Space Physics and Aeronomy, Solar Physics and Solar Wind

75 Fenrich, F.R. and Waters, C.L. (2008, October). Phase coherence analysis of a field line resonance and solar wind oscillation. Geophysical Research Letters 35: L20102. https://doi.org/10.1029/2008GL035430.

76 Fisk, L.A. (1996, July). Motion of the footpoints of heliospheric magnetic field lines at the Sun: Implications for recurrent energetic particle events at high heliographic latitudes. Journal of Geophysical Research: Space Physics 101: 15547–15554. https://doi.org/10.1029/96JA01005.

77 Fisk, L.A., Schwadron, N.A., and Zurbuchen, T.H. (1998, July). On the slow solar wind. Space Science Reviews 86: 51–60. https://doi.org/10.1023/A:1005015527146.

78 Forsyth, R.J., Balogh, A., and Smith, E.J. (2002, November). The underlying direction of the heliospheric magnetic field through the Ulysses first orbit. Journal of Geophysical Research: Space Physics 107: 1405. https://doi.org/10.1029/2001JA005056.

79 Gary, S.P. and Smith, C.W. (2009, December). Short‐wavelength turbulence in the solar wind: Linear theory of whistler and kinetic Alfvén fluctuations. Journal of Geophysical Research: Space Physics 114: A12105. https://doi.org/10.1029/2009JA014525.

80 Geiss, J. (1998). Constraints on the FIP mechanisms from solar wind abundance data. Space Science Reviews 85: 241–252.

81 Geiss, J., Gloeckler, G., and von Steiger, R. (1995, April). Origin of the solar wind from composition data. Space Science Reviews 72: 49–60. https://doi.org/10.1007/BF00768753.

82 Giacalone, J., Jokipii, J.R., and Mazur, J.E. (2000, March). Small‐scale gradients and large‐scale diffusion of charged particles in the heliospheric magnetic field. The Astrophysical Journal Letters 532: L75–L78. https://doi.org/10.1086/312564.

83 Goldstein, H. (1983, November). On the field configuration in magnetic clouds. In Nasa conference publication (Vol. 228).

84 Goldstein, M. L., Roberts, D. A., & Matthaeus, W. H. (1995). Magnetohydrodynamic turbulence in the solar wind. Annual Review of Astronomy and Astrophysics, 33, 283–326. doi: 10.1146/annurev.aa .33.090195.001435.

85 Gosling, J.T. (2005). Magnetic disconnection from the Sun: Observations of a reconnection exhaust in the solar wind at the heliospheric current sheet. Geophysical Research Letters 32 (5) https://doi.org/10.1029/2005GL022406.

86 Gosling, J.T. (2012, November). Magnetic reconnection in the solar wind. Space Science Reviews 172: 187–200. https://doi.org/10.1007/s11214‐011‐9747‐2.

87 Gosling, J.T., Borrini, G., Asbridge, J.R. et al. (1981, July). Coronal streamers in the solar wind at 1 AU. Journal of Geophysical Research 86: 5438–5448. https://doi.org/10.1029/JA086iA07p05438.

88 Gosling, J.T., Eriksson, S., and Schwenn, R. (2006, October). Petschek‐type magnetic reconnection exhausts in the solar wind well inside 1 AU: Helios. Journal of Geophysical Research 111 (A10) https://doi.org/10.1029/2006JA011863.

89 Gosling, J.T., Hundhausen, A.J., and Bame, S.J. (1976, May). Solar wind stream evolution at large heliocentric distances – Experimental demonstration and the test of a model. Journal of Geophysical Research 81: 2111–2122. https://doi.org/10.1029/JA081i013p02111.

90 Gosling, J.T. and Phan, T.D. (2013, January). Magnetic reconnection in the solar wind at current sheets associated with extremely small field shear angles. The Astrophysical Journal 763 (2): L39. https://doi.org/10.1088/2041‐8205/763/2/L39.

91 Gosling, J.T. and Pizzo, V.J. (1999, July). Formation and evolution of corotating interaction regions and their three dimensional structure. Space Science Review 89: 21–52. https://doi.org/10.1023/A:1005291711900.

92 Gosling, J.T. and Szabo, A. (2008). Bifurcated current sheets produced by magnetic reconnection in the solar wind. Journal of Geophysical Research: Space Physics 113 (A10).

93 Gosling, J.T., Skoug, R.M., McComas, D.J., and Smith, C.W. (2005, January). Direct evidence for magnetic reconnection in the solar wind near 1 AU. Journal of Geophysical Research: Space Physics 110: A01107. https://doi.org/10.1029/2004JA010809.

