Полярные геомагнитные возмущения и связанные с ними явления : материалы международного симпозиума «Полярные геомагнитные явления», 25-31 мая 1986 г., Суздаль / Междунар. геодез. и геофиз. союз, междунар. ассоциация геомагнетизма и аэрономии, АН СССР, КНЦ, ПГИ. – Апатиты : [б. и.], 1989.

0 -1 1 0 -1 1 0 -1 1 0 -1 1 а -1 1 0 -1 1 а -1 1 о -1 1 W 0 i w f mmmmnmi mi 1 < w 2 W , % w4 1 < W f f v/g v j ■ ! h 10 го -40 •60 Hit,»? ! А IS.01 26.01 27.01.74 IPh 25.01 И н?м ~2Ш ----7 m w а / У MPh2 И RPh -10 '20 i S y , » r 21.01 им п.п п т а -------- \ р / Pig. 1. W a l s h funotions (N»0*7) in Paley (W ) and Gray (ч’д) coae. Pig. 2. The ro u g h i n g off examples of AE(t), Dst(t) an d By(t) parameters w i t h the 0.95 p r e c i sion (thin line) for *.ha storm 2. The precise data are g i v e n b y the thiolc line. conclusions we use the data of analysis of the two concrete GMS: the storm of F e bruary 15-18, 1967 (storm 1), the storm of J anuary 24-27, 1974 (storm 2) /3/. 13 initial and 16 "derivative" processes has been u s e d i n the a n a l y sis r epr e s e n t e d by 64 h o u r l y data each. These processes ("parameters") ha v e b e e n c h aracterizing separate components of the complex. So, i n t e r p lanetary m e d i u m has b e e n d e scribed by vel o c i t y v , density n , an d temperature T of solar w i n d pr o t o n component, intensity В of Interplanetary m a gnetic field (IMP), its compon e nts В , b v , I +в coordinates, dia p e r a i o n tr2 В • I in solar m a gnetoapheric of B 2 component, longitude ч a n d latitude 0 „ of vector В ative" parameters, s u c h as i n solar-ecliptio coordinates and b y a set of other "derlv- 2 __2 _„S v P. В V ( m n v 2 )1 / 3 , £ , B z at . ---- „ --- ,_ ,) at B z > B ~ < ° t 1 ni? * ( M ^ / 4 f m n v 2 ) 1 / ^ М ц - 8 . 6 1 0 2 5 Bcrz - * B2>* BaV' V - „ Pp - B 2 /ein3 (8/2)/|VrT, where B Q proton mass, 6 • a r o t g ( l B v /B LCP H V ‘, n v " , E „ = * v B z, E z ^ v b y , E T - V B T - VB 2 s i n ^ ( © / 2ДQp, OP B t < 0 at B z > 0. m is ■arctg(t By / B z I) at g- cm 3 . Geomagnetosphere has been and B z ■ 0 and 8 « 180° • 64