Spatially resolved evolution of the local H2O production rates of comet 67P/Churyumov-Gerasimenko from the MIRO instrument on Rosetta-Reference-Cited by-同舟云学术

Spatially resolved evolution of the local H2O production rates of comet 67P/Churyumov-Gerasimenko from the MIRO instrument on Rosetta

Published:2017-07 Issue: Volume:603 Page:A87
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

Marshall D. W.,Hartogh P.,Rezac L.,von Allmen P.,Biver N.,Bockelée-Morvan D.,Crovisier J.,Encrenaz P.,Gulkis S.,Hofstadter M.,Ip W.-H.,Jarchow C.,Lee S.,Lellouch E.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361/201730502/pdf

Reference47 articles.

1. Ancillary data services of NASA's Navigation and Ancillary Information Facility

2. Estimate of the erosion rate from H2O mass-loss measurements from SWAN/SOHO in previous perihelions of comet 67P/Churyumov-Gerasimenko and connection with observed rotation rate variations

3. The water production rate of Rosetta target Comet 67P/Churyumov–Gerasimenko near perihelion in 1996, 2002 and 2009 from Lyman α observations with SWAN/SOHO

4. Comparison of 3D kinetic and hydrodynamic models to ROSINA-COPS measurements of the neutral coma of 67P/Churyumov-Gerasimenko

5. Distribution of water around the nucleus of comet 67P/Churyumov-Gerasimenko at 3.4 AU from the Sun as seen by the MIRO instrument on Rosetta

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