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

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style="font-size:15px;">      182 Nicol, R.M., Chapman, S.C., and Dendy, R.O. (2009, October). Quantifying the anisotropy and solar cycle dependence of “1/f” solar wind fluctuations observed by advanced composition explorer. The Astrophysical Journal 703: 2138–2151. https://doi.org/10.1088/0004‐637X/703/2/2138.

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      187 Owens, M.J., Crooker, N.U., and Lockwood, M. (2013, May). Solar origin of heliospheric magnetic field inversions: Evidence for coronal loop opening within pseudostreamers. Journal of Geophysical Research: Space Physics 118: 1868–1879. https://doi.org/10.1002/jgra.50259.

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      191 Perrone, D., Alexandrova, O., Mangeney, A. et al. (2016, August). Compressive coherent structures at ion scales in the slow solar wind. The Astrophysical Journal 826: 196. https://doi.org/10.3847/0004‐637X/826/2/196.

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      193 Phan, T.D., Gosling, J.T., Davis, M.S. et al. (2006, January). A magnetic reconnection X‐line extending more than 390 Earth radii in the solar wind. Nature 439 (7073): 175–178. https://doi.org/10.1038/nature04393.

      194 Pierrard, V. (2011, February). Solar wind electron transport: Interplanetary electric field and heat conduction. 172: 315–324. https://doi.org/10.1007/s11214‐011‐9743‐6.

      195 Pierrard, V., & Lamy, H. (2003, September). The effects of the velocity filtration mechanism on the minor ions of the corona. Solar Physics, 216, 47–58. doi: 10.1023/ A:1026157306754.

      196 Pierrard, V. and Lazar, M. (2010, November). Kappa distributions: Theory and applications in space plasmas. Solar Physics 267: 153–174. https://doi.org/10.1007/s11207‐010‐9640‐2.

      197 Pierrard, V., Lazar, M., Poedts, S. et al. (2016, August). The electron temperature and anisotropy in the solar wind. comparison of the core and halo populations. Solar Physics 291: 2165–2179. https://doi.org/10.1007/s11207‐016‐0961‐7.

      198 Pierrard, V., Lazar, M., and Schlickeiser, R. (2011, April). Evolution of the electron distribution function in the whistler wave turbulence of the solar wind. Solar Physics 269: 421–438. https://doi.org/10.1007/s11207‐010‐9700‐7.

      199 Pierrard, V., Maksimovic, M., and Lemaire, J. (1999, August). Electron velocity distribution functions from the solar wind to the corona. Journal of Geophysical Research: Space Physics 104: 17021–17032. https://doi.org/10.1029/1999JA900169.

      200 Pierrard, V. and Pieters, M. (2014, December). Coronal heating and solar wind acceleration for electrons, protons, and minor ions obtained from kinetic models based on kappa distributions. Journal of Geophysical Research: Space Physics 119: 9441–9455. https://doi.org/10.1002/2014JA020678.

      201 Pilipp, W.G., Miggenrieder, H., Montgomery, M.D. et al. (1987, February). Characteristics of electron velocity distribution functions in the solar wind derived from the HELIOS plasma experiment. Journal of Geophysical Research: Space Physics 92: 1075–1092. https://doi.org/10.1029/JA092iA02p01075.

      202 Pilipp, W.G., Muehlhaeuser, K.‐H., Miggenrieder, H. et al. (1990, May). Large‐scale variations of thermal electron parameters in the solar wind between 0.3 and 1 AU. Journal of Geophysical Research: Space Physics 95: 6305–6329. https://doi.org/10.1029/JA095iA05p06305.

      203 Pinto, R.F., Brun, A.S., Jouve, L., and Grappin, R. (2011, August). Coupling the solar dynamo and the corona: Wind properties, mass, and momentum losses during an activity cycle. The Astrophysical Journal 737: 72. https://doi.org/10.1088/0004‐637X/737/2/72.

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      205 Pinto, R.F. and Rouillard, A.P. (2017, April). A multiple flux‐tube solar wind model. The Astrophysical Journal 838: 89. https://doi.org/10.3847/1538‐4357/aa6398.

      206 Pizzo, V.J. (1982, June). A three‐dimensional model of corotating streams in the solar wind. III ‐ Magnetohydrodynamic streams. Journal of Geophysical Research: Space Physics 87: 4374–4394. https://doi.org/10.1029/ JA087iA06p04374.

      207 Podesta, J. J., Roberts, D. A., & Goldstein, M. L. (2006, October). Power spectrum of small‐scale turbulent velocity fluctuations

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