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ReportsMercury's Exosphere: Observations During MESSENGER's First Mercury Flyby
During MESSENGER's first Mercury flyby, the Mercury Atmospheric and Surface Composition Spectrometer measured Mercury's exospheric emissions, including those from the antisunward sodium tail, calcium and sodium close to the planet, and hydrogen at high altitudes on the dayside. Spatial variations indicate that multiple source and loss processes generate and maintain the exosphere. Energetic processes connected to the solar wind and magnetospheric interaction with the planet likely played an important role in determining the distributions of exospheric species during the flyby.
1 Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, CO 80303, USA.
2 Department of Physics, University of Central Florida, Orlando, FL 32816, USA. 3 Johns Hopkins University Applied Physics Laboratory, Laurel, MD 20723, USA. 4 Department of Astronomy, University of Maryland, College Park, MD 20742, USA. 5 Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ 85721, USA. 6 Department of Terrestrial Magnetism, Carnegie Institution of Washington, Washington, DC 20015, USA. * To whom correspondence should be addressed. E-mail: william.mcclintock{at}lasp.colorado.edu
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Science. ISSN 0036-8075 (print), 1095-9203 (online)