TO THE QUESTION OF CHOOSING THE MODEL OF WEAK INTERPLANETARY SCINTILLATIONS OF COSMIC SOURCES RADIOEMISSION IN RANGE FROM 8 TO 80 MHZ

Author:

Кuhai N. V., ,Kalinichenko N. N.,

Publisher

National Academy of Sciences of Ukraine (Co. LTD Ukrinformnauka)

Reference36 articles.

1. 1. HEWISH, A., SCOTT, P. F.and WILLS, D., 1964. Interplanetary scintillations of small diameter radio sources. Nature. vol. 203, is. 4951, pp. 1214-1217. DOI: 10.1038/2031214a0

2. 2. RICKETT, B. J., COLES, W. A. and BOURGOIS, G., 1984. Slow scintillations in the interstellar medium. Astron. Astrophys. vol. 134, is. 2, pp. 390-395.

3. 3. COLES, W. A. and KAUFMAN, J. J., 1977. Angular size of the Crab pulsar at 74 MHz. Mon. Not. R. Astron. Soc. vol. 181, is. 1, pp. 57P-59P. DOI: 10.1093/mnras/181.1.57P

4. 4. LEE, L. C. and JOKIPII, J. R., 1975. Strong scintillations in astrophysics. II. A theory of temporal broadening of pulses. Astrophys. J. vol. 201, pp. 532-543. DOI:10.1086/153916

5. 5. FALKOVICH, I. S., KONOVALENKO, A .A., KALINICHENKO, N. N., OLYAK, M. R., GRIDIN, A. A., BUBNOV, I. N., LECACHEUX, A. and RUCKER, H. O., 2006. Variations of parameters of solar wind stream structure outside 1 AU in 2003-2004. Radio Phys. Radio Astron. vol. 11, no. 1, pp. 31-41. (in Russian).

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