Fine Structure of the Solar Wind Turbulence Inferred from Simultaneous Radio Occultation Observations at Widely-Spaced Ground Stations

AIP Conference Proceedings

Volumn 679, Issue , 2003, Pages 465-468

  Bird, M K ^a   Janardhan, P ^b   Efimov, A I ^c   Samoznaev, L N ^c   Andreev, V E ^c   Chashei, I V ^d   Edenhofer, P ^e   Plettemeier, D ^e   Wohlmuth, R ^e  

^a UNIVERSITY OF BONN   (Germany)

^b PHYSICAL RESEARCH LABORATORY   (India)

^c INSTITUTE OF RADIO ENGINEERING AND ELECTRONICS   (Russian Federation)

^d LEBEDEV PHYSICAL INSTITUTE   (Russian Federation)

^e RUHR UNIVERSITY BOCHUM   (Germany)

Author keywords

[No Author keywords available]

Indexed keywords

TURBULENCE;

CORONAL RADIO SOUNDINGS; CROSS-CORRELATION COEFFICIENT; HELIOCENTRIC DISTANCES; SIMULTANEOUS OBSERVATION; SOLAR WIND DENSITY; SOLAR-WIND TURBULENCE; TEMPORAL FREQUENCY; ULYSSES SPACECRAFT;

SOLAR WIND;

EID: 84908054810     PISSN: 0094243X     EISSN: 15517616     Source Type: Conference Proceeding    
DOI: 10.1063/1.1618635     Document Type: Conference Paper

References (8)

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8. Wohlmuth, R., Plettemeier, D., Edenhofer, P, Bird, M. K., Efimov, A. I, Andreev, V. E., Samoznaev, L. N., Chashei, I. V., 2001, Radio frequency fluctuation spectra during the solar conjunctions of the Ulysses and Galileo spacecraft, Space Sci. Rev. 97, 9-12.