Excess open solar magnetic flux from satellite data: 1. Analysis of the third perihelion Ulysses pass

Journal of Geophysical Research: Space Physics

Volumn 114, Issue 11, 2009, Pages

  Lockwood, M ^a,b   Owens, M ^c   Rouillard, A P ^a,b  

^a UNIVERSITY OF SOUTHAMPTON   (United Kingdom)

^b RUTHERFORD APPLETON LABORATORY   (United Kingdom)

^c IMPERIAL COLLEGE LONDON   (United Kingdom)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 72149123635     PISSN: None     EISSN: 21699402     Source Type: Journal    
DOI: 10.1029/2009JA014449     Document Type: Article

References (28)

1. Arge, C. N., and V. J. Pizzo (2000), Improvement in the prediction of solar wind conditions using near-real time solar magnetic field updates, J. Geophys. Res., 105, 10,465-10,479, doi:10.1029/1999JA000262.
2. Balogh, A., E. J. Smith, B. T. Tsurutani, D. J. Southwood, F. J. Forsyth, and T. S. Horbury (1995), The heliospheric field over the south polar region of the Sun, Science, 268,1007-1010, doi:10.1126/science.268.5213.1007.
3. Burlaga, L. F., and E. Barouch (1976), Interplanetary stream magnetism: Kinematic effects, Astrophys. J., 203, 257-267, doi: 10.1086/154074.
4. Gosling, J. T. (1996), Co-rotating and transient solar wind flows in three dimensions, Annu. Rev. Astron. Astrophys., 34, 35-73, doi:10.1.146/ annurev.astro.34.1.35.
5. Jones, G. H., A. Balogh, and R. J. Forsyth (1998), Radial heliospheric magnetic fields detected by Ulysses, Geophys. Res. Lett., 25, 3109-3112.
6. Lockwood, M. (2002), Relationship between the near-Earth interplanetary field and the coronal source flux: Dependence on timescale, J. Geophys. Res., 107(A12), 1425, doi: 10.1029/2001JA009062.
7. Lockwood, M. (2004), Solar outputs, their variations and their effects on. Earth, in The Sun, Solar Analogs and the Climate, Saas-Fee Adv. Course, vol., 34, edited by I. Redi, M, Güdel, and W. Schmutz, pp. 107-304, Springer, New York.
8. Lockwood, M., and M. Owens (2009), The accuracy of using the Ulysses result of the spatial invariance of the radial heliospheric field to compute the open solar flux, Astrophys. J., 701, 964-973, doi: 10.1088/0004637.X/701/2/964.
9. Lockwood, M., R. Stamper, and M. N. Wild (1999a), A doubling of the Sun's coronal magnetic field during the last 100 years, Nature, 399, 437-439, doi:10.1038/20867. (Pubitemid 29258842)
10. Lockwood, M., R. Stamper, M. N. Wild, A. Balogh, and G. Jones (1999b), Our changing Sun, Astron. Geophys., 40, .10-16.
11. Lockwood, M., R. B. Forsyth, A. Balogh, and D. J. McComas (2004), The accuracy of open solar flux estimates from near-Earth measurements of the interplanetary magnetic field: Analysis of the first two perihelion passes of the Ulysses spacecraft, Ann. Geophys., 22, 1395-1405. (Pubitemid 38615948)
12. Lockwood, M., A. P. Rouillard, I. Finch, and R. Stamper (2006), Comment on "The IDV index: Its derivation and use in inferring long-term variations of the interplanetary magnetic field strength" by Leif Svalgaard and Edward. W. Cliver, J. Geophys. Res., 111, A09109, doi:10.1029/ 2006JA011640.
13. Lockwood, M., M. Owens, and A. P. Rouillard (2009), Excess open solar magnetic flux from satellite data: 2. A survey of kinematic effects, J. Geophys. Res., 114, A11104, doi:10.1029/2009JA014450.
14. McComas, D. J., J. T. Gosling, and J. L. Phillips (1992), Interplanetary magnetic flux: Measurement and balance, J. Geophys. Res., 97,171 -177, doi:10.1029/91JA02370.
15. McComas, D. J., H. A. Elliott, N. A. Schwadron, J. T. Gosling, R. M. Skoug, and B. E. Goldstein (2003), The three-dimensional solar wind around solar maximum, Geophys. Res. Lett., 30(10), .1517, doi:10.1029/ 2003GL017136.
16. McComas, D. J., R., W. Ebert, H. A. Elliott, 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.
17. Owens, M. J., C. N. Arge, N. U. Crooker, N. A. Schwadron, and T. S. Horbury (2008), Estimating total heliospheric magnetic flux from, singlepoint in situ measurements, J. Geophys. Res., 113, A 12103, doi:10.1029/ 2008JA013677.
18. Riley, P., and J. T. Gosling (2007), On the origin of near-radial magnetic fields in the heliosphere: Numerical simulations, J. Geophys. Res., 112, A06115, doi:10.1029/2006JA012210.
19. Rouillard, A. P., M. Lockwood, and I. Finch (2007), Centennial changes in the solar wind speed and in the open solar flux, J. Geophys. Res., 112, A05103, doi:10.1029/2006JA012130.
20. Smith, E. J., and A. Balogh (1995), Ulysses observations of the radial magnetic field, Geophys. Res. Lett., 22, 3317-3320, doi:10.1029/ 95GL02826.
21. Smith, E. J., and A. Balogh (2003), Open magnetic flux: Variation with latitude and solar cycle, in Solar Wind Ten, edited by M. Velli, R. Bruno, and F. Malara, pp. 67-70, Springer, New York.
22. Smith, E. J., A. Balogh, R. J. Forsyth, and D. J. McComas (2001), Ulysses in the south polar cap at solar maximum, Geophys. Res. Lett., 28,4159-4162, doi: 10.1029/2001GL013471.
23. Smith, E. J., et al. (2003), The Sun and heliosphere at solar maximum. Science, 302, 1165-1169, doi:10.1126/science.1086295.
24. Suess, S. T., and E. J. Smith (1996), Latitudinal dependence of the radial IMF component coronal imprint, Geophys. Res. Lett., 23, 3267-3270, doi:10.1029/96GL02908. (Pubitemid 126671572)
25. Suess, S. T, E. J. Smith, J. Phillips, B. E. Goldstein, and S. Nerney (1996), Latitudinal dependence of the radial IMF component interplanetary imprint, Astron. Astrophys., 316, 304-312. (Pubitemid 126522379)
26. Suess, S. T., J. L. Phillips, D. J. McComas, B. E. Goldstein, M., Neugebauer, and S. Nerney (1998), The solar wind inner heliosphere, Space Sci. Rev., 83, 75-86, doi:10.1023/A:1005069328058.
27. Wang, Y.-M., and N. R. Sheeley Jr. (1995), Solar implications of Ulysses interplanetary field measurements, Astrophys. J., 447, L143-L146.
28. Wang, Y.-M., and. N. R. Sheeley Jr. (2002), Sunspot activity and the longterm variation of the Sun's open magnetic flux, J. Geophys. Res., 107(A10), 1302, doi:10.1029/2001JA000500.