Review of Fast Solar Jets and Coronal Mass Ejections

Document Type : Review Paper

Authors

1 Department of Physics, Tabriz Branch, Islamic Azad University, Tabriz, Iran

2 Physics Department, Payame Noor University (PNU), 19395-3697-Tehran, I. R. of Iran

Abstract

The Sun is a magnetically active star. It has a powerful magnetic field that shifts slightly from year to year until it reverses about every eleven years. The sun's magnetic field has many effects, the collection of which is called solar activity such as, sunspots, solar flares, and coronal mass ejections(CMEs). Currently, it is only possible to predict a magnetic storm 30 to 60 minutes before it occurs, which is a very short time. Solar flares and CMEs, massive eruptions of superheated plasma, are the two most energetic phenomenon which impulsively ejected and accelerated by releasing magnetic energy in the solar corona. Heliosphere, space weather, and the Earth are affected from transporting coronal plasma. Following the occurrence of these phenomenon in the Sun, the solar wind blows with greater speed and intensity and sends energetic charged particles into the space of the solar system. When these particles reach the Earth, their radiating electromagnetic waves interact with magnetic field of the Earth. Then various effects are observed, as shock waves and massive geomagnetic storms that disrupt satellites and power grids. Today, using the advancements of ground and space technology, the solar surface can be easily observed. Therefore, observation and prediction of solar storm will be possible more than in the past. In this paper, we review papers intended to collect comprehensive information about what has already been researched about fast solar jets and CMEs made by ground and space instruments over the last decades.

