Modeling Kelvin–Helmholtz Instability in Soft X-Ray Solar Jets

Advances in Astronomy

Review Article

Abhishek K. Srivastava³  Ramesh Chandra²  Ivan Zhelyazkov¹ 

[1] Faculty of Physics, Sofia University, 1164 Sofia, Bulgaria, uni-sofia.bg;Department of Physics, Kumaun University, Nainital 263001, India, kunainital.ac.in;Department of Physics, Indian Institute of Technology, Banaras Hindu University, Varanasi 221005, India, iitb.ac.in

Others  :  1414890
DOI  :  10.1155/2017/2626495

 received in 2016-08-08, accepted in 2016-12-01,  发布年份 2017

【 授权许可】

CC BY   
Copyright © 2017 Ivan Zhelyazkov et al. 2017

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【 参考文献 】

• [1]J. M. Beckers. (1972). Solar spicules. Annual Review of Astronomy and Astrophysics.10(1):73-100. DOI: 10.1146/annurev.aa.10.090172.000445.
• [2]J. R. Roy. (1973). The magnetic properties of solar surges. Solar Physics.28(1):95-114. DOI: 10.1146/annurev.aa.10.090172.000445.
• [3]K. Shibata, T. Nakamura, T. Matsumoto, K. Otsuji. et al.(2007). Chromospheric anemone jets as evidence of ubiquitous reconnection. Science.318(5856):1591-1594. DOI: 10.1146/annurev.aa.10.090172.000445.
• [4]C. Chifor, H. Isobe, E. Mason, G. Hannah. et al.(2008). Magnetic flux cancellation associated with a recurring solar jet observed with Hinode, RHESSI, and STEREO/EUVI. Astronomy & Astrophysics.491(1):279-288. DOI: 10.1146/annurev.aa.10.090172.000445.
• [5]N. Nishizuka, M. Shimizu, T. Nakamura, K. Otsuji. et al.(2008). Giant chromospheric anemone jet observed with and comparison with magnetohydrodynamic simulations: Evidence of propagating Alfvén waves and magnetic reconnection. The Astrophysical Journal Letters.683(1):L83-L86. DOI: 10.1146/annurev.aa.10.090172.000445.
• [6]D. Alexander, L. Fletcher. (1999). High-resolution observations of plasma jets in the solar corona. Solar Physics.190(1-2):167-184. DOI: 10.1146/annurev.aa.10.090172.000445.
• [7]K. Shibata, Y. Ishido, L. Acton. (1992). Observations of X-ray jets with the Yohkoh soft X-ray telescope. Publications of the Astronomical Society of Japan.44(5):L173-L179. DOI: 10.1146/annurev.aa.10.090172.000445.
• [8]S. Tsuneta, L. Acton, M. Bruner, J. Lemen. et al.(1991). The soft X-ray telescope for the SOLAR-A mission. Solar Physics.136(1):37-67. DOI: 10.1146/annurev.aa.10.090172.000445.
• [9]M. Shimojo, S. Hashimoto, K. Shibata, T. Hirayama. et al.(1996). Statistical study of solar X-ray jets observed with the Yohkoh soft X-ray telescope. Publications of the Astronomical Society of Japan.48(1):123-136. DOI: 10.1146/annurev.aa.10.090172.000445.
• [10]M. Shimojo, K. Shibata. (2000). Physical parameters of solar X-ray jets. The Astrophysical Journal.542(2):1100-1108. DOI: 10.1146/annurev.aa.10.090172.000445.
• [11]L. Culhane, L. K. Harra, D. Baker, L. Van Driel-Gesztelyi. et al.(2007). Hinode EUV study of jets in the Sun's south polar corona. Publications of the Astronomical Society of Japan.59:S751-S756. DOI: 10.1146/annurev.aa.10.090172.000445.
• [12]C. Chifor, P. R. Young, H. Isobe, H. E. Mason. et al.(2008). An active region jet observed with Hinode. Astronomy & Astrophysics.481(1):L57-L60. DOI: 10.1146/annurev.aa.10.090172.000445.
• [13]A. Savcheva, J. Cirtain, E. E. DeLuca, L. L. Lundquist. et al.(2007). A study of polar jet parameters based on Hinode XRT observations. Publications of the Astronomical Society of Japan.59:S771-S778. DOI: 10.1146/annurev.aa.10.090172.000445.
