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Lockwood, Mike; Owens, Matt J. (2013)
Publisher: American Geophysical Union
Languages: English
Types: Article

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    • Balogh, A., R. J. Forsyth, E. A. Lucek, T. S. Horbury, and E. J. Smith (1999), Heliographic magnetic field polarity inversions at high heliographic latitudes, Geophys. Res. Lett., 26, 631-634, doi:10.1029/1999GL900061.
    • Crooker, N. U., S. W. Kahler, D. E. Larson, and R. P. Lin (2004), Largescale magnetic field inversions at sector boundaries, J. Geophys. Res., 109, A03108, doi:10.1029/2003JA010278.
    • Erdős, G., and A. Balogh (2012), Magnetic flux density measured in fast and slow solar wind streams, Ap. J., 753(2), Article 130, doi:10.1088/0004-637X/753/2/130.
    • Foullon, C., et al. (2011), Plasmoid releases in the heliospheric current sheet and associated coronal hole boundary layer evolution, Ap. J., 737(1), Article 16, doi:10.1088/0004-637x/737/1/16.
    • Jones, G. H., A. Balogh, and R. J. Forsyth (1998), Radial heliospheric magnetic fields detected by Ulysses, Geophys. Res. Lett., 25, 3109-3112.
    • Gosling, J. T., R. M. Skoug, and W. C. Feldman (2001), Solar wind electron halo depletions at 90 pitch angle, Geophys. Res. Lett., 28, 4155-4158, doi:10.1029/2001GL013758.
    • Kahler, S., and R. P. Lin (1994), The determination of interplanetary magnetic field polarities around sector boundaries using E > 2 keV electrons, Geophys. Res. Lett., 21, 1575-1578, doi:10.1029/94GL01362.
    • Kahler, S. W., and R. P. Lin (1995), An examination of directional discontinuities and magnetic polarity changes around interplanetary sector boundaries using E > 2 keV electrons, Sol. Phys., 161, 183-195, doi:10.1007/BF00732092.
    • Kahler, S. W., N. U. Crooker, and J. T. Gosling (1996), The topology of intrasector reversals of the interplanetary magnetic field, J. Geophys. Res., 101(All), 24373-24382, doi:10.1029/96JA02232.
    • Kahler, S. W., N. U. Crooker, and J. T. Gosling (1998), Properties of interplanetary magnetic sector boundaries based on electron heat-flux flow directions, J. Geophys. Res., 103(A9), 20603-20612. doi:10.1029/98JA01745.
    • Lockwood, M., R. B. Forsyth, A. Balogh, and D. J. McComas (2004), Open solar flux estimates from near-Earth measurements of the interplanetary magnetic field: Comparison of the first two perihelion passes of the Ulysses spacecraft, Ann. Geophys., 22, 1395-1405.
    • Lockwood, M. (2010), Solar change and climate: an update in the light of the current exceptional solar minimum, Proc. R. Soc. A, 466(2114), 303-329, doi:10.1098/rspa.2009.0519.
    • Lockwood, M., M. Owens, and A. P. Rouillard (2009a), Excess open solar magnetic flux from satellite data: I. Analysis of the 3rd Perihelion Ulysses Pass, J. Geophys. Res., 114, A11103, doi:10.1029/2009JA014449.
    • Lockwood, M., M. Owens, and A. P. Rouillard (2009b), Excess open solar magnetic flux from satellite data: II. A survey of kinematic effects, J. Geophys. Res., 114, A11104, doi:10.1029/2009JA014450.
    • Lockwood, M., A. P. Rouillard, and I. D. Finch (2009c), The rise and fall of open solar flux during the current grand solar maximum, Ap. J., 700(2), 937-944, doi:10.1088/0004-637X/700/2/937.
    • 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(2), 964-973, doi:10.1088/0004-637X/701/2/964.
    • 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.
    • Owens, M. J., and M. Lockwood (2012), Cyclic loss of open solar flux since 1868: The link to heliospheric current sheet tilt and implications for the Maunder Minimum, J. Geophys. Res., 117, A04102, doi:10.1029/ 2011JA017193.
    • Owens, M. J., C. N. Arge, N. U. Crooker, N. A. Schwadron, and T. S. Horbury (2008), Estimating total heliospheric magnetic flux from single-point in situ measurements, J. Geophys. Res., 113, A12103, doi:10.1029/2008JA013677.
    • Owens, M. J., N. U. Crooker, and M. Lockwood (2012), Solar origin of heliospheric magnetic field inversions: Evidence for coronal magnetic loop opening within pseudostreamers, J. Geophys. Res., in press, doi:10.1002/jgra.50259.
    • Riley, P., and J. T. Gosling (2007), On the origin of near-radial magnetic fields in the heliosphere: Numerical simulations, J. Geophys. Res., 112, 917, A06115, doi:10.1029/2006JA012210.
    • Schatten, K. H. (1999), Models for coronal and interplanetary magnetic fields: A critical commentary, in Sun - Earth Plasma Connections, Geophys. Monogr. Ser., vol. 109, edited by J. L. Burch, R. L. Caravillano, and S. K. Antiochos, pp. 129-142, AGU, Washington, D. C.
    • Schatten, K. H., J. M. Wilcox, and N. F. Ness (1969), A model of interplanetary and coronal magnetic fields, PFSS method, Sol. Phys., 6, 442-455, doi:10.1007/BF00146478.
    • Smith, E. J. (2011), What causes the flux excess in the heliospheric magnetic field?, J. Geophys. Res., 116, A12101, doi:10.1029/ 2011JA016521.
    • Smith, E. J., and A. Balogh (1995), Ulysses observations of the radial magnetic field, Geophys. Res. Lett., 22, 3317-3320. doi:10.1029/95GL02826.
    • Wang, Y.-M., and N. R. Sheeley Jr. (1995), Solar implications of Ulysses interplanetary field measurements, Astrophys. J., 447, L143-L146, 961, doi:10.1086/309578.96.
    • Wang, Y.-M., and N. R. Sheeley Jr. (2003), On the topological evolution of the coronal magnetic field during the solar cycle, Astrophys. J., 599, 964, 1404-1417, doi:10.1086/379348.
    • Wilcox, J. M. (1968), The interplanetary magnetic field. Solar origin and terrestrial effects, Space Sci. Rev., 8(2), 258-328.
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