Behavior of planetary dynamos under the influence of external magnetic fields: Application to Mercury and Ganymede

被引:12
作者
Gomez-Perez, Natalia [1 ]
Wicht, Johannes [2 ]
机构
[1] Carnegie Inst Washington, Dept Terr Magnetism, Washington, DC 20015 USA
[2] Max Planck Inst Solar Syst Res, D-37191 Katlenburg Lindau, Germany
关键词
Planetary dynamics; Magnetic fields; Magnetospheres; Mercury; Interior; Ganymede; Terrestrial planets; SPHERICAL-SHELL GEOMETRY; CONVECTION; MODELS; IO; MAGNETOCONVECTION; GENERATION; DIPOLAR; EUROPA; CORE;
D O I
10.1016/j.icarus.2010.04.006
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
For planets with strong intrinsic magnetic fields such as Earth and Jupiter, an external magnetic field is unlikely to affect the internal dynamo, but for bodies with weak intrinsic fields in appropriate environments. such as Mercury and Ganymede, the interaction with near by Field sources may determine the internal dynamics and overall behavior of their liquid iron cores On the basis of simulations of such interactions using numerical models for fluid flow and dynamo generation, the parameter regimes for stable dipolar and multipolar reversing dynamo magnetic fields established for isolated systems can be substantially changed by the action of external sources Relatively weak external background fields (as low as 2% of the averaged undisturbed field at the core-mantle boundary) may change the energy balance and alter the regime over which natural isolated dynamos operate (C) 2010 Elsevier Inc All rights reserved
引用
收藏
页码:53 / 62
页数:10
相关论文
共 41 条
[1]   Crustal remanence in an internally magnetized non-uniform shell: a possible source for Mercury's magnetic field? [J].
Aharonson, O ;
Zuber, MT ;
Solomon, SC .
EARTH AND PLANETARY SCIENCE LETTERS, 2004, 218 (3-4) :261-268
[2]   Varying the spherical shell geometry in rotating thermal convection [J].
Al-Shamali, FM ;
Heimpel, MH ;
Aurnou, JM .
GEOPHYSICAL AND ASTROPHYSICAL FLUID DYNAMICS, 2004, 98 (02) :153-169
[3]   The structure of Mercury's magnetic field from MESSENGER's first flyby [J].
Anderson, Brian J. ;
Acuna, Mario H. ;
Korth, Haje ;
Purucker, Michael E. ;
Johnson, Catherine L. ;
Slavin, James A. ;
Solomon, Sean C. ;
McNutt, Ralph L., Jr. .
SCIENCE, 2008, 321 (5885) :82-85
[4]   The production of Ganymede's magnetic field [J].
Bland, Michael T. ;
Showman, Adam P. ;
Tobie, Gabriel .
ICARUS, 2008, 198 (02) :384-399
[5]   The magnetic field of the planet-hosting star τ Bootis [J].
Catala, C. ;
Donati, J. -F. ;
Shkolnik, E. ;
Bohlender, D. ;
Alecian, E. .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2007, 374 (01) :L42-L46
[6]   Non-ideal liquidus curve in the Fe-S system and Mercury's snowing core [J].
Chen, Bin ;
Li, Jie ;
Hauck, Steven A., II .
GEOPHYSICAL RESEARCH LETTERS, 2008, 35 (07)
[7]   Scaling properties of convection-driven dynamos in rotating spherical shells and application to planetary magnetic fields [J].
Christensen, U. R. ;
Aubert, J. .
GEOPHYSICAL JOURNAL INTERNATIONAL, 2006, 166 (01) :97-114
[8]   Models of magnetic field generation in partly stable planetary cores: Applications to Mercury and Saturn [J].
Christensen, Ulrich R. ;
Wicht, Johannes .
ICARUS, 2008, 196 (01) :16-34
[9]   A deep dynamo generating Mercury's magnetic field [J].
Christensen, Ulrich R. .
NATURE, 2006, 444 (7122) :1056-1058
[10]  
COWLING TG, 1957, INTERSCIENCE TRACTS, V4, P13