Data for: The Surface Distributions of the Production of the Major Volatile Species, H2O, CO2, CO and O2, from the Nucleus of Comet 67P/Churyumov-Gerasimenko throughout the Rosetta Mission as Measured by the ROSINA Double Focusing Mass Spectrometer

Published: 7 September 2019| Version 1 | DOI: 10.17632/mcckfhybhj.1
Michael Combi, Nicolas Fougere, Valeriy Tenishev, Yinsi Shou, Kenneth Hansen, Zhenguang Huang, David Marshall, Dominique Bockelee-Morvan, Martin Rubin, Kathrin Altwegg, Tamas Gombosi, Gabor Toth, Uwe Fink, Yu-Chi Cheng, Fabrizio Capaccioni


The file MIRO_Columns.txt contains the column densities and their uncertainties corresponding to the results published previously in the paper by Marshall, D.W., Hartogh, P. Rezac, L. von Allmen, P., Biver, N., Bockelée-Morvan, D., Crovisier, J., Encrenaz, P. Bulkis, S. Hofstadter, M. Ip, W.-H., Jarchow, C. Lee, S., Lellouch, E. 2017. Spatially resolved evolution of the local H2O production rates of coet 67P/Churyumov,Gerasimenko, from the MIRO instrument of Rosetta. Astronomy & Astrophysics 603, A87. The format containes space delimited columns corresponding to Date, UT time, Heliocentric Distance (AU), column density (cm^-2), column density error (cm^-2).



Planetary Atmosphere