C/NOFS measurements of magnetic perturbations in the low-latitude ionosphere during magnetic storms

被引:21
作者
Le, Guan [1 ]
Burke, William J. [2 ,3 ]
Pfaff, Robert F. [1 ]
Freudenreich, Henry [1 ]
Maus, Stefan [4 ]
Luehr, Hermann [5 ]
机构
[1] NASA, Space Weather Lab, Heliophys Sci Div, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[2] USAF, Space Vehicles Directorate, Res Lab, Hanscom AFB, MA 01731 USA
[3] Boston Coll, Inst Sci Res, Chestnut Hill, MA 02167 USA
[4] NOAA, Natl Geophys Data Ctr, Boulder, CO 80305 USA
[5] GFZ German Res Ctr Geosci, D-14473 Potsdam, Germany
关键词
TIME MAGNETOSPHERIC CURRENTS; RING CURRENT; INNER MAGNETOSPHERE; GEOMAGNETIC STORMS; TAIL CURRENT; FIELD; DST; EARTH; DISTURBANCE;
D O I
10.1029/2011JA017026
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The Vector Electric Field Investigation suite on the C/NOFS satellite includes a fluxgate magnetometer to monitor the Earth's magnetic fields in the low-latitude ionosphere. Measurements yield full magnetic vectors every second over the range of +/- 45,000 nT with a one-bit resolution of 1.37 nT ( 16 bit A/D) in each component. The sensor's primary responsibility is to support calculations of both V x B and E x B with greater accuracy than can be obtained using standard magnetic field models. The data also contain information about large-scale current systems that, when analyzed in conjunction with electric field measurements, promise to significantly expand understanding of equatorial electrodynamics. We first compare in situ measurements with the POMME (Potsdam Magnetic Model of the Earth) model to establish in-flight sensor "calibrations" and to compute magnetic residuals. At low latitudes the residuals are predominately products of the storm time ring current. Since C/NOFS provides a complete coverage of all local times every 97 min, magnetic field data allow studies of the temporal evolution and local time variations of storm time ring current. The analysis demonstrates the feasibility of using instrumented spacecraft in low-inclination orbits to extract a timely proxy for the provisional Dst index and to specify the ring current's evolution.
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页数:11
相关论文
共 27 条
[1]  
[Anonymous], 1991, INT ASS GEOMAGN AERO
[2]   DIRECT-DETECTION OF SOLAR-WIND DYNAMIC PRESSURE EFFECT ON GROUND GEOMAGNETIC-FIELD [J].
ARAKI, T ;
FUNATO, K ;
IGUCHI, T ;
KAMEI, T .
GEOPHYSICAL RESEARCH LETTERS, 1993, 20 (09) :775-778
[3]  
Bowman B. R, 2008, ASTR SPEC C AM I AER
[4]   Estimating Dst indices and exospheric temperatures from equatorial magnetic fields measured by DMSP satellites [J].
Burke, W. J. ;
Wilson, G. R. ;
Lin, C. S. ;
Rich, F. J. ;
Wise, J. O. ;
Hagan, M. P. .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 2011, 116
[5]   C/NOFS:: a mission to forecast scintillations [J].
de La Beaujardière, O .
JOURNAL OF ATMOSPHERIC AND SOLAR-TERRESTRIAL PHYSICS, 2004, 66 (17) :1573-1591
[6]   C/NOFS observations of deep plasma depletions at dawn [J].
de La Beaujardiere, Odile ;
Retterer, John M. ;
Pfaff, Robert F. ;
Roddy, Patrick A. ;
Roth, Christopher ;
Burke, William J. ;
Su, Yi Jiun ;
Kelley, Michael C. ;
Ilma, Ronald R. ;
Wilson, Gordon R. ;
Gentile, Louise C. ;
Hunton, Donald E. ;
Cooke, David L. .
GEOPHYSICAL RESEARCH LETTERS, 2009, 36
[7]   HYDROMAGNETIC THEORY OF GEOMAGNETIC STORMS [J].
DESSLER, AJ ;
PARKER, EN .
JOURNAL OF GEOPHYSICAL RESEARCH, 1959, 64 (12) :2239-2252
[8]   Statistical distribution of the storm-time proton ring current: POLAR measurements [J].
Ebihara, Y ;
Ejiri, M ;
Nilsson, H ;
Sandahl, I ;
Milillo, A ;
Grande, M ;
Fennell, JF ;
Roeder, JL .
GEOPHYSICAL RESEARCH LETTERS, 2002, 29 (20) :30-1
[9]   Effects of induced currents on Dst and on magnetic variations at midlatitude stations -: art. no. 1014 [J].
Häkkinen, LVT ;
Pulkkinen, TI ;
Nevanlinna, H ;
Pirjola, RJ ;
Tanskanen, EI .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 2002, 107 (A1)
[10]  
Iyemori T, 1996, ANN GEOPHYS, V14, P608, DOI 10.1007/s00585-996-0608-3