Erika L. Barth, Ph.D.
Affiliations: | 2004 | University of Colorado, Boulder, Boulder, CO, United States |
Area:
Astronomy and Astrophysics, Atmospheric Science Physics, GeophysicsGoogle:
"Erika Barth"Mean distance: 1936
Cross-listing: Meteorology Tree
Parents
Sign in to add mentorOwen Brian Toon | grad student | 2004 | CU Boulder | |
(Microphysical modeling of clouds in Titan's atmosphere.) |
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Publications
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Barth EL. (2017) Modeling survey of ices in Titan's stratosphere Planetary and Space Science. 137: 20-31 |
Barth EL, Farrell WM, Rafkin SCR. (2016) Electric field generation in martian dust devils Icarus. 268: 253-265 |
Spiga A, Barth E, Gu Z, et al. (2016) Large-Eddy Simulations of Dust Devils and Convective Vortices Space Science Reviews. 1-31 |
Harrison RG, Barth E, Esposito F, et al. (2016) Applications of Electrified Dust and Dust Devil Electrodynamics to Martian Atmospheric Electricity Space Science Reviews. 1-47 |
Charnay B, Barth E, Rafkin S, et al. (2015) Methane storms as a driver of Titan’s dune orientation Nature Geoscience. 8: 362-366 |
Rafkin SCR, Barth EL. (2015) Environmental control of deep convective clouds on Titan: The combined effect of CAPE and wind shear on storm dynamics, morphology, and lifetime Journal of Geophysical Research E: Planets. 120: 739-759 |
Barth EL. (2010) Cloud formation along mountain ridges on Titan Planetary and Space Science. 58: 1740-1747 |
Barth EL, Rafkin SCR. (2010) Convective cloud heights as a diagnostic for methane environment on Titan Icarus. 206: 467-484 |
Barth EL, Rafkin SCR. (2007) TRAMS: A new dynamic cloud model for Titan's methane clouds Geophysical Research Letters. 34 |
Barth EL, Toon OB. (2006) Methane, ethane, and mixed clouds in Titan's atmosphere: Properties derived from microphysical modeling Icarus. 182: 230-250 |