High-resolution magnetic field modeling: application to MAGSAT and Ørsted data

[1]  B. Langlais,et al.  Observatory crustal magnetic biases during MAGSAT and Ørsted satellite missions , 2002 .

[2]  Mioara Mandea,et al.  The southern edge of cratonic North America: Evidence from new satellite magnetometer observations , 2002 .

[3]  Mioara Mandea,et al.  Small-scale structure of the geodynamo inferred from Oersted and Magsat satellite data , 2002, Nature.

[4]  Mioara Mandea,et al.  An IGRF candidate main geomagnetic field model for epoch 2000 and a secular variation model for 2000–2005 , 2000 .

[5]  S. Macmillan,et al.  International Geomagnetic Reference Field—the eighth generation , 2000 .

[6]  R. Holme,et al.  Modelling of attitude error in vector magnetic data: application to Ørsted data , 2000 .

[7]  Mioara Mandea,et al.  Ørsted Initial Field Model , 2000 .

[8]  Jeremy Bloxham,et al.  The treatment of attitude errors in satellite geomagnetic data , 1996 .

[9]  R. Langel,et al.  Toward an Improved Distribution of Magnetic Observatories for Modeling of the Main Geomagnetic Field and Its Temporal Change. , 1995 .

[10]  M. Alexandrescu,et al.  Geographical Distribution of Magnetic Observatories and Field Modelling , 1994 .

[11]  Jeremy Bloxham,et al.  Time‐dependent mapping of the magnetic field at the core‐mantle boundary , 1992 .

[12]  Walter H. F. Smith,et al.  Free software helps map and display data , 1991 .

[13]  J. Cain,et al.  Derivation of a geomagnetic model to n=63 , 1989 .

[14]  D. Barraclough International geomagnetic reference field: the fourth generation , 1987 .

[15]  Robert A. Langel,et al.  The near‐Earth magnetic field at 1980 determined from Magsat data , 1985 .

[16]  D. Barraclough A comparison of satellite and observatory estimates of geomagnetic secular variation , 1985 .

[17]  J. Cain,et al.  The use of Magsat data to determine secular variation , 1983 .

[18]  S. R. C. Malin,et al.  The direction of the Earth's magnetic field at London, 1570-1975 , 1981, Philosophical Transactions of the Royal Society of London. Series A, Mathematical and Physical Sciences.

[19]  R. Hide How to locate the electrically conducting fluid core of a planet from external magnetic observations , 1978, Nature.

[20]  F. Lowes,et al.  Spatial Power Spectrum of the Main Geomagnetic Field, and Extrapolation to the Core , 1974 .

[21]  George E. Backus,et al.  APPLICATION OF A NON-LINEAR BOUNDARY-VALUE PROBLEM FOR LAPLACE'S EQUATION TO GRAVITY AND GEOMAGNETIC INTENSITY SURVEYS , 1968 .

[22]  Robert A. Langel,et al.  A Proposed Model for the International Geomagnetic Reference Field-1965 , 1967 .

[23]  B. Langlais Les champs magnétiques de la Terre et de Mars : apport des satellites Ørsted et Mars Global Surveyor , 2001 .

[24]  J. Mouel,et al.  Time Variations of the Earth's Magnetic Field: From Daily to Secular , 1988 .