Principles Of Planetary Climate

By Marina Bosch. 2016

342 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/a1d7b3b6b9ca35dd772e1df5237d6f6252b7f080

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Citations in the corpus

Transient reducing greenhouse warming on early Mars (2016, unknown): “Because peak valley network formation occurs toward the end of the Noachian, a period of higher impact ﬂux than today [ Fassett and Head , 2008b, 2011], this mechanism deserves detailed investigation in future.”
How to Characterize Habitable Worlds and Signs of Life (2017, background): “First, we will look at climate feedbacks: Positive feedbacks further increase warming (or cooling) due to temperature increase (or decrease), whereas negative feedbacks decrease such warming (or cooling), stabilizing the climate system (see Pierrehumbert 2010).”
HABITABLE ZONES AROUND MAIN-SEQUENCE STARS: DEPENDENCE ON PLANETARY MASS (2014, methodology): “2013; Lissauer et al. 2014; Rowe et al. 2014). Recently Kopparapu et al. (2013) obtained new, improved estimates of the boundaries of the HZ by updating the Kasting et al. (1993) model with new H2O and CO2 absorption coefficients from updated line-by-line databases such as HITRAN 2008 (Rothman et al”
Comparison of “warm and wet” and “cold and icy” scenarios for early Mars in a 3‐D climate model (2015, methodology): “In addition, the thermal inertia was adjusted to 14,500 tiu, corresponding to an ocean mixed layer depth of approximately 50 m [Pierrehumbert, 2011].”
 ?> -REx. II. RETRIEVAL OF EMISSION SPECTRA (2015, background): “We refer the reader to the relevant literature for a more in-depth discussion on the various analytic approaches (e.g. Liou 2002; Hubeny et al. 2003; Hansen 2008; Burrows et al. 2008; Showman et al. 2009; Madhusudhan & Seager 2009; Pierrehumbert 2010; Guillot 2010; Heng et al. 2012, 2014; Robinson &”