... smaller number of larger inhomogeneities with a = 45 m, the frequency profile of the ... 1d + 8, n2 = 1.5n0 , n1 = n2 /2, a = 45 m, b = a, N = 10, and B = 5 G (from Laptuhov ...
5. http://www.izmiran.rssi.ru/ionosphere/esound/pdf/IK19_Gulyaeva.pdf
... h 0 5 to p = h 0 5 to p h m F 2 h 0 5 t o p N e 0 5 = 0 .5 N m F 2 : H t o p = 1.3 236 h 0 5 t o p (EISCAT), ISIS1,2 K19 . ... 4 : Rz= 0, 50, 100, 150 |µ |=0, 10,...,90є - 5 (µ ) = jCjpj(u), j=0,1,2,3,4,5 u = (µ -45)/10 t=0, 6, 12, 18 . ...
6. http://www.izmiran.rssi.ru/ionosphere/esound/pdf/Karpachev3.pdf
... M a ui 12 16 20 00 100 50 0 12 16 20 50 0 P oi nt Arguello 0 12 16 20 To m s k 100 50 100 50 12 16 20 50 0 0 12 16 20 Magadan ... P, % 16.5 14.6 10.3 17.3 5.9 10.7 0.05 0.07 6 .6 7 .2 0.04 0.04 , 1032 657 621 668 658 45 6 47 9 45 8 5 III. 30 1979 . ...
7. Ilya M
... by Chertok I. M., Fomichev V.V., Gnezdilov A.A, Gorgutsa R.V., Markeev A.K., and Sobolev D.E. Astronomical and Astrophysical ... 45-52, 2005 . · Large-Scale Activity in Solar Eruptive Events of October-November 2003 by SOHO/EIT Data , . ...
8. The frequency of the spectral maximum fm of the gyrosynchrotron emission vs
... The frequency of the spectral maximum f m of the gyrosynchrotron emission vs. the power-law index of the electron spectrum ... The angle between the line of sight and the magnetic field is 45 degree.. ...
9. The frequency of the spectral maximum fm of the gyrosynchrotron emission vs
... The frequency of the spectral maximum f m of the gyrosynchrotron emission vs. the column density of accelerated electrons ... The angle between the line of sight and the magnetic field is 45 degree.. ...
10. publications
... Т.39. ?5. С.38 - 45. Sorokin V.M., Cherny G.P., 1999. It is quite possible to monitor typhoons from outer space. ... 5. С.38 - 45. Sorokin V.M., Cherny G.P., 1999. It is quite possible to monitor typhoons from outer space. Aerospace courier. ...