Keywords

References

[1] Ajabshirizadeh, A., Tavabi, E., & Koutchmy, S. 2008, New Astron., 13, 93.
[2] Ajabshirizadeh, A., Tavabi, & E., Koutchmy, S. 2009, A&SS, 319, 31.
[3] Ajabshirizadeh, A., Koutchmy, S., & Tavabi, E. 2008, Resolution Effect in the Solar Spicules Oscillations, 12th European Solar Physics Meeting, Freiburg, Germany, held September, ESPM, 12, 44.
[4] Ajabshirizadeh, A., Tavabi, E., & Koutchmy, S. 2008, Magneto-Acoustic Wave (KINK) Oscillations In Solar Spicules First Middle East and Africa IAU-Regional Meeting Proceedings MEARIM, 1, 109.
[5] Almeida, J. S., Bonet, J. A., Viticchi, B., & Moro, D. D. 2010, ApJL, 715, L26.
[6] Alipour, N., & Safari, H. 2015, ApJ, 807, 175.
[7] Alipour, N., & Safari, H. 2019, IJPR. 12, 29.
[8] Alipour, N., Safari, H., Verbeeck, C., Berghmans, D., & et al. 2022, A&A, 663, 12.
[9] Alipour, N., Safari, H., & Innes, D. 2012, ApJ, 746, 8.
[10] Abramenko, V., Yurchyshyn, V., Goode, P., Kilcik, A. 2010, ApJ, 725, L101.
[11] Amirkhanlou, E., Tavabi, E., & Zeighami, S. 2018, JESP, 44, 674.
[12] Athay, R. G. 1961, ApJ, 134, 756.
[13] Athay, R. G. ApJ, 66, 278.
[14] Athay, R. G. 1974, Radiation Pressure in Stellar Atmospheres with Application to Solar Spicules, Cambridge University Press.
[15] Balasis, G., Papadimitriou, C., & Boutsi, A. Z. 2019, Ionospheric response to solar and interplanetary disturbances: a Swarm perspective. Philosophical Transactions of the Royal Society of London Series A, 377, 20180098.
[16] Bazin, C., Koutchmy, S., & Tavabi, E. 2012, Prominence-cavity regions observed in 2010 eclipse flash spectra and SWAP images, EAS, 55, 185B.
[17] Beckers, J. M. 1968, SoPh, 3, 367.
[18] Berger, T. E., Lofdahl, M. G., Shine, R. A., & Title, A. M. 1998, ApJ, 506, 439.
[19] Brueckner, G. E., & Bartoe, J. D. F. 1983, ApJ. 272, 329.
[20] Brueckner, G. E. 1980, in Highlights in Astron. Reidel Publ. 5, 557.
[21] Brueckner, G. E. 1981, Space Sci. Rev., 29, 407.
[22] Bohlin, J. D., Vogel, S. N., Purcell, J. D., Sheeley, N. R., Jr., Tousey, R., & Vanhoosier, M. E. 1975, ApJ. 197, L133.
[23] Beckers, J. M. 1966, ApJ, 71, 155.
[24] Chae, J. Qiu, J. Wang, H., & Goode, P. R. 1999, ApJL. 513, L75.
[25] Cheng, Q. Q., Ulmschneider, P., & Korevaar, P. 1991, Mechanisms of Chromospheric and Coronal Heating, Proceedings of the International Conference, New York, 350.
[26] Chen, P. F. 2011, Coronal Mass Ejections: Models and Their Observational Basis. Living Reviews in Solar Physics, 8.
[27] Cirtain, J. W., & et al. 2007, Science, 318, 1580.
[28] Daw, A., DeLuca, E. E., & Golub, L. 1995, ApJ, 453, 929.
[29] Defouw, R. J. 1976, ApJ, 209, 266.
[30] de la Cruz Rodrguez, J., Pontieu, B. D., Carlsson, M., & Van der Voort, L. H. M. R. 2013, ApJ, 764, L11.
[31] De Pontieu, B., Carlsson, M., Rouppe van der Voort, L. H. M., & et al. 2012, ApJ, 752, L12.
[32] De Pontieu, B., Erdlyi, R., & James, S. P. 2004, Nature, 430, 536.
[33] Dere, K. P., Bartoe, J. D. F., & Brueckner, G. E. 1983, ApJ, 2, 267.
[34] Dere, K. P. Bartoe, J. D., & Brueckner, G. E. 1989, SoPh. 123, 41.
[35] de Wijn, A. G., Lites, B. W., Berger, T. E., Frank, Z. A., Tarbell, T. D., & Ishikawa, R. 2008, ApJ, 684, 1469.
