtained with the Galileo spacecraft during an approximately 3.5-hour interval in the vicinity of Venus on 10 February 1990. Several crossings of the bow shock in the local dawn sector were recorded before the spacecraft passed into the solar wind upstream from this planet. Although observations of ions of the solar wind and the postshock magnetosheath plasmas were not possible owing to the presence of a sunshade for thermal protection of the instrument, solar wind densities and bulk speeds were determined from the electron velocity distributions. A magnetic field—aligned distribution of hotter electrons or ``strahl'' was also found in the solar wind. Ions streaming into the solar wind from the bow shock were detected. Electron heating at the bow shock, le20%, was notably small, with substantial density increases by factors of 2 to 3 at the day side of the shock that decrease for shock crossings further downstream from the planet. A search for pickup ions from the hot hydrogen and oxygen planetary coronas yielded an upper limit for these densities in the range of 10-3 ion per cubic centimeter, which is consistent with densities expected from current models of neutral gas densities.

Revised on April 26, 1991
Accepted on July 9, 1991


THIS ARTICLE HAS BEEN CITED BY OTHER ARTICLES:
Magnetic Field Studies of the Solar Wind Interaction with Venus from the Galileo Flyby.
M. G. KIVELSON, C. F. KENNEL, R. L. MCPHERRON, C. T. RUSSELL, D. J. SOUTHWOOD, R. J. WALKER, C. M. HAMMOND, K. K. KHURANA, R. J. STRANGEWAY, and P. J. COLEMAN (1991)
Science 253, 1518-1522
   Abstract »    PDF »
Lightning and Plasma Wave Observations from the Galileo Flyby of Venus.
D. A. GURNETT, W. S. KURTH, A. ROUX, R. GENDRIN, C. F. KENNEL, and S. J. BOLTON (1991)
Science 253, 1522-1525
   Abstract »    PDF »
Energetic Particles at Venus: Galileo Results.
D. J. WILLIAMS, R. W. MCENTIRE, S. M. KRIMIGIS, E. C. ROELOF, S. JASKULEK, B. TOSSMAN, B. WILKEN, W. STUDEMANN, T. P. ARMSTRONG, T. A. FRITZ, et al. (1991)
Science 253, 1525-1528
   Abstract »    PDF »


To Advertise     Find Products

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