• [14]J. W. Cirtain, L. Golub, L. Lundquist, A. Van Ballegooijen. et al.(2007). Evidence for Alfvén waves in solar X-ray jets. Science.318(5856):1580-1582. DOI: 10.1146/annurev.aa.10.090172.000445.
• [15]Y.-H. Kim, Y.-J. Moon, Y.-D. Park, T. Sakurai. et al.(2007). Small-scale X-ray/EUV jets seen in Hinode XRT and TRACE. Publications of the Astronomical Society of Japan.59:S763-S769. DOI: 10.1146/annurev.aa.10.090172.000445.
• [16]L.-H. Yang, Y.-C. Jiang, J.-Y. Yang, Y. Bi. et al.(2011). Observations of EUV and soft X-ray recurring jets in an active region. Research in Astronomy and Astrophysics.11(10):1229-1242. DOI: 10.1146/annurev.aa.10.090172.000445.
• [17]M. S. Madjarska. (2011). Dynamics and plasma properties of an X-ray jet from SUMER, EIS, XRT, and EUVI A & B simultaneous observations. Astronomy & Astrophysics.526(2, article A19). DOI: 10.1146/annurev.aa.10.090172.000445.
• [18]K. Chandrashekhar, A. Bemporad, D. Banerjee, G. R. Gupta. et al.(2014). Characteristics of polar coronal hole jets. Astronomy & Astrophysics.561, article A104. DOI: 10.1146/annurev.aa.10.090172.000445.
• [19]W. D. Pesnell, B. J. Thompson, P. C. Chamberlin. (2012). The (SDO). Solar Physics.275(1):3-15. DOI: 10.1146/annurev.aa.10.090172.000445.
• [20]J. R. Lemen, A. M. Title, D. J. Akin. (2012). The (AIA) on the (SDO). Solar Physics.275(1):17-40. DOI: 10.1146/annurev.aa.10.090172.000445.
• [21]P. Boerner, C. Edwards, J. Lemen, A. Rausch. et al.(2012). Initial calibration of the (AIA) on the (SDO). Solar Physics.275(1):41-66. DOI: 10.1146/annurev.aa.10.090172.000445.
• [22]S. P. Moschou, K. Tsinganos, A. Vourlidas, V. Archontis. et al.(2013). SDO observations of solar jets. Solar Physics.284(2):427-438. DOI: 10.1146/annurev.aa.10.090172.000445.
• [23]K. Chandrashekhar, R. J. Morton, D. Banerjee, G. R. Gupta. et al.(2014). The dynamical behaviour of a jet in an on-disk coronal hole observed with AIA/SDO. Astronomy & Astrophysics.562, article A98. DOI: 10.1146/annurev.aa.10.090172.000445.
• [24]A. C. Sterling, R. L. Moore, D. A. Falconer, M. Adams. et al.(2015). Small-scale filament eruptions as the driver of X-ray jets in solar coronal holes. Nature.523(7561):437-440. DOI: 10.1146/annurev.aa.10.090172.000445.
• [25]B. Filippov, A. K. Srivastava, B. N. Dwivedi, S. Masson. et al.(2015). Formation of a rotating jet during the filament eruption on 2013 April 10-11. Monthly Notices of the Royal Astronomical Society.451(1):1117-1129. DOI: 10.1146/annurev.aa.10.090172.000445.
• [26]M. Shimojo, K. Shibata, T. Yokoyama, K. Hori. et al.(2001). One-dimensional and pseudo-two-dimensional hydrodynamic simulations of solar X-ray jets. Astrophysical Journal.550(2):1051-1063. DOI: 10.1146/annurev.aa.10.090172.000445.
• [27]S. Kamio, H. Hara, T. Watanabe, K. Matsuzaki. et al.(2007). Velocity structure of jets in a coronal hole. Publications of the Astronomical Society of Japan.59:S757-S762. DOI: 10.1146/annurev.aa.10.090172.000445.
• [28]R. L. Moore, J. W. Cirtain, A. C. Sterling, D. A. Falconer. et al.(2010). Dichotomy of solar coronal jets: Standard jets and blowout jets. The Astrophysical Journal.720(1):757-770. DOI: 10.1146/annurev.aa.10.090172.000445.