[36] Dunn, R. B., Zirker, J. B. 1973, SoPh, 33, 281.
[37] Filippov, B., Koutchmy, S., & Tavabi, E. 2013, SoPh. 286, 143.
[38] Filippov, B., Koutchmy, S., & Golub, L. 2009, Geomagnetism and Aeronomy, 49, 1109.
[39] Golub, L., Krieger, A. S., & Vaiana, G. S., 1975, SoPh., 42, 131.
[40] Georgakilas, A. A., Koutchmy, S., & Alissandrakis, C. F. 1999, A&A, 341, 610.
[41] Guo, L.-J., Tian, H., & He, J.-S. 2010, ApJ, 10, 1307.
[42] Haerendel, G. 1992, Nature, 360, 241.
[43] Moore, R. L., Cirtain, J. W., Sterling, A. C., & Falconer, D. A. 2010, ApJ, 720, 757.
[44] Halain, J. P., Berghmans, D., Defise, J. M., Renotte, E., Thibert, T., Mazy, E., & et al. 2010, Space Telescopes and Instrumentation, Ultraviolet to Gamma Ray, Proceedings of the SPIE, 7732, 77320P.
[45] Harrison, R. A., Bryans, P., & Bingham, R. 2001, A&A, 379, 324.
[46] Hofmeister, U., Dominik, H., & Stephan, G. 2019, Veronig, Astrid Temmer, Manuela, A&A.
[47] Honarbakhsh, L., Alipour, N., & Safari, H. 2016, SoPh. 291, 941.
[48] Innes, D. E., Inhester, B., Axford, W. I., & Wilhelm, K. 1997, Nature, 386, 811.
[49] Jafarzadeh, S., Solanki, S. K., Stangalini, M., Steiner, O., Cameron, R. H., & Danilovic, S. 2017, ApJ, 229, 10.
[50] Javaherian, M., Safari, H., Dadashi, N., & Aschwanden, M., 2017, SoPh, 292, 15.
[51] Jess, D. B., Mathioudakis, M., Christian, D. J., Crockett, P. J., & Keenan F. P. 2010.
[52] Kayshap, P., & Dwivedi, B. N. 2017, SoPh, 292, 108.
[53] Koutchmy, S., & Stellmacher, G. 1976, SoPh., 49, 253.
[54] Koutchmy, S., & Loucif, M. L. 1991, in: Ulmschneider P., Priest E. R., Ros-ner R. (eds.), Springer-Verlag, 152.
[55] Koutchmy, S., Hara, H., Suematsu, Y., Reardon, K. 1997, A&A, 320, L33.
[56] Koutchmy, S., Hara, H., Shibata, K., Suematsu, Y., & Reardon, K. 1998, In: Watanabe, T., Kosugi, T., Sterling, A. C.
[57] Koutchmy, S., Filippov, B., Tavabi, E., Bazin, C., & Weiller, S. 2013, Nature of Prominences and their role in Space Weather Proceedings IAU Symposium.
[58] Koutchmy, S., Tavabi, E., & Urtado, O. 2018, MNRAS., 478.
[59] Lamy, P. L., Floyd, O., Boclet, B., Wojak, J., Gilardy, H. & Barlyaeva, T. 2019, Space Sci. Rev., 215, 39.
[60] Lites, B. W., Rutten, R. J., & Kalkofen, W. 1993, Apj, 414, 345.
[61] Lites, B. W., Thomas, J. H., Bogdan, T. J., & Cally, P. S. 1998, ApJ, 497, 464.
[62] Madjarska, M. S., Doyle, J. G., Teriaca, L., & Banerjee, D. 2003, A&A, 398, 775.
[63] Moore, R. L., Tang, F., Bohlin, J. D., & Golub, L. 1977, ApJ. 218, 286.
[64] Muller, R., Dollfus, A., Montagne, M., Moity, J., & Vigneau, J. 2000, A&A, 359, 373.
[65] Parmenter, B. C. 1966, Publications of the Astronomical Society of the Pacific, 78, 463.
[66] Pasachoff, J. M., Jacobson, W. A., & Sterling, A. C., 2009, SoPh. 260, 59.
[67] Papushev, P. G., & Salakhutdinov, R. T. 1994, ApJ, 136, 250.
[68] Patsourakos, S., Pariat, E., Vourlidas, A., Antiochos, S. K., & Wuelser, J. P. 2008, ApJ, 680, L73.
[69] Roberts, W. O. 1945, ApJ, 101, 136.
[70] Rubio, L. B., & Suarez, D. O. 2019, Living Reviews in Solar Physics, 16, 1.
[71] Roudier, T., Rieutord, M., Brito, D., Rincon, F., Malherbe, J. M., Meunier, N., Berger, T., & Frank, Z. 2009, A&A, 495, 945. 945
[72] Rush, J. H., & Roberts, W. O. 1953, ApJ, 58, 226.