94 Greco, A., Perri, S., Servidio, S. et al. (2016, June). The complex structure of magnetic field discontinuities in the turbulent solar wind. The Astrophysical Journal Letters 823: L39. https://doi.org/10.3847/2041‐8205/823/2/L39.

95 Hamilton, K., Smith, C.W., Vasquez, B.J., and Leamon, R.J. (2008, January). Anisotropies and helicities in the solar wind inertial and dissipation ranges at 1 AU. Journal of Geophysical Research: Space Physics 113: A01106. https://doi.org/10.1029/2007JA012559.

96 Harrison, R.A., Davis, C.J., and Davies, J.A. (2009, October). Pre‐CME onset fuses – Do the STEREO heliospheric imagers hold the clues to the CME onset process? Solar Physics 259: 277–296. https://doi.org/10.1007/s11207‐009‐9417‐7.

97 Hartinger, M.D., Welling, D., Viall, N.M. et al. (2014, October). The effect of magnetopause motion on fast mode resonance. Journal of Geophysical Research: Space Physics 119: 8212–8227. https://doi.org/10.1002/2014JA020401.

98 Hellinger, P., Matteini, L., Štverák, S., Trávníček, P. M., & Marsch, E. (2011, September). Heating and cooling of protons in the fast solar wind between 0.3 and 1 AU: Helios revisited. Journal of Geophysical Research: Space Physics, 116, 9105. doi: 10.1029/2011JA016674.

99 Higginson, A.K., Antiochos, S.K., DeVore, C.R. et al. (2017, May). Formation of heliospheric arcs of slow solar wind. The Astrophysical Journal 840: L10. https://doi.org/10.3847/2041‐8213/aa6d72.

100 Higginson, A.K. and Lynch, B.J. (2018, May). Structured slow solar wind variability: Streamer‐blob flux ropes and torsional Alfvén waves. The Astrophysical Journal 859: 6. https://doi.org/10.3847/1538‐4357/aabc08.

101 Hollweg, J.V. (2002). Heating and acceleration of the solar wind in coronal holes: cyclotron resonances. Advances in Space Research 30: 469–469. https://doi.org/10.1016/ S0273‐1177(02)00324‐1.

102 Horbury, T. S., Forman, M., & Oughton, S. (2008, October). Anisotropic scaling of magnetohydrodynamic turbulence. Physical Review Letters, 101 (17), 175005‐+. doi: https://doi.org/10.1103/ PhysRevLett.101.175005.

103 Horbury, T. S., Matteini, L., & Stansby, D. (2018, August). Short, large‐amplitude speed enhancements in the near‐Sunfast solar wind. Monthly Notices of the Royal Astronomical Society, 478, 1980–1986. doi: 10 .1093/mnras/sty953.

104 Howes, G.G., Cowley, S.C., Dorland, W. et al. (2006, November). Astrophysical gyrokinetics: Basic equations and linear theory. The Astrophysical Journal 651: 590–614. https://doi.org/10.1086/506172.

105 Howes, G.G., Tenbarge, J.M., Dorland, W. et al. (2011, July). Gyrokinetic simulations of solar wind turbulence from ion to electron scales. Physical Review Letters 107 (3): 035004. https://doi.org/10.1103/PhysRevLett.107.035004.

106 Hudson, P.D. (1970, November). Discontinuities in an anisotropic plasma and their identification in the solar wind. Planetary and Space Science 18: 1611–1622. https://doi.org/10.1016/0032‐0633(70) 90036‐X.

107 Hundhausen, A.J. and Gosling, J.T. (1976, March). Solar wind structure at large heliocentric distances – an interpretation of Pioneer 10 observations. Journal of Geophysical Research 81: 1436–1440. https://doi.org/10.1029/JA081i007p01436.

108 Hyder, C.L. and Lites, B.W. (1970, September). Hα Doppler brightening and Lyman‐a Doppler dimming in moving Hα Prominences. Solar Physics 14: 147–156. https://doi.org/10.1007/BF00240170.

109 Isenberg, P.A. (1987, February). Evolution of interstellar pickup ions in the solar wind. Journal of Geophysical Research 92: 1067–1073. https://doi.org/10.1029/JA092iA02p01067.

110 Isenberg, P.A., Lee, M.A., and Hollweg, J.V. (2001, April). The kinetic shell model of coronal heating and acceleration by ion cyclotron waves: 1. Outward propagating waves. Journal of Geophysical Research: Space Physics 106: 5649–5660. https://doi.org/10.1029/2000JA000099.