The spinning Astrid-2 satellite used for modeling the Earth's main magnetic field

被引:9
作者
Merayo, JMG [1 ]
Brauer, P
Primdahl, F
Joergensen, PS
Risbo, T
Cain, J
机构
[1] Tech Univ Denmark, Oersted DTU, DK-2800 Lyngby, Denmark
[2] Danish Space Res Inst, DK-2100 Copenhagen, Denmark
[3] Univ Copenhagen, Dept Geophys, DK-2100 Copenhagen, Denmark
[4] Florida State Univ, Inst Geophys Fluid Dynam, Tallahassee, FL 32306 USA
来源
IEEE TRANSACTIONS ON GEOSCIENCE AND REMOTE SENSING | 2002年 / 40卷 / 04期
关键词
amorphous magnetic materials; calibration; data models; data processing; geomagnetism; geophysical inverse problems; magnetic fields; magnetic field measurement; magnetometers; measurement; modeling; satellites;
D O I
10.1109/TGRS.2002.1006371
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
The Swedish micro-satellite Astrid-2 was successfully launched into a near polar orbit in December 1998. Despite the fact that the primary science mission was auroral research, the magnetic instrument was designed to accomplish high-resolution and high-precision vector field magnetic measurements, and therefore mapping of the Earth's magnetic field was possible. The spacecraft spins about a highly stable axis in space. This fact and the globally distributed data make the magnetic measurements well suited for the estimate of a magnetic field model at the spacecraft altitude (about 1000 km). This paper describes the initial analysis of the Astrid-2 magnetic data. As a result of the study of a single day (February 7, 1999), magnetically fairly quiet, it was possible to in-flight adjust the calibration of the magnetometer and find a magnetic field model fitting the scalar component of the measurements to better than 5 nT(rms) for latitudes Equatorward of 50degrees. Several methods for field modeling are discussed in this paper under the assumption that the direction of the spin axis in inertial space is nearly constant, and this assumption is corroborated by the observations. The approximate inertial orientation of the magnetometer could then be determined simultaneously with the instrument intrinsic calibration and the estimate of main field model coefficients. Hence, apart from the scientific use of the magnetic data, the attitude of the spacecraft may be estimated with high precision.
引用
收藏
页码:898 / 909
页数:12
相关论文
共 20 条
[1]   NON-UNIQUENESS OF EXTERNAL GEOMAGNETIC FIELD DETERMINED BY SURFACE INTENSITY MEASUREMENTS [J].
BACKUS, GE .
JOURNAL OF GEOPHYSICAL RESEARCH, 1970, 75 (31) :6339-+
[2]  
BAK T, 1999, THESIS AALBORG U AAL
[3]   Fluxgate sensor for the vector magnetometer onboard the 'Astrid-2' satellite [J].
Brauer, P ;
Risbo, T ;
Merayo, JMG ;
Nielsen, OV .
SENSORS AND ACTUATORS A-PHYSICAL, 2000, 81 (1-3) :184-188
[4]  
CAIN JC, 1985, EOS, V66, P861
[5]   THE MAGNETIC-FIELD OF JUPITER - A GENERALIZED INVERSE APPROACH [J].
CONNERNEY, JEP .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1981, 86 (NA9) :7679-7693
[6]  
Langbein W. E., 1993, IEEE Transactions on Rehabilitation Engineering, V1, P49, DOI 10.1109/86.242408
[7]   THE MAGSAT MISSION [J].
LANGEL, R ;
OUSLEY, G ;
BERBERT, J ;
MURPHY, J ;
SETTLE, M .
GEOPHYSICAL RESEARCH LETTERS, 1982, 9 (04) :243-245
[8]  
LANGEL RA, 1987, GEOMAGN AERON, V2, P249
[9]  
Marklund G, 1997, ESA SP PUBL, V397, P387
[10]   SPATIAL POWER SPECTRA OF THE CRUSTAL GEOMAGNETIC-FIELD AND CORE GEOMAGNETIC-FIELD [J].
MCLEOD, MG ;
COLEMAN, PJ .
PHYSICS OF THE EARTH AND PLANETARY INTERIORS, 1980, 23 (02) :P5-P19