Deriving iron contents from past and future Venus surface spectra with new high-temperature laboratory emissivity data
Author:
Affiliation:
1. DLR Berlin, Berlin, German.
2. Planetary Science Institute, 1700 East Fort Lowell, Suite 106, Tucson, AZ 85719, USA.
3. Department of Astronomy, Mount Holyoke College, 50 College St., South Hadley, MA 01075, USA.
Abstract
Funder
National Aeronautics and Space Administration
H2020 European Research Council
German Academic Exchange Service
Helmholtz Association
Publisher
American Association for the Advancement of Science (AAAS)
Subject
Multidisciplinary
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