The turbulent structure of the solar wind from observations in the decameter radio wavelength range

被引：0

作者：

Braude, SY ^{[1
]}

Galanin, VV ^{[1
]}

Inyutin, GA ^{[1
]}

Men, AV ^{[1
]}

Mori, K ^{[1
]}

Rashkovskii, SL ^{[1
]}

Sinitsyn, VG ^{[1
]}

Sharykin, NK ^{[1
]}

机构：

[1] TOKYO COMMUN RES LAB,TOKYO,JAPAN

来源：

ASTRONOMICHESKII ZHURNAL | 1995年 / 72卷 / 05期

关键词：

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Results of observations of scattering of the decameter radio emission of a compact object in the source 3C 144 on inhomogeneities in the electron density of the solar wind plasma over a wide range of elongation on the URAN-1 and URAN-4 radio interferometers with baselines 42.3 and 613 km are presented. The experimental relationships obtained are compared with calculations made for a power law inhomogeneity spectrum. Dependences of the results of the calculations on a number of solar wind plasma parameters are presented, and probable values for these parameters are estimated.

引用

页码：761 / 766

页数：6

共 50 条

[31] EVIDENCE FOR THE SOLAR CORPUSCULAR ORIGIN OF THE DECAMETER-WAVELENGTH RADIATION FROM JUPITER
CARR, TD
SMITH, AG
BOLLHAGEN, H
PHYSICAL REVIEW LETTERS, 1960, 5 (09) : 418 - 420
[32] DETERMINATION OF THE PARAMETERS OF THE SPATIAL-DISTRIBUTION OF EXTRAGALACTIC RADIO-SOURCES OBSERVED IN THE DECAMETER-WAVELENGTH RANGE
SOKOLOV, KP
ASTRONOMICHESKII ZHURNAL, 1986, 63 (03): : 426 - 433
[33] FINE STRUCTURE IN METER WAVELENGTH SOLAR RADIO BURSTS
PHILIP, KW
ASTRONOMICAL JOURNAL, 1968, 73 (10P2): : S197 - &
[34] High-Latitude Inner Solar Wind from Pulsar Radio Sounding Observations
I. V. Chashei
V. I. Shishov
T. V. Smirnova
Solar Physics, 2010, 265 : 129 - 135
[35] High-Latitude Inner Solar Wind from Pulsar Radio Sounding Observations
Chashei, I. V.
Shishov, V. I.
Smirnova, T. V.
SOLAR PHYSICS, 2010, 265 (1-2) : 129 - 135
[36] Solar wind structure dynamics by multipoint observations
Zastenker, GN
Dalin, PA
Petrukovich, AA
Nozdrachev, MN
Romanov, SA
Paularena, KI
Richardson, JD
Lazarus, AJ
Lepping, RP
Szabo, A
PHYSICS AND CHEMISTRY OF THE EARTH PART C-SOLAR-TERRESTIAL AND PLANETARY SCIENCE, 2000, 25 (1-2): : 137 - 140
[37] Structure of thermal radio emission from the atmosphere in the middle part of the submillimeter wavelength range
Kitai S.D.
Naumov A.P.
Osharina N.N.
Radiophysics and Quantum Electronics, 2002, 45 (02) : 147 - 152
[38] Observations of magnetic reconnection in the turbulent high-speed solar wind
Gosling, J. T.
ASTROPHYSICAL JOURNAL LETTERS, 2007, 671 (01) : L73 - L76
[39] Solar wind cluster observations: Turbulent spectrum and role of Hall effect
Alexandrova, O.
Carbone, V.
Veltri, P.
Sorriso-Valvo, L.
PLANETARY AND SPACE SCIENCE, 2007, 55 (15) : 2224 - 2227
[40] Fine structure of the solar wind turbulence inferred from simultaneous radio occultation observations at widely-spaced ground stations
Bird, MK
Janardhan, P
Efimov, AI
Samoznaev, LN
Andreev, VE
Chashei, IV
Edenhofer, P
Plettemeier, D
Wohlmuth, R
SOLAR WIND TEN, PROCEEDINGS, 2003, 679 : 465 - 468

← 1 2 3 4 5 →