Generation of planetary magnetism by convection

Physics of the Earth and Planetary Interiors

Volumn 12, Issue 4, 1976, Pages 350-358

  Busse, F H ^a  

^a UNIVERSITY OF CALIFORNIA   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0001164961     PISSN: 00319201     EISSN: None     Source Type: Journal    
DOI: 10.1016/0031-9201(76)90030-3     Document Type: Article

References (24)

1. Kinematic models of the earth's hydromagnetic dynamo
2. Magnetic waves in the earth's core
3. Saturn radio emission near 1 MHz
4. Thermal instabilities in rapidly rotating systems
5. Differential rotation in stellar convection zones
6. Generation of magnetic fields by convection
7. The nonlinear dynamo problem
8. A model of the geodynamo
9. Numerical solutions of the kinematic dynamo problem
10. Free hydromagnetic oscillations of the earth's core and the theory of geomagnetic secular variation
11. Structure of Jupiter and Saturn
12. Precession of the earth as the cause of geomagnetism
13. Convection at the melting point a thermal history of the earth's core
14. The magnetic field of Mercury Part 1
15. Models of the giant planets
16. On finite amplitude convection in rotating magnetic system
17. An ancient lunar magnetic dipole field
18. On the interpretation of lunar magnetism
19. Mercury: Internal structure and thermal evolution
20. Measuring the magnetic fields of Jupiter and the outer solar system
21. A convection driven dynamo
22. Thermal evolution and the present state of the moon and terrestrial planets
23. Venus: An upper limit on intrinsic magnetic dipole movement based on absence of a radiation belt
24. Temperatures inside Mars Is the core liquid or solid?