... m f(x) x н nвm Ф Г Г Г Г Г Г Г Г Г Г Г Г Г Г Г Г Г Г Г Г Г Г Г Г Г Г Г Г Г Г Г Г Г Г ... n m rang A = m ( n m , rang A < m ). x B mвm, , , . , A 1.3. ... M = -µ s r, 2r r r3 r r = r ; -- , r ; s = Gm -- , S. C S FS = -G Mm r m = µc r , 2r ...
... Galeev A.A., and A.M.Sadovski, Solar wind acceleration by the dissipation o f Alfven waves, Astrophysics and Space Science, 264, 101-112, 1999. ...
... Denton, M. H., Thomsen, M. F., Korth, H., Lynch, S., Zhang, J. C., and Liemohn, M. W ... M. H., Borovsky, J. E., Skoug, R. M., Thomsen, M. F., Lavraud, B., Henderson, M. G ...
... Yamamoto, T., S. Inoue, N. Nishitani, M. Ozaki, and C.-I. Meng, A theory for generation of the paired region 1 and region 2 ... Res. , 101 , 27199-27222, 1996. See also: . Space Physics Text Book of Oulu. ...
... m 2 nd layer - transition layer defined by ( = 10 - 103 Om x m diurnal or seasonal ... m. B. Small station HFS sounding with Antenna size ( 0.5 m. and Low-frequency ... m * m, I=1A) less than 3 - current output (A) 1 or 3 (selectable) -Period of ...
... M.Yu., and Lodkina, I.G., Comment on "A Statistical Comparison of Solar Wind Sources of Moderate and Intense Geomagnetic Storms at Solar Minimum and Maximum" by Zhang, J.-C., M.W. Liemohn, J.U. Kozyra, M.F. Thomsen, H.A. Elliott, and J. M. Weygand, JGR ...
... Petrinec, S. M., and C. T. Russell, Near-Earth magnetotail shape and size as determined from the magnetopause flaring angle, J ... 101, 137, 1996. ...
... leading to large geomagnetic storms: Similar and individual characteristics I.S. Veselovsky a a,b,* , M.I. Panasyuk a, Yu.I. Yermolaev b, L.M. Zelenyi b Skobel'tsyn Institute of Nuclear Physics (SINP), Moscow State University, Moscow 119992, Russia b ...