[73] Sadeghi, R., & Tavabi, E. 2022, ApJ, 938, 945.
[74] Sadeghi, R., & Tavabi, E. 2022, MNRAS, 512, 4164.
[75] Sheeley, N. R., & Golub L. 1979, SoPh, 63, 119.
[76] Sheeley, N. R. 1967, SoPh, 1, 171.
[77] Shibata, K., & Magara, T. 2011, Solar Flares: Magnetohydrodynamic Processes. Living Rev. Solar Phys., 8.
[78] Shibata, K., Nitta, N., Strong, K. T., Matsumoto, R., Yokoyama, T., Hirayama, T., Hudson, H., & Ogawara, Y. 1994, ApJL. 431, L51.
[79] Shimojo, M., Hashimoto, S., Shibata, K., Hirayama, T., Hudson, H. S., & Acton, L. 1996, Publ. Astron. Soc. Japan, 48, 123.
[80] Shimojo, M., Narukage, N., Kano, R., Sakao, T., Tsuneta, S., Shibasaki, K., & et al. 2007, Publ. Astron. Soc. Japan, 59, S625.
[81] Simon, G. W., & Leighton, R. B. 1964, ApJ, 140, 1120.
[82] Singh, K. A. P., Isobe, H., Nishida, K., & Shibata, K. 2012, ApJ, 760, 28.
[83] Snodgrass, H. B., & Ulrich, R. K. 1990, ApJ, 351, 309.
[84] Stangalini, M., Giannattasio, F., Moro, D. D., & Berrilli, F. 2012, A&A, 539, L4.
[85] Sterling, H. C. 2000, SoPh., 196, 79.
[86] Sterling, A. C., Harra, L. K., & Moore, R. L. 2010, ApJ, 722, 1644.
[87] Suematsu, Y., Ichimoto, K., Katsukawa, Y., Shimizu, T., Okamoto, T., Tsuneta, S., Tarbell, T., & Shine, R. A. 2008, Astron. Soc. Pac., 397, 27.
[88] Tavabi, E., Koutchmy, S., & Ajabshirzadeh, A. 2011, New Astron., 16, 296.
[89] Tavabi, E., Koutchmy, S., & Ajabshirizadeh, A. 2011, Adv. Space Res., 47.
[90] Tavabi, E. 2012, J. Modern Physics, 3, 11, 1786.
[91] Tavabi, E., Koutchmy, S., & Ajabshirizadeh, A. 2013, SoPh., 283, 187.
[92] Tavabi, E., & Koutchmy, S. 2014, Ap&SS, 352, 7T.
[93] Tavabi, E. 2014, Ap&SS, 350, 489.
[94] Tavabi, E. 2014, Ap&SS, 352, 43.
[95] Tavabi, E., Koutchmy, S., & Bazin, C. 2018, SoPh., 293, 42T.
[96] Tavabi, E., Ajabshirizadeh, A., Ahangarzadeh Maralani, A. R., & Zeighami, S. 2015, J. ApA, 41, 18.
[97] Tavabi, E., Koutchmy, S., Ajabshirizadeh, A., Ahangarzadeh Maralani, A. R., & Zeighami, S. 2015, A&A, 573, 7.
[98] Tavabi, E., Koutchmy, S., & Golub, L. 2015, SoPh., 290, 2871.
[99] Tavabi, E., Koutchmy, S., & Golub, L. 2018, ApJ, 866, 35.
[100] Tavabi, E. 2018, MNRAS, 476, 868.
[101] Tavabi, E., & Koutchmy, S. 2019, ApJ, 883, 41.
[102] Tavabi, E., Zeighami, S., & Heydari, M. 2022, SoPh., 297, 76.
[103] Tavabi, E., & Sadeghi, R. 2022, JESP, 48, 749.
[104] Tavabi, E., Rajabi, M., & Zeighami, S. 2022, IJAA.
[105] Tavabi, E., & Zeighami, S. 2022, IJAA.
[106] Tsiropoula, G., Tziotziou, K., Kontogiannis, I., & et al. 2012, Space Sci. Rev., 169, 181.
[107] Utz Hanslmeier, A., Mostl, C., Muller, R., Veronig, A., & Muthsam, H. 2009, A&A, 498, 289.
[108] Yokoyama, T., & Shibata K. 1995, Nature, 375, 42.
[109] Yokoyama, T., & Shibata, K. 1996, PASJ, 48, 353.
[110] Wang, Y. M., & Sheeley, N. R. 2002, ApJ, 575, 542.
[111] Webb, D. F., & Howard, T. A. 2012, Coronal Mass Ejections: Observations, Living Reviews in Solar Physics, 9.
[112] Wulser, J.-P., Lemen, J. R., Tarbell, T. D., Wolfson, C. J., Cannon, J. C., Brock, A., & Carpenter, B. A., 2004, Telescopes and Instrumentation for Solar Astrophysics, Proc. SPIE 5171, 111.
[113] Xiong, J., Yang, Y., Jin, C., Ji, K., Feng, S., Wang, F., