1 Parker E. Dynamics of the interplanetary gas and magnetic fields. Astrophys J, 1958, 128: 664
[2]
2 Neugebauer M, Snyder C W. Solar plasma experiment. Science, 1962, 138: 1095-1097
[3]
3 Nolte J T, Krieger A S, Timothy A F, et al. Coronal holes as sources of solar wind. Sol Phys, 1976, 46: 303-322
[4]
4 Pilipp W G, Muehlhaeuser K H, Miggenrieder H, et al. Characteristics of electron velocity distribution functions in the solar wind derived from the HELIOS plasma experiment. J Geophys Res, 1987, 92: 1075
[5]
5 Bavassano B, Dobrowolny M, Mariani F, et al. Radial evolution of power spectra of interplanetary Alfvenic turbulence. J Geophys Res, 1982, 87: 3617-3622
[6]
6 Marsch E, Mühlh?user K H, Schwenn R, et al. Solar wind protons: Three-dimensional velocity distributions and derived plasma parameters measured between 0.3 and 1 AU. J Geophys Res, 1982, 87: 52-72
[7]
7 Tu C Y, Pu Z Y, Wei F S. The power spectrum of interplanetary Alfvenic fluctuations derivation of the governing equation and its solution. J Geophys Res, 1984, 89: 9695
[8]
8 Tu C Y. The damping of interplanetary Alfvenic fluctuations and the heating of the solar wind. J Geophys Res, 1988, 93: 7
[9]
9 Hollweg J V. Transition region, corona, and solar wind in coronal holes. J Geophys Res, 1986, 91: 4111
[10]
10 Axford W I, McKenzie J F. The origin of high speed solar wind streams. Solar Wind Seven Colloquium, 1992. 1-5
[11]
11 Tu C Y, Marsch E. Two-fluid model for heating of the solar corona and acceleration of the solar wind by high-frequency Alfven waves. Sol Phys, 1997, 171: 363
[12]
12 Hassler D M, Dammasch I E, Lemaire P, et al. Solar wind outflow and the chromospheric magnetic network. Science, 1999, 283: 810
[13]
13 Tu C Y, Zhou C, Marsch E, et al. Solar wind origin in coronal funnels. Science, 2005, 308: 519
[14]
14 Xia L D, Popescu M D, Doyle J G, et al. Time series study of EUV spicules observed by SUMER/SoHO. Astron Astrophys, 2005, 438: 1115
[15]
15 Hollweg J V. On the origin of solar spicules. Astrophys J, 1982, 257: 345
[16]
16 Shibata K, Nakamura T, Matsumoto T, et al. Chromospheric anemone jets as evidence of ubiquitous reconnection. Science, 2007, 318: 1591
[17]
17 Kohl J L, Noci G, Antonucci E, et al. First results from the SOHO ultraviolet coronagraph spectrometer. Sol Phys, 1997, 175: 613-644
[18]
18 Li X, Habbal S R, Kohl J, et al. The effect of temperature anisotropy on observations of Doppler dimming and pumping in the inner corona. Astrophys J Lett, 1998, 501: L133-L137
[19]
19 Hu Y Q, Habbal, S R. Resonant acceleration and heating of solar wind ions by dispersive ion cyclotron waves. J Geophys Res, 1999, 104: 17045-17056
[20]
20 Cranmer S R. Coronal holes. Living Rev Sol Phys, 2009, 6: 3
[21]
21 Sheeley N R, Jr, Wang Y M, Hawley S H, et al. Measurements of flow speeds in the corona between 2 and 30 R sub sun. Astrophys J, 1997, 484: 472
[22]
22 Chen Y, Li X, Song H Q, et al. Intrinsic instability of coronal streamers. Astrophys J, 2009, 691: 1936-1942
[23]
23 McComas D J, Bame S J, Barraclough B L, et al. Ulysses’ return to the slow solar wind. Geophys Res Lett, 1998, 25: 1
[24]