• [29]E. Pariat, S. K. Antiochos, C. R. DeVore. (2009). A model for solar polar jets. The Astrophysical Journal.691(1):61-74. DOI: 10.1146/annurev.aa.10.090172.000445.
• [30]B. Filippov, L. Golub, S. Koutchmy. (2009). X-ray jet dynamics in a polar coronal hole region. Solar Physics.254(2):259-269. DOI: 10.1146/annurev.aa.10.090172.000445.
• [31]E. Pariat, S. K. Antiochos, C. R. Devore. (2010). Three-dimensional modeling of quasi-homologous solar jets. Astrophysical Journal.714(2):1762-1778. DOI: 10.1146/annurev.aa.10.090172.000445.
• [32]F. Jiang, J. Zhang, S. Yang. (2015). Interaction between an emerging flux region and a pre-existing fan-spine dome observed by IRIS and SDO. Publications of the Astronomical Society of Japan.67(4, article 78). DOI: 10.1146/annurev.aa.10.090172.000445.
• [33]A. C. Sterling, L. K. Harra, R. L. Moore. (2010). Fibrillar chromospheric spicule-like counterparts to an extreme-ultraviolet and soft X-ray blowout coronal jet. The Astrophysical Journal.722(2):1644-1653. DOI: 10.1146/annurev.aa.10.090172.000445.
• [34]S. Pucci, G. Poletto, A. C. Sterling, M. Romoli. et al.(2013). Physical parameters of standard and blowout jets. Astrophysical Journal.776, article 16. DOI: 10.1146/annurev.aa.10.090172.000445.
• [35]R. L. Moore, A. C. Sterling, D. A. Falconer, D. Robe. et al.(2013). The cool component and the dichotomy, lateral expansion, and axial rotation of solar X-ray jets. The Astrophysical Journal.769(2, article 134). DOI: 10.1146/annurev.aa.10.090172.000445.
• [36]R. L. Moore, A. C. Sterling, D. A. Falconer. (2015). Magnetic untwisting in solar jets that go into the outer corona in polar coronal holes. Astrophysical Journal.806(1, article 11). DOI: 10.1146/annurev.aa.10.090172.000445.
• [37]G. E. Brueckner, R. A. Howard, M. J. Koomen, C. M. Korendyke. et al.(1995). The Large Angle Spectroscopic Coronagraph (LASCO). Solar Physics.162(1):357-402. DOI: 10.1146/annurev.aa.10.090172.000445.
• [38]B. Schmieder, Y. Guo, F. Moreno-Insertis, G. Aulanier. et al.(2013). Twisting solar coronal jet launched at the boundary of an active region. Astronomy and Astrophysics.559, article A1. DOI: 10.1146/annurev.aa.10.090172.000445.
• [39]E. Pariat, K. Dalmasse, C. R. DeVore, S. K. Antiochos. et al.(2015). Model for straight and helical solar jets: I. Parametric studies of the magnetic field geometry. Astronomy and Astrophysics.573, article 130. DOI: 10.1146/annurev.aa.10.090172.000445.
• [40]S. Patsourakos, E. Pariat, A. Vourlidas, S. K. Antiochos. et al.(2008). SECCHI stereoscopic observations constraining the initiation of polar coronal jets. The Astrophysical Journal.680(1):L73-L76. DOI: 10.1146/annurev.aa.10.090172.000445.
• [41]C. Gontikakis, V. Archontis, K. Tsinganos. (2009). Observations and 3D MHD simulations of a solar active region jet. Astronomy & Astrophysics.506(3):L45-L48. DOI: 10.1146/annurev.aa.10.090172.000445.
• [42]R. Chandra, G. R. Gupta, S. Mulay, D. Tripathi. et al.(2015). Sunspot waves and triggering of homologous active region jets. Monthly Notices of the Royal Astronomical Society.446(4):3741-3748. DOI: 10.1146/annurev.aa.10.090172.000445.
• [43]J. Chae, H. Wang, C.-Y. Lee, P. R. Goode. et al.(1998). Photospheric magnetic field changes associated with transition region explosive events. Astrophysical Journal.497(2):L109-L112. DOI: 10.1146/annurev.aa.10.090172.000445.
