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Episodic warming of early Mars by punctuated volcanism
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“Hence for pure clear-sky CO 2 -H 2 O atmospheres under early Martian conditions, modern radiativeconvective models obtain mean surface temperatures of 225 K or less (Wordsworth, Forget & Eymet 2010; Ramirez et al. 2014; Halevy & Head 2014).”
From The Climate of Early Mars (2016) · cites this paper as Halevy & Head 2014
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Cites
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Research works printed but not linked: 1
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Metadata
- Authors
- Halevy, I., & Head III, J. W.
- Affiliations
- Weizmann Institute of Science (IL)
- Corresponding author
- Halevy, Itay
- ORCID
- Halevy, Itay
- Venue
- Nature Geoscience
- Published
- 2014-11-17
- Volume
- 7
- Issue
- 12
- Pages
- 865-868
- ISSN
- 1752-0894 (ISSN-L)
- 1752-0908
- OpenAlex
- W2054092907
- Cited by
- 179
- References
- 30
- Citations by year
- 2026: 4 · 2025: 8 · 2024: 6 · 2023: 6 · 2022: 11 · 2021: 22 · 2020: 23 · 2019: 16 · 2018: 22 · 2017: 24 · 2016: 17 · 2015: 18 · 2014: 2
- FWCI
- 10.96
- Type
- journal article
- Language
- en
- Open access
- closed
- Licence
- www.springer.com/tdm (tdm)
- Locations
- Nature Geoscience (publishedVersion)
- Topics
- Physical Sciences › Earth and Planetary Sciences › Space and Planetary Science › Planetary Science and Exploration
- Physical Sciences › Earth and Planetary Sciences › Space and Planetary Science › Astro and Planetary Science
- Physical Sciences › Earth and Planetary Sciences › Atmospheric Science › Geology and Paleoclimatology Research
- Keywords
- early Mars climate, volcanic eruptions, sulfur dioxide, hydrogen sulfide, sulfate aerosols, global warming, liquid water on Mars, aerosol microphysics, Mars atmosphere, valley networks
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