24 Chen Y, Hu Y Q. A two-dimensional Alfvén-wave-driven solar wind model. Sol Phys, 2001, 199: 371-384
[25]
38 Gary S P, Nishimura K. Kinetic Alfvén waves: Linear theory and a particle-in-cell simulation. J Geophys Res, 2007, 109: 02109
[26]
39 Bale S D, Kellogg P J, Mozer F S, et al. Measurement of the electric fluctuation spectrum of magnetohydrodynamic turbulence. Phys Rev Lett, 2005, 94: 5002
[27]
40 Matthaeus W H, Goldstein M L, Smith C. Evaluation of magnetic helicity in homogeneous turbulence. Phys Rew Lett, 1982, 48: 1256
[28]
41 Goldstein M L, Roberts D A, Fitch C A. Properties of the fluctuating magnetic helicity in the inertial and dissipation ranges of solar wind turbulence. J Geophys Res, 1994, 99: 11519
[29]
42 He J S, Marsch E, Tu C Y, et al. Possible evidence of Alfvén-cyclotron waves in the angle distribution of magnetic helicity of solar wind turbulence. Astrophys J, 2011, 731: 85
[30]
43 He J S, Tu C Y, Marsch E, et al. Do oblique Alfvén/ion-cyclotron or fast-mode/whistler waves dominate the dissipation of solar wind turbulence near the proton inertial length? Astrophys J, 2012, 745: L8
[31]
25 Li B, Li X, Hu Y Q, et al. A two-dimensional Alfvén wave-driven solar wind model with proton temperature anisotropy. J Geophys Res, 2004, 109: 07103
[32]
26 de Pontieu B, McIntosh S W, Carlsson M, et al. Chromospheric Alfvénic waves strong enough to power the solar wind. Science, 2007, 318: 1574
[33]
27 He J S, Tu C Y, Marsch E, et al. Upward propagating high-frequency Alfvén waves as identified from dynamic wave-like spicules observed by SOT on Hinode. Astron Astrophys, 2009, 497: 525-535
[34]
28 He J S, Marsch E, Tu C Y, et al. Excitation of kink waves due to small-scale magnetic reconnection in the chromosphere? Astrophys J Lett, 2009, 705: L217-L222
[35]
29 Tian H, Tu C Y, Marsch E, et al. The nascent fast solar wind observed by the EUV imaging spectrometer on board Hinode. Astrophys J, 2010, 709: 88
[36]
30 DeForest C E, Howard T A, Tappin S J. Observations of detailed structure in the solar wind at 1 AU with STEREO/HI-2. Astrophys J, 2011, 738: 103
[37]
31 Richardson J D, Paularena K I, Lazarus A J, et al. Radial evolution of the solar wind from IMP 8 to Voyager 2. Geophys Res Lett, 1995, 22: 325
[38]
32 Wang C, Richardson J D, Gosling J T. Slowdown of the solar wind in the outer heliosphere and the interstellar neutral hydrogen density. Geophys Res Lett, 2000, 27: 2429
[39]
33 Marsch E, Tu C Y. Evidence for pitch angle diffusion of solar wind protons in resonance with cyclotron waves. J Geophys Res, 2001, 106: 8357
[40]
34 Gary S P, Saito S. Particle-in-cell simulations of Alfvén-cyclotron wave scattering: Proton velocity distributions. J Geophys Res, 2003, 108: 1194
[41]
35 Wang C B, Wu C S, Yoon P. Heating of ions by Alfvén waves via nonresonant interactions. Phy Res Lett, 2006, 96: 125001
[42]
36 Li X, Lu Q M, Li B. Ion pickup by finite amplitude parallel propagating Alfvén waves. Astrophys J, 2007, 661: L105-L108
[43]
37 Araneda J A, Marsch E, Vi?as A F. Collisionless damping of parametrically unstable Alfvén waves. J Geophys Res, 2007, 112: 04104