• [44]L. R. B. Rubio, C. Beck. (2005). Magnetic flux cancellation in the moat of sunspots: results from simultaneous vector spectropolarimetry in the visible and the infrared. Astrophysical Journal.626(2):L125-L128. DOI: 10.1146/annurev.aa.10.090172.000445.
• [45]L. Heggland, B. De Pontieu, V. H. Hansteen. (2009). Observational signatures of simulated reconnection events in the solar chromosphere and transition region. The Astrophysical Journal.702(1):1-18. DOI: 10.1146/annurev.aa.10.090172.000445.
• [46]D. E. Innes, R. H. Cameron, S. K. Solanki. (2011). EUV jets, type III radio bursts and sunspot waves investigated using SDO/AIA observations. Astronomy and Astrophysics.531, article L13. DOI: 10.1146/annurev.aa.10.090172.000445.
• [47]A. K. Srivastava, K. Murawski. (2011). Observations of a pulse-driven cool polar jet by SDO/AIA. Astronomy & Astrophysics.534, article A62. DOI: 10.1146/annurev.aa.10.090172.000445.
• [48]S. Chandrasekhar. (1961). Hydrodynamic and Hydromagnetic Stability. DOI: 10.1146/annurev.aa.10.090172.000445.
• [49]T. V. Zaqarashvili, I. Zhelyazkov, L. Ofman. (2015). Stability of rotating magnetized jets in the solar atmosphere. I. Kelvin–Helmholtz instability. Astrophysical Journal.813(2, article 123). DOI: 10.1146/annurev.aa.10.090172.000445.
• [50]D. Ryu, T. W. Jones, A. Frank. (2000). The magnetohydrodynamic Kelvin-Helmholtz instability: A three-dimensional study of nonlinear evolution. The Astrophysical Journal.545(1):475-493. DOI: 10.1146/annurev.aa.10.090172.000445.
• [51]S. A. Maslowe. (1985). Shear flow instabilities and transition. Hydromagnetic Instabilities and the Transition to Turbulence:181-228. DOI: 10.1146/annurev.aa.10.090172.000445.
• [52]T. E. Berger, G. Slater, N. Hurlburt, R. Shine. et al.(2010). Quiescent prominence dynamics observed with the Hinode solar optical telescope. I. Turbulent upflow plumes. The Astrophysical Journal.716(2):1288-1307. DOI: 10.1146/annurev.aa.10.090172.000445.
• [53]M. Ryutova, T. Berger, Z. Frank, T. Tarbell. et al.(2010). Observation of plasma instabilities in quiescent prominences. Solar Physics.267(1):75-94. DOI: 10.1146/annurev.aa.10.090172.000445.
• [54]D. Martínez-Gómez, R. Soler, J. Terradas. (2015). Onset of the Kelvin-Helmholtz instability in partially ionized magnetic flux tubes. Astronomy and Astrophysics.578, article A104. DOI: 10.1146/annurev.aa.10.090172.000445.
• [55]N. F. Loureiro, A. A. Schekochihin, D. A. Uzdensky. (2013). Plasmoid and Kelvin-Helmholtz instabilities in Sweet-Parker current sheets. Physical Review E: Statistical, Nonlinear, and Soft Matter Physics.87(1, article 013102). DOI: 10.1146/annurev.aa.10.090172.000445.
• [56]L. Feng, B. Inhester, W. Q. Gan. (2013). Kelvin–Helmholtz instability of a coronal streamer. Astrophysical Journal.774(2, article 141). DOI: 10.1146/annurev.aa.10.090172.000445.
• [57]C. Foullon, E. Verwichte, V. M. Nakariakov, K. Nykyri. et al.(2011). Magnetic Kelvin–Helmholtz instability at the Sun. Astrophysical Journal Letters.729(1, article L8). DOI: 10.1146/annurev.aa.10.090172.000445.
• [58]L. Ofman, B. J. Thompson. (2011). /AIA observation of Kelvin–Helmholtz instability in the solar corona. The Astrophysical Journal Letters.734(1, article L11). DOI: 10.1146/annurev.aa.10.090172.000445.
• [59]C. Foullon, E. Verwichte, K. Nykyri, M. J. Aschwanden. et al.(2013). Kelvin–Helmholtz instability of the CME reconnection outflow layer in the low corona. The Astrophysical Journal.767(2, article 170). DOI: 10.1146/annurev.aa.10.090172.000445.
