Understanding the escape of water from Enceladus

Author:

Burger M. H.1,Sittler E. C.1,Johnson R. E.2,Smith H. T.2,Tucker O. J.2,Shematovich V. I.3

Affiliation:

1. Goddard Space Flight Center; NASA; Greenbelt MD USA

2. University of Virginia; Charlottesville Virginia USA

3. Department of Stellar Physics and Evolution, Institute of Astronomy; Russian Academy of Sciences; Moscow Russia

Publisher

American Geophysical Union (AGU)

Subject

Paleontology,Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Atmospheric Science,Earth-Surface Processes,Geochemistry and Petrology,Soil Science,Water Science and Technology,Ecology,Aquatic Science,Forestry,Oceanography,Geophysics

Reference42 articles.

1. Discovery of an extended sodium atmosphere around Europa;Brown;Nature,1996

2. Burger , M. H. 2003 Io’s neutral clouds: From the atmosphere to the plasma torus University of Colorado, Boulder, Colorado

3. Europa’s neutral cloud: Morphology and comparisons to Io;Burger;Icarus,2004

4. Identification of a dynamic atmosphere at Enceladus with the Cassini magnetometer;Dougherty;Science,2006

5. Emperical model of the state-state dynamics in near-resonant hyperthermal X+ + H2O charge-transfer reactions;Dressler;Int. J. Mass Spectrom.,2006

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