Zobrazeno 1 - 10
of 10
pro vyhledávání: '"Krista M. Soderlund"'
Autor:
Natalia Gómez-Pérez, Carol Paty, Steven D. Vance, M. J. Styczinski, Corey J. Cochrane, Krista M. Soderlund, Bruce G. Bills
To date, analyses of magnetic induction in putative oceans in Jupiter's large icy moons have assumed uniform conductivity in the modeled oceans. However, the phase and amplitude response of the ind...
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::9bfd24d350731111867278a320985009
https://doi.org/10.1002/essoar.10502420.1
https://doi.org/10.1002/essoar.10502420.1
Autor:
Krista M. Soderlund, Johannes Wicht, Wieland Dietrich, Jonathan M. Aurnou, Christopher T. Russell, Hao Cao
Publikováno v:
Geophysical Research Letters. 41:4127-4134
Recent MErcury Surface, Space ENvironment, GEochemistry, and Ranging (MESSENGER) measurements have shown that Mercury's magnetic field is axial-dominant, yet strongly asymmetric with respect to the equator: the field strength in the Northern Hemisphe
Publikováno v:
Icarus, vol 224, iss 1
The ice giant planets, Uranus and Neptune, have magnetic fields, atmospheric circulation patterns, and thermal emissions that are distinct from other planets in our Solar System. However, no self-consistent dynamical model has been able to reproduce
Publikováno v:
Earth and Planetary Science Letters. :9-20
The magnetic fields of planets and stars are thought to play an important role in the fluid motions responsible for their field generation, as magnetic energy is ultimately derived from kinetic energy. We investigate the influence of magnetic fields
Publikováno v:
Progress in Earth and Planetary Science, vol 2, iss 1
Fluid motions within planetary cores generate magnetic fields through dynamo action. These core processes are driven by thermo-compositional convection subject to the competing influences of rotation, which tends to organize the flow into axial colum
Autor:
Michael A. Calkins, Krista M. Soderlund, Jonathan S. Cheng, Stephan Stellmach, David Nieves, E.M. King, Keith Julien, Jonathan M. Aurnou
Publikováno v:
Aurnou, JM; Calkins, MA; Cheng, JS; Julien, K; King, EM; Nieves, D; et al.(2015). Rotating convective turbulence in Earth and planetary cores. Physics of the Earth and Planetary Interiors, 246, 52-71. doi: 10.1016/j.pepi.2015.07.001. UCLA: Retrieved from: http://www.escholarship.org/uc/item/97s3x12h
© 2015 Elsevier B.V. An accurate description of turbulent core convection is necessary in order to build robust models of planetary core processes. Towards this end, we focus here on the physics of rapidly rotating convection. In particular, we pres
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7875d638c2b69473500143271dafea60
https://escholarship.org/uc/item/97s3x12h
https://escholarship.org/uc/item/97s3x12h
Autor:
Gerald Schubert, Krista M. Soderlund
Publikováno v:
Physics of the Earth and Planetary Interiors. 187:92-108
The state of knowledge and understanding of planetary magnetic fields is reviewed. All of the planets, with the possible exception of Venus, have had active dynamos at some time in their evolution. The properties and characteristics of the dynamos ar
Publikováno v:
Earth and Planetary Science Letters, vol 392
Soderlund, KM; King, EM; & Aurnou, JM. (2014). Corrigendum to "The influence of magnetic fields in planetary dynamo models" [Earth Planet. Sci. Lett. 333-334 (2012) 9-20]. Earth and Planetary Science Letters, 392, 121-123. doi: 10.1016/j.epsl.2014.01.052. UCLA: Retrieved from: http://www.escholarship.org/uc/item/08t8k3vp
Soderlund, KM; King, EM; & Aurnou, JM. (2014). Corrigendum to "The influence of magnetic fields in planetary dynamo models" [Earth Planet. Sci. Lett. 333-334 (2012) 9-20]. Earth and Planetary Science Letters, 392, 121-123. doi: 10.1016/j.epsl.2014.01.052. UCLA: Retrieved from: http://www.escholarship.org/uc/item/08t8k3vp
Earth and Planetary Science Letters 392 (2014) 121–123 Contents lists available at ScienceDirect Earth and Planetary Science Letters www.elsevier.com/locate/epsl Corrigendum Corrigendum to “The influence of magnetic fields in planetary dynamo m
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7eb70b56d0a6f9285101439259d92822
https://escholarship.org/uc/item/08t8k3vp
https://escholarship.org/uc/item/08t8k3vp
Publikováno v:
Geochemistry, Geophysics, Geosystems. 11
[1] The magnetic fields of planets and stars are generated by the motions of electrically conducting fluids within them. These fluid motions are thought to be driven by convective processes, as internal heat is transported outward. The efficiency wit
Autor:
Dale P. Cruikshank, B. J. Buratti, Krista M. Soderlund, Michael D. Hicks, James M. Bauer, Ralf Jaumann, Robert H. Brown, J. A. Mosher, D. P. Simonelli, Roger N. Clark, Tom Momary
Three weeks prior to the commencement of Cassini's 4 year tour of the saturnian system, the spacecraft executed a close flyby of the outer satellite Phoebe. The infrared channel of the Visual Infrared Mapping Spectrometer (VIMS) obtained images of re
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b91612dd677d1aa32a13e472c64153c1
https://elib.dlr.de/61559/
https://elib.dlr.de/61559/