Physics of auroral phenomena : proceedings of the 33rd Annual seminar, Apatity, 02 - 05 March, 2010 / [ed.: A.G. Yahnin, A. A. Mochalov]. - Апатиты : Издательство Кольского научного центра РАН, 2011. - 206 с. : ил.

M.Forster at al Table. Magnetospheric magnetic field values as measured by Cluster C3 and obtained from the T01, T96, and PM models together with the results of the mapping along the magnetic field lines into the ionosphere at 400 km height. Date UT Xgsm Re Ygsm Re Zgsm Re R Re BXgsm nT BYgsm nT BZgsm nT |B|, nT Geo Lat Geo Long -28.77 -3.68 -6.47 29.72 CL 11.08.07 04:42 -14.58 -5.78 -10.66 18.96 -30.47 -27.91 -4.26 -6.30 -4.53 -5.21 31.09 29.08 -81.30° -82.54° 85.96° 88.00° T01 T96 -22.52 -4.52 -4.74 23.46 -82.52° 43.55° PM -60.48 -2.24 -14.36 62.20 CL 19.08.06 12:19 -10.44 -4.32 -11.32 15.99 -53.41 -53.78 -2.88 -9.06 -10.06 -16.21 54.42 56.90 -81.61° -81.06° 138.79° 137.13° T01 T96 -35.47 -5.83 -10.40 37.42 -84.01° 134.20° PM -46.89 -1.90 -12.86 48.66 CL 25.08.07 17:39 -10.31 -0.76 -11.93 15.79 -41.58 -37.76 -3.45 -2.74 -10.91 -14.04 43.12 40.37 -75.14° -74.48° 127.32° 126.37° T01 T96 -31.72 -1.90 -10.33 33.41 -78.75° 110.22° PM -40.84 6.42 -20.35 46.08 CL 02.09.06 20:50 -8.00 1.75 -12.47 14.92 -42.68 -37.48 4.68 5.10 -17.45 -18.56 46.34 42.13 -76.99° -76.59° 128.45° 122.23° T01 T96 -33.32 3.92 -14.81 36.67 -80.98° 97.51° PM 29.62 -20.10 5.56 36.22 CL 01.11.05 00:14 -9.96 10.74 0.60 14.64 17.41 5.26 -17.43 -15.20 4.03 13.52 24.96 21.01 58.46° 59.62° 294.86° 296.48° T01 T96 20.60 -10.53 6.09 23.92 61.15° 290.74° PM 50.78 -5.43 -3.91 51.22 CL 11.09.02 00:56 -12.02 0.33 6.87 13.85 54.94 50.38 -0.84 -0.85 -4.80 -5.13 55.16 50.64 69.61° 69.01° 318.84° 320.31° T01 T96 37.70 -0.60 -2.21 37.76 67.93° 320.79° PM 57.10 7.39 -14.32 59.33 CL 21.08.05 10:39 -8.18 -1.93 7.52 11.27 53.54 54.24 6.72 7.18 -9.02 -12.18 54.71 56.05 69.48° 68.91° 240.80° 239.84° T01 T96 48.67 7.03 -7.18 49.70 69.69° 245.09° PM 60.10 6.50 -2.38 60.50 CL 10.09.06 18:56 -9.27 -1.33 4.46 10.38 57.88 59.76 2.67 4.10 3.72 -1.91 58.06 59.93 74.11° 72.75° 79.56° 79.20° T01 T96 51.72 5.13 7.1 52.45 79.07° 61.28° PM 98.55 -54.52 -25.01 115.37 CL 31.10.05 16:56 -5.96 4.61 4.76 8.91 101.36 95.53 -53.49 -61.39 -24.63 -23.84 117.22 116.03 75.86° 75.37° 37.79° 45.97° T01 T96 73.49 -51.64 -15.30 91.11 76.78° 21.35° PM 131.02 -10.50 -118.50 176.98 CL 05.10.03 23:35 -3.42 0.39 6.70 7.53 112.35 119.02 -14.95 -15.51 -112.43 -119.60 159.65 169.44 78.84° 79.01° 309.36° 308.24° T01 T06 105.48 -11.78 -109.52 152.51 76.02° 312.23° PM References Alexeev, I.I., E. S. Belenkaya, V.V. Kalegaev, Y.I. Feldstein, A. Grafe, Magnetic storms and magnetotail currents, J. Geophys. Res., 101, 7737 - 7747, 1996. Balogh A., et al., The Cluster magnetic field investigations: overview of in-flight performance and initial results, Ann.Geophys., 19, 1207-1217, 2001 . Feldstein Y. I., A. H. Levitin, J. U. Kozyra, В. T. Tsurutani, A. Prigancova, L. Alperovich, W. D. Gonzalez, U. Mall, I. 1. Alexeev, L. I. Gromova, L. A. Dremukhina, Self-consistent modeling of the large-scale distortions in the geomagnetic field during the 24-27 September 1998 major magnetic storm, J. Geophys. Res., 110, Al 1214, doi: 10.1029/2004JA010584, 2005. F6rster М., G. Paschmann, S. E. Haaland et al., High-latitude plasma convection from Cluster EDI: Variances and solar wind correlations, Ann. Geophys., 25, 1691, 2007. Fflrster М., S. E. Haaland, Paschmann G. et al., High-latitude plasma convection during northward IMF as derived from in-situ magnetospheric Cluster EDI measurements, Ann. Geophys., 26,2685,2008. Forster М., Y. I. Feldstein, S. E. Haaland, L. A. Dremukhina, L. I. Gromova, A. E. Levitin, Magnetospheric convection from Cluster EDI measurements compared with the ground-based ionospheric convection model IZMEM, Ann. Geophys., 27, 3077 - 3087, 2009. Haaland S.E., G. Paschmann, M. Forster et al., High-latitude plasma convection from Cluster EDI measurements: method and IMF-dependence, Ann. Geophys., 25, 239, 2007. Reme H., J. M. Bosqued, J. A. Sauvaud et al., The Cluster ion spectrometry (CIS) experiment, Space Science Reviews, 79, 303 - 350, 1997. Tsyganenko N. A., Effects of the solar wind conditions on the global magnetospheric configuration as deduced from data-based field models, ESA SP-389,181-185,1996. Tsyganenko N. A., A model of the near magnetosphere with a dawn-dusk asymmetry. 2. Parameterization and fitting to observations, J. Geophys. Res.,\01, 1176, doi: 1029/2001JA000220, 2002. Woodfield E. E., M. W. Dunlop, R. Holme, J. A. Davies, M. A. Hapgood, A comparison of Cluster magnetic data with the Tsyganenko 2001 model, J. Geophys. Res., 112, A06248, doi: 10.1029/2006JАО12217,2007. 62