Magnetic energy distribution in the four-dimensional frequency and wave vector domain in the solar wind

Journal of Geophysical Research: Space Physics

Volumn 115, Issue 4, 2010, Pages

  Narita, Y ^a   Sahraoui, F ^b   Goldstein, M L ^b   Glassmeier, K H ^a,c  

^a TECHNICAL UNIVERSITY OF BRAUNSCHWEIG   (Germany)

^b NASA GODDARD SPACE FLIGHT CENTER   (United States)

^c MAX PLANCK INSTITUT FÜR SONNENSYSTEMFORSCHUNG   (Germany)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 77950661990     PISSN: None     EISSN: 21699402     Source Type: Journal    
DOI: 10.1029/2009JA014742     Document Type: Article

References (23)

1. Coles, W. A., B. J. Rickett, V. H. Rumsey, J. J. Kaufman, D. G. Turley, S. Ananthakrishnan, J. W. Armstrong, J. K. Harmons, S. L. Scott, and D. G. Sime (1980), Solar cycle changes in the polar solar wind, Nature, 286, 239-241.
2. Dennison, P. A., and A. Hewish (1967), The solar wind outside the plane of the ecliptic, Nature, 213, 343-346.
3. Fujiki, K., M. Kojima, M. Tokumaru, T. Ohmi, A. Yokobe, K. Hayashi, D. J. McComas, and H. A. Elliott (2003), How did the solar wind structure change around the solar maximum? - From interplanetary scintillation observation, Ann. Geophys, 21, 1257-1261. (Pubitemid 36906422)
4. Hakamada, K., and M. Kojima (1999), Solar wind speed and expansion rate of the coronal magnetic field during Carrington rotation 1909, Sol. Phys., 187, 115-122. (Pubitemid 37133143)
5. Hoeksema, T. (1995), The large-scale structure of the heliospheric current sheet during the Ulysses epoch, Space Sci. Rev., 72, 137-148.
6. Hoeksema, J. T., J. M. Wilcox, and P. H. Scherrer (1983), The structure of the heliospheric current sheet: 1978-1982, J. Geophys. Res., 88, 9910-9918.
7. Hundhausen, A. J., R. T. Hansen, and S. F. Hansen (1981), Coronal evolution during the sunspot cycle: Coronal holes observed with Mauna Loa K-coronameters, J. Geophys. Res., 86, 2079-2094.
8. Issautier, K., G. Le Chat, N. Meyer-Vernet, M. Monecuquet, S. Hoang, R. J. MacDowall, and D. J. McComas (2008), Electron properties of high-speed solar wind from polar coronal holes obtained by Ulysses thermal noise spectroscopy: Not so dense, not so hot, Geophys. Res. Lett., 35, L19101, doi:10.1029/ 2008GL034912.
9. Kojima, M., and T. Kakinuma (1987), Solar cycle evolution of solar wind speed structure between 1973 and 1985, J. Geophys. Res., 92, 7269-7279.
10. Kojima, M., and T. Kakinuma (1990), Solar cycle dependence of global distribution of solar wind speed, Space Sci. Rev., 53, 173-222.
11. Kojima, M., M. Tokumaru, H. Watanabe, A. Yokobe, K. Asai, B. V. Jackson, and P. L. Hick (1998), Heliospheric tomography using interplanetary scintillation observations: 2. Latitude and heliocentric distance dependence of solar wind structure at 0.1-1 AU, J. Geophys. Res., 103, 1981-1989. (Pubitemid 128664978)
12. Kojima, M., K. Fujiki, M. Hirano, M. Tokumaru, T. Ohmi, and K. Hakamada (2004), Solar wind properties from IPS observations, in The Sun and Heliosphere as an Integrated System, edited by G. Poletto and S. T. Suess, chap. 6, pp. 147-178, Kluwer Acad., Norwell, Mass.
13. Kojima, M., M. Tokumaru, K. Fujiki, K. Hayashi, and B. V. Jackson (2007), IPS tomographic observations of 3D solar wind structure, Astron. Astrophys. Trans., 26, 467-476, doi:10.1080/10556790701596200.
14. Lee, C. O., J. G. Luhmann, X. P. Zhao, Y. Liu, P. Riley, C. N. Arge, C. T. Russell, and I. de Pater (2009), Effects of the weak polar fields of solar cycle 23: Investigation using OMNI for the STEREO mission period, Sol. Phys., 256, 345-363.
15. Luhmann, J. G., C. O. Lee, Y. Li, C. N. Arge, A. B. Galvin, K. Simunac, C. T. Russell, R. A. Howard, and G. Petric (2009), Solar wind sources in the late declining phase of cycle 23: Effects of the weak solar polar field on high speed streams, Sol. Phys., 256, 285-305.
16. McComas, D. J., et al. (1998), Solar Wind Electron Proton Alpha Monitor (SWEPAM) for the Advanced Composition Explorer, Space Sci. Rev., 86, 563-612.
17. McComas, D. J., R. W. Ebert, H. A. Elliot, B. E. Goldstein, J. T. Gosling, N. A. Schwadron, and R. M. Skoug (2008), Weaker solar wind from the polar coronal holes and the whole Sun, Geophys. Res. Lett., 35, L18103, doi:10.1029/2008GL034896.
18. Rickett, B. J., and W. A. Coles (1991), Evolution of the solar wind structure over a solar cycle: Interplanetary scintillation velocity measurements compared with coronal observations, J. Geophys. Res., 96, 1717-1736.
19. Smith, E. J., and A. Balogh (2008), Decrease in heliospheric magnetic flux in this solar minimum: Recent Ulysses magnetic field observations, Geophys. Res. Lett., 35, L22103, doi:10.1029/2008GL035345.
20. Suzuki, T. K. (2006), Forecasting solar wind speeds, Astrophys. J., 640, L75-L78.
21. Svalgaard, L., T. L. Duvall Jr., and P. H. Scherrer (1978), The strength of the Sun's polar fields, Sol. Phys. 58, 225-240.
22. Tokumaru, M., M. Kojima, K. Fujiki, and K. Hayashi (2009), Non-dipolar solar wind structure observed in the cycle 23/24 minimum, Geophys. Res. Lett., 36, L09101, doi:10.1029/2009GL037461.
23. Wang, Y.-M., and N. R. Sheeley Jr. (1990), Solar wind speed and coronal flux-tube expansion, Astrophys. J., 355, 726-732.