How did the solar wind structure change around the solar maximum? From interplanetary scintillation observation

Annales Geophysicae

Volumn 21, Issue 6, 2003, Pages 1257-1261

  Fujiki, K ^a   Kojima, M ^a   Tokumaru, M ^a   Ohmi, T ^a   Yokobe, A ^a   Hayashi, K ^a   McComas, D J ^b   Elliott, H A ^b  

^a NAGOYA UNIVERSITY   (Japan)

^b SOUTHWEST RESEARCH INSTITUTE   (United States)

Author keywords

Interplanetary physics (solar wind plasma); Radio science (remote sensing)

Indexed keywords

COSMIC RAY; SOLAR PHENOMENA; SOLAR WIND;

EID: 0042848784     PISSN: 09927689     EISSN: None     Source Type: Journal    
DOI: 10.5194/angeo-21-1257-2003     Document Type: Article

References (6)

1. McComas, D. J., Balogh, A., Bame, S. J., Barraclough, B. L., Feldman, W. C., Forsyth, R., Goldstein, B. E., Gosling, J. T., Funsten, H. O., Neugebauer, M., Riley, P., and Skoug, R.: Ulysses' return to the slow solar wind, Geophys. Res. Lett., 25, 1-4. 1998.
2. McComas, D. J., Elliott, H. A., Gosling, J. T., Reisenfeld, D. B., Skoug, R. M., Goldstein, B. E., Neugebauer, M., and Balogh. A.: Ulysses' second fast-latitude scan: Complexity near solar maximum and the reformation of polar coronal holes, Geophys. Res. Lett., 29(9), 10.1029/2001GL014164, 2002.
3. Kojima, M., Tokumaru, M., Watanabe, H., Yokobe. A., Asai, K., Jackson, B. V., and Hick, P. L.: Heliospheric tomography using interplanetary scintillation observations. 2, Latitude and heliospheric distance dependence of solar wind structure at 0.1-1 AU. J. Geophys Res., 103, 1981-1989, 1998.
4. Kojima, M., Fujiki, K., Ohmi, T., Tokumaru, M., Yokobe, V., and Hakamada, K.: Latitudinal Velocity Structures up to the Solar Poles Estimated from IPS Tomography Analysis, J. Geophys. Res. 106, 15677-15 686, 2001.
5. Kojima, M., Fujiki, K., Tokumaru, M., Ohmi, T., Shimizu, Y., Yokobe, A., Jackson, B. V., and Hick, P. L.: Tomographic Analysis of Solar Wind Structure Using Interplanetary Scintillation, COSPAR Colloquium Series, Vol. 12. 55-59, Proc. COSPAR Colloquium "Space Weather Study Using Multi-point Techniques." 2002.
6. Ohmi, T.: The Origin of the Low-speed Solar Wind, Ph.D. thesis, to be published, 2003.