Episodic warming of early Mars by punctuated volcanism
By I. Halevy, James W. Head III. 2014
183 citations recorded by the source corpus.
Subfields: Aerospace Engineering, Astronomy and Astrophysics
View Paper: https://www.semanticscholar.org/paper/bb2bd1fee740498a7e63e74dfcf69880280a613e
How researchers see this paper
The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.
In Aerospace Engineering
In Astronomy and Astrophysics
- R. Wordsworth
- E. Kite
- Francois Forget
- James W. Head III
- R. Pierrehumbert
- L. Kerber
- Ehouarn Millour
- L. Kaltenegger
Citations in the corpus
- Transient reducing greenhouse warming on early Mars (2016, unknown): “, 2002], sulfur dioxide emission from volcanos [ Postawko and Kuhn , 1986; Halevy and Head , 2014], and local snowmelt due to diurnal forcing and/or obliquity and eccentricity variations [e.g., Wordsworth et al. , 2013].”
- Geologic Constraints on Early Mars Climate (2018, background): “Such eruptions would last < 30 yr (Halevy & Head 2014, Kerber et al. 2015).”
- Comparison of “warm and wet” and “cold and icy” scenarios for early Mars in a 3‐D climate model (2015, background): “…of melting processes in marginally warm scenarios may still allow for significant fluvial erosion, as evidenced by geomorphic studies of the McMurdo Dry Valleys in Antarctica [Head and Marchant, 2014] and recent modeling of top-down melting from a late Noachian icesheet [Fastook and Head, 2014].”