• [60]U. V. Möstl, M. Temmer, A. M. Veronig. (2013). The Kelvin–Helmholtz instability at coronal mass ejection boundaries in the solar corona: Observations and 2.5D MHD simulations. Astrophysical Journal Letters.766(1, article 12). DOI: 10.1146/annurev.aa.10.090172.000445.
• [61]K. Nykyri, C. Foullon. (2013). First magnetic seismology of the CME reconnection outflow layer in the low corona with 2.5-D MHD simulations of the Kelvin-Helmholtz instability. Geophysical Research Letters.40(16):4154-4159. DOI: 10.1146/annurev.aa.10.090172.000445.
• [62]T. V. Zaqarashvili, A. J. Díaz, R. Oliver, J. L. Ballester. et al.(2010). Instability of twisted magnetic tubes with axial mass flows. Astronomy & Astrophysics.516, article A84. DOI: 10.1146/annurev.aa.10.090172.000445.
• [63]R. Soler, A. J. Díaz, J. L. Ballester, M. Goossens. et al.(2012). Kelvin–Helmholtz instability in partially ionized compressible plasmas. The Astrophysical Journal.749(2, article 163). DOI: 10.1146/annurev.aa.10.090172.000445.
• [64]T. V. Zaqarashvili. Solar spicules: recent challenges in observations and theory. .1356:106-116. DOI: 10.1146/annurev.aa.10.090172.000445.
• [65]I. Zhelyazkov. (2012). Magnetohydrodynamic waves and their stability status in solar spicules. Astronomy & Astrophysics.537, article A124. DOI: 10.1146/annurev.aa.10.090172.000445.
• [66]A. Ajabshirizadeh, H. Ebadi, R. E. Vekalati, K. Molaverdikhani. et al.(2015). The possibility of Kelvin-Helmholtz instability in solar spicules. Astrophysics and Space Science.357(1, article 33). DOI: 10.1146/annurev.aa.10.090172.000445.
• [67]I. Zhelyazkov, T. V. Zaqarashvili. (2012). Kelvin-Helmholtz instability of kink waves in photospheric twisted flux tubes. Astronomy & Astrophysics.547, article A14. DOI: 10.1146/annurev.aa.10.090172.000445.
• [68]I. Zhelyazkov, R. Chandra, A. K. Srivastava, T. Mishonov. et al.(2015). Kelvin–Helmholtz instability of magnetohydrodynamic waves propagating on solar surges. Astrophysics and Space Science.356(2):231-240. DOI: 10.1146/annurev.aa.10.090172.000445.
• [69]I. Zhelyazkov, T. V. Zaqarashvili, R. Chandra, A. K. Srivastava. et al.(2015). Kelvin–Helmholtz instability in solar cool surges. Advances in Space Research.56(12):2727-2737. DOI: 10.1146/annurev.aa.10.090172.000445.
• [70]I. Zhelyazkov, R. Chandra, A. K. Srivastava. (2015). Can magnetohydrodynamic waves traveling on solar dark mottles become unstable?. Bulgarian Journal of Physics.42(1):68-87. DOI: 10.1146/annurev.aa.10.090172.000445.
• [71]I. Zhelyazkov, T. V. Zaqarashvili, R. Chandra. (2015). Kelvin-Helmholtz instability in coronal mass ejecta in the lower corona. Astronomy and Astrophysics.574. DOI: 10.1146/annurev.aa.10.090172.000445.
• [72]I. Zhelyazkov, R. Chandra, A. K. Srivastava. Kelvin–Helmholtz instability in coronal mass ejections and solar surges. .1714. DOI: 10.1146/annurev.aa.10.090172.000445.
• [73]D. Kuridze, V. Henriques, M. Mathioudakis, R. Erdélyi. et al.(2015). The dynamics of rapid redshifted and blueshifted excursions in the solar H line. The Astrophysical Journal.802(1, article 26). DOI: 10.1146/annurev.aa.10.090172.000445.
• [74]I. Zhelyazkov. (2015). On modeling the Kelvin–Helmholtz instability in solar atmosphere. Journal of Astrophysics and Astronomy.36(1):233-254. DOI: 10.1146/annurev.aa.10.090172.000445.
• [75]S. Vasheghani Farahani, T. Van Doorsselaere, E. Verwichte, V. M. Nakariakov. et al.(2009). Propagating transverse waves in soft X-ray coronal jets. Astronomy & Astrophysics.498(2):L29-L32. DOI: 10.1146/annurev.aa.10.090172.000445.
