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.

OCTOBER 1979 I к. V km/e г 500 -«00 -300 ТТ TAT ТА А** АА АА АА АА АА 1--- 1___ I--- 1--- 1--- 1___ I___ I___ I -3 -2 -1 0 1 2 3 4 зо 20 10- FEBRUARY 1978 500 -400 300 fig. 3. The ваше ав in JPig.1. P e r t u rbation in the polarity of the IMP b y the ne w M o o n is flhown i n a d d i tion. There are 112 perturb atione -out of total 145 investigated peripds, i.e. 77 per cent of the canes. ТТ T - ТА T- I___ 1___ I--- U -4 -3 -2 -1 0 1 2 3 JULY 1874 30л 20 10 J -500 -400 -300 TT IT AAT ATT ТТ ТТ TT I T i--- 1___ i___ i___ i___ i i i -4 - 3 -2 -1 0 1 2 3 perturbance i n the p o l a r i t y only. Correlative a n a l y s i s . As is k n o w n as early as in the 60-s a close r e l a t i o n b e t w e e n the phenomena o b served i n the solar w i n d and aotce g e o m a g n e tic processes was distinguished. As a basic c h aracteristic we have chosen the three h o u r pl a n e t a r y K p - i n d e x and its derivative Kp. One of the first wo r k s indicating the correlative rel a t i o n s h i p of the aolar w i n d ve l o c i t y to the m a gnetospheric a c t i v i t y /9/ is the work, where: S K p O ( K M / s ) - ^ 3 0 ± 1 7 ) ] / ( 8 , 4 4 ± 0 . 7 4 ) . Subsequently, a n u m b e r of other relations o f the K p - i n d e x to the parameters of the int e r p l a n e t a r y m e d i u m w a s e s t a blished /10,11/. In this w o r k we shall try to find the r e l a t i o n of the solar w i n d v elocity V to K p d e pending o n the lunar phase in or d e r to e s t a b l i s h wh e t h e r the magne t o h y d r o d y n a m i c a l wake of the M o o n c hanges this r e l a t i o n by the aero day. Рог this purpose all d iurnal periods (-4, +4 days) of the n e w M o o n were ana l y z e d during the period 1970-1985 and the c o r r e l a t i o n coefficient R wa s I05