Zobrazeno 1 - 10
of 231
pro vyhledávání: '"Solomon, SC"'
Autor:
Gettelman, A, Mills, MJ, Kinnison, DE, Garcia, RR, Smith, AK, Marsh, DR, Tilmes, S, Vitt, F, Bardeen, CG, McInerney, J, Liu, H, Solomon, SC, Polvani, LM, Emmons, LK, Lamarque, J, Richter, JH, Glanville, AS, Bacmeister, JT, Phillips, AS, Neale, RB, Simpson, IR, DuVivier, AK, Hodzic, A, Randel, WJ
The Whole Atmosphere Community Climate Model version 6 (WACCM6) is a major update of the whole atmosphere modeling capability in the Community Earth System Model (CESM), featuring enhanced physical, chemical and aerosol parameterizations. This work d
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=core_ac_uk__::8b7df997f24ce80d8121d65c39ccfc08
https://eprints.whiterose.ac.uk/152722/8/2019JD030943.pdf
https://eprints.whiterose.ac.uk/152722/8/2019JD030943.pdf
We conducted global simulations of temperature change due to anthropogenic trace gas emissions, which extended from the surface, through the thermosphere and ionosphere, to the exobase. These simulations were done under solar maximum conditions, in o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=core_ac_uk__::237d7fa78464e9c5a5cc64e419a67392
https://eprints.whiterose.ac.uk/147734/8/2019JA026678.pdf
https://eprints.whiterose.ac.uk/147734/8/2019JA026678.pdf
We performed simulations of the atmosphere‐ionosphere response to the solar eclipse of 21 August 2017 using the Whole Atmosphere Community Climate Model‐eXtended (WACCM‐X v. 2.0) with a fully interactive ionosphere and thermosphere. Eclipse sim
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=core_ac_uk__::d6dd3ad0a5a095522862fae9170ebd9b
https://eprints.whiterose.ac.uk/131565/1/mcinerney_grl2018.pdf
https://eprints.whiterose.ac.uk/131565/1/mcinerney_grl2018.pdf
Autor:
Liu, J, Liu, H, Wang, W, Burns, AG, Wu, Q, Gan, Q, Solomon, SC, Marsh, DR, Qian, L, Lu, G, Pedatella, NM, McInerney, JM, Russell III, JM, Schreiner, WS
New ionosphere and electrodynamics modules have been incorporated in the thermosphere and ionosphere eXtension of the Whole Atmosphere Community Climate Model (WACCM‐X), in order to self‐consistently simulate the coupled atmosphere‐ionosphere s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=core_ac_uk__::7f694866894af0be15cecf6dffe997b7
https://eprints.whiterose.ac.uk/131568/1/lui_j_jgrspace_2018.pdf
https://eprints.whiterose.ac.uk/131568/1/lui_j_jgrspace_2018.pdf
We simulated anthropogenic global change through the entire atmosphere, including the thermosphere and ionosphere, using the Whole Atmosphere Community Climate Model‐eXtended. The basic result was that even as the lower atmosphere gradually warms,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=core_ac_uk__::7d3ead817518344d075807410fb73402
https://eprints.whiterose.ac.uk/131562/1/solomon_grl2018.pdf
https://eprints.whiterose.ac.uk/131562/1/solomon_grl2018.pdf
Publikováno v:
Peale, SJ; Margot, JL; Hauck, SA; & Solomon, SC. (2016). Consequences of a solid inner core on Mercury's spin configuration. Icarus, 264, 443-455. doi: 10.1016/j.icarus.2015.09.024. UCLA: Retrieved from: http://www.escholarship.org/uc/item/0s31k8hr
© 2015 Elsevier Inc. The pressure torque by a liquid core that drove Mercury to the nominal Cassini state of rotation is dominated by the torque from the solid inner core. The gravitational torque exerted on Mercury's mantle from an asymmetric solid
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::9a612f3c1548e823dc7e930e72590225
https://escholarship.org/uc/item/0s31k8hr
https://escholarship.org/uc/item/0s31k8hr