• [76]I. Zhelyazkov. (2012). Review of the magnetohydrodynamic waves and their stability in solar spicules and X-ray jets. Topics in Magnethydrodynamics. DOI: 10.1146/annurev.aa.10.090172.000445.
• [77]I. Zhelyazkov. (2013). Kelvin–Helmholtz instability of kink waves in photospheric, chromospheric, and X-ray solar jets. Proceedings of the 4th School and Workshop on Space Plasma Physics.1551:150-164. DOI: 10.1146/annurev.aa.10.090172.000445.
• [78]M. Goossens, J. V. Hollweg, T. Sakurai. (1992). Resonant behaviour of MHD waves on magnetic flux tubes. III. Effect of equilibrium flow. Solar Physics.138(2):233-255. DOI: 10.1146/annurev.aa.10.090172.000445.
• [79]K. Hain, R. Lüst. (1958). Zur Stabilität zylindersymmetrischer Plasmakonfigurationen mit Volumenströmen. Zeitschrift für Naturforschung.13:936-940. DOI: 10.1146/annurev.aa.10.090172.000445.
• [80]J. P. Goedbloed. (1971). Stabilization of magnetohydrodynamic instabilities by force-free magnetic fields: I. Plane plasma layer. Physica.53(3):412-444. DOI: 10.1146/annurev.aa.10.090172.000445.
• [81]T. Sakurai, M. Goossens, J. V. Hollweg. (1991). Resonant behaviour of MHD waves on magnetic flux tubes. I. Connection formulae at the resonant surfaces. Solar Physics.133(2):227-245. DOI: 10.1146/annurev.aa.10.090172.000445.
• [82]P. M. Edwin, B. Roberts. (1983). Wave propagation in a magnetic cylinder. Solar Physics.88(1-2):179-191. DOI: 10.1146/annurev.aa.10.090172.000445.
• [83]M. Terra-Homem, R. Erdélyi, I. Ballai. (2003). Linear and non-linear MHD wave propagation in steady-state magnetic cylinders. Solar Physics.217(2):199-223. DOI: 10.1146/annurev.aa.10.090172.000445.
• [84]V. M. Nakariakov. (2007). MHD oscillations in solar and stellar coronae: current results and perspectives. Advances in Space Research.39(12):1804-1813. DOI: 10.1146/annurev.aa.10.090172.000445.
• [85]K. Bennett, B. Roberts, U. Narain. (1999). Waves in twisted magnetic flux tubes. Solar Physics.185(1):41-59. DOI: 10.1146/annurev.aa.10.090172.000445.
• [86]P. S. Cally. (1986). Leaky and non-leaky oscillations in magnetic flux tubes. Solar Physics.103(2):277-298. DOI: 10.1146/annurev.aa.10.090172.000445.
• [87]I. Zhelyazkov, R. Chandra, A. K. Srivastava. (2016). Kelvin-Helmholtz instability in an active region jet observed with Hinode. Astrophysics and Space Science.361(2, article 51). DOI: 10.1146/annurev.aa.10.090172.000445.
• [88]T. V. Zaqarashvili, Z. Vörös, I. Zhelyazkov. (2014). Kelvin-Helmholtz instability of twisted magnetic flux tubes in the solar wind. Astronomy & Astrophysics.561, article A62. DOI: 10.1146/annurev.aa.10.090172.000445.
• [89]J. W. Dungey, R. E. Loughhead. (1954). Twisted magnetic fields in conducting fluids. Australian Journal of Physics.7(1):5-13. DOI: 10.1146/annurev.aa.10.090172.000445.
• [90]A. R. Paraschiv, A. Bemporad, A. C. Sterling. (2015). Physical properties of solar polar jets: A statistical study with Hinode XRT data. Astronomy & Astrophysics.579, article A96. DOI: 10.1146/annurev.aa.10.090172.000445.
• [91]T. Miyagoshi, T. Yokoyama. (2003). Magnetohydrodynamic numerical simulations of solar X-ray jets based on the magnetic reconnection model that includes chromospheric evaporation. The Astrophysical Journal.593(2):L133-L136. DOI: 10.1146/annurev.aa.10.090172.000445.