Space Physics and Aeronomy, Solar Physics and Solar Wind. Группа авторов

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Space Physics and Aeronomy, Solar Physics and Solar Wind - Группа авторов

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J.T., Smith, C.W., Vasquez, B.J. et al. (2014, May). Variable cascade dynamics and intermittency in the solar wind at 1 AU. The Astrophysical Journal 786: 52. https://doi.org/10.1088/0004‐637X/786/1/52.

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      52 Cranmer, S.R., van Ballegooijen, A.A., and Woolsey, L.N. (2013, April). Connecting the Sun’s high‐resolution magnetic carpet to the turbulent heliosphere. The Astrophysical Journal 767: 125. https://doi.org/10.1088/0004‐637X/767/2/125.

      53 Crooker, N.U., Antiochos, S.K., Zhao, X., and Neugebauer, M. (2012, April). Global network of slow solar wind. Journal of Geophysical Research: Space Physics 117: A04104. https://doi.org/10.1029/2011JA017236.

      54 Crooker, N.U., Burton, M.E., Siscoe, G.L. et al. (1996, November). Solar wind streamer belt structure. Journal of Geophysical Research 101: 24331–24342. https://doi.org/10.1029/96JA02412.

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      56 Crooker, N.U., McPherron, R.L., and Owens, M.J. (2014, June). Comparison of interplanetary signatures of streamers and pseudostreamers. Journal of Geophysical Research: Space Physics 119: 4157–4163. https://doi.org/10.1002/2014JA020079.

      57 Crooker, N.U., Siscoe, G.L., Russell, C.T., and Smith, E.J. (1982, April). Factors controlling degree of correlation between ISEE 1 and ISEE 3 interplanetary magnetic field measurements. Journal of Geophysical Research: Space Physics 87: 2224–2230. https://doi.org/10.1029/JA087iA04p02224.

      58 Crooker, N.U., Siscoe, G.L., Shodhan, S. et al. (1993, June). Multiple heliospheric current sheets and coronal streamer belt dynamics. Journal of Geophysical Research: Space Physics 98: 9371–9381. https://doi.org/10.1029/93JA00636.

      59 D’Amicis, R. and Bruno, R. (2015, May). On the origin of highly Alfvénic slow solar wind. The Astrophysical Journal 805: 84. https://doi.org/10.1088/0004‐637X/805/1/84.

      60 D’Amicis, R., Matteini, L., & Bruno, R. (2018, December). On slow solar wind with high Alfv\’enicity: From composition and microphysics to spectral properties. arXiv e‐prints.

      61 Dasso, S., Nakwacki, M.S., Démoulin, P., and Mandrini, C.H. (2007, August). Progressive transformation of a flux rope to an ICME. Comparative analysis using the direct and fitted expansion methods. Solar Physics 244: 115–137. https://doi.org/10.1007/s11207‐007‐9034‐2.

      62 DeForest, C.E., Howard, R.A., Velli, M. et al. (2018, July). The highly structured outer solar corona. The Astrophysical Journal 862: 18. https://doi.org/10.3847/1538‐4357/aac8e3.

      63 DeForest, C.E., Matthaeus, W.H., Viall, N.M., and Cranmer, S.R. (2016, September). Fading coronal structure and the onset of turbulence in the young solar wind. The Astrophysical Journal 828: 66. https://doi.org/10.3847/0004‐637X/828/2/66.

      64 Denskat, K.U. and Neubauer, F.M. (1982, April). Statistical properties of low‐ frequency magnetic field fluctuations in the solar wind from 0.29 to 1.0 AU during solar minimum conditions – HELIOS 1 and HELIOS 2. Journal of Geophysical Research: Space Physics 87: 2215–2223. https://doi.org/10.1029/JA087iA04p02215.

      65 Di Matteo, S., Viall, N.M., Kepko, L. et al. (2019). Helios observations of quasiperiodic density structures in the slow solar wind at 0.3, 0.4, and 0.6 AU. Journal of Geophysical Research: Space Physics 124 (2): 837–860. https://doi.org/10.1029/2018JA026182.

      66 Di Matteo, S. and Villante, U. (2017, May). The identification of solar wind waves at discrete frequencies and the role of the spectral analysis techniques. Journal of Geophysical Research: Space Physics 122: 4905–4920. https://doi.org/10.1002/2017JA023936.

      67 Dolei, S., Susino, R., Sasso, C. et al. (2018, May). Mapping the solar wind HI outflow velocity in the inner heliosphere by coronagraphic ultraviolet and visible‐light observations. Astronomy & Astrophysics (A&A) 612: A84. https://doi.org/10.1051/0004‐6361/201732118.

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      69 Dyrud, L.P., Behnke, R., Kepko, E.L. et al. (2008, July). Ionospheric ULF oscillations driven from above Arecibo. Geophysical Research Letters 35: L14101. https://doi.org/10.1029/2008GL034073.

      70 Endeve, E., Holzer, T.E., and Leer, E. (2004, March). Helmet streamers gone unstable: Two‐fluid magnetohydrodynamic models of the solar corona. The Astrophysical Journal 603: 307–321. https://doi.org/10.1086/381239.

      71 Eriksson, S., Gosling, J.T., Phan, T.D. et al. (2009). Asymmetric shear flow effects on magnetic field configuration within oppositely directed solar wind reconnection exhausts. Journal of Geophysical Research: Space Physics 114 (A7) https://doi.org/10.1029/2008JA013990.

      72 Fahr, H.J. and Fichtner, H. (2011, September). Pick‐up ion transport under conservation of particle invariants: How important are velocity diffusion and cooling processes? Astronomy and Astrophysics 533: A92. https://doi.org/10.1051/0004‐6361/201116880.

      73 Feng, H.Q., Wu, D.J., and Chao, J.K. (2007, February). Size and energy distributions of interplanetary magnetic flux ropes. Journal of Geophysical Research: Space Physics 112: A02102. https://doi.org/10.1029/2006JA011962.

      74 Feng, H.Q., Wu, D.J., Wang, J.M., and Chao, J.W. (2011, March). Magnetic reconnection exhausts at the boundaries of small interplanetary magnetic flux ropes. Astronomy & Astrophysics 527: A67. https://doi.org/10.1051/0004‐6361/201014473.

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