A comparison of Cluster magnetic data with the Tsyganenko 2001 model

Journal of Geophysical Research: Space Physics

Volumn 112, Issue 6, 2007, Pages

  Woodfield, E E ^a   Dunlop, M W ^b   Holme, R ^a   Davies, J A ^b   Hapgood, M A ^b  

^a UNIVERSITY OF LIVERPOOL   (United Kingdom)

^b RUTHERFORD APPLETON LABORATORY   (United Kingdom)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 34548355319     PISSN: None     EISSN: 21699402     Source Type: Journal    
DOI: 10.1029/2006JA012217     Document Type: Article

References (17)

1. Balogh, A., et al. (2001), The Cluster Magnetic Field Investigation: Overview of in-flight performance and initial results, Ann. Geophys., 19, 1207-1217.
2. Blakely, R. J. (1996), Potential Theory in Gravity and Magnetic Applications, Cambridge Univ. Press, New York.
3. Covington, A. E. (1969), Solar radio emission at 10.7 cm, J. R. Astron. Soc. Canada, 63, 125.
4. Dunlop, M. W., A. Balogh, K.-H. Glassmeier, and P. Robert (2002), Four-point Cluster application of magnetic field analysis tools: The Curlometer, J. Geophys. Res., 107(A11), 1384, doi:10.1029/2001JA005088.
5. Escoubet, C. P., M., Fehringer, and M. Goldstein (2001), The Cluster mission - Introduction, Ann. Geophys., 19(10-12), 1197-1200.
6. Iijima, T., and T. A. Potemra (1976), Amplitude distribution of field-aligned currents at northern high latitudes observed by Triad, J. Geophys. Res., 81, 2165-2174.
7. Maus, S., et al. (2005), The 10th-generation international geomagnetic reference field, Geophys. J. Int., 161, 561-565.
8. McComas, D. J., B. S. J. P.Bame, W. C. Feldman, J. L. Phillips, P. Riley, and J. W. Griffee (1998), Solar Wind Electron Proton Alpha Monitor (SWEPAM) for the Advanced Composition Explorer, Space Sci. Rev., 86, 563-612.
9. Sabaka, T. J., N. Olsen, and R. A. Langel (2004), Extending comprehensive models of the Earth's magnetic field with Oersted and Champ data, Geophys. J. Int., 159, 521-547.
10. Shue, J. H., et al. (1998), Magnetopause location under extreme solar wind conditions, J. Geophys. Res., 103(A8), 17,691-17,700.
11. Smith, C. W., J. L'Heureux, N. F. Ness, M. H. Acuña, L. F. Burlaga, and J. Scheifele (1998), The ACE Magnetic Fields Experiment, Space Sci. Rev., 86, 613-632.
12. Sugiura, M., and T. Kamei (1991), Equatorial DST index 1957-1986, in IAGA Bull. 40, edited by A. Bethelier and M. Menvielle, Int. Serv. of Geomagn., Indices Publ. Off., Saint Maur, France.
13. Tsyganenko, N. A. (2002a), A model of the near magnetosphere with a dawn-dusk asymmetry: 1. Mathematical structure, J. Geophys. Res., 107(A8), 1179, doi:10.1029/2001JA000219.
14. Tsyganenko, N. A. (2002b), A model of the near magnetosphere with a dawn-dusk asymmetry: 2. Parameterization and fitting to observations, J. Geophys. Res., 107(A8), 1176, doi:10.1029/2001JA000220.
15. Vallat, C., I. Dandouras, M. Dunlop, A. Balogh, E. Lucek, G. K. Parks, M. Wilber, E. C. Roelof, G. Chanteur, and H. Reme (2005), First current density measurements in the ring current region using simultaneous multi-spacecraft CLUSTER-FGM data, Ann. Geophys., 23, 1849-1865.
16. Wanliss, J. A., and K. M. Showalter (2006), High-resolution global storm index: Dst versus SYM-H, J. Geophys. Res., 111, A02202, doi:10.1029/2005JA011034.
17. Wilken, B., et al. (2001), First results from the RAPID imaging energetic particle spectrometer on board Cluster, Ann. Geophys., 19(10-12), 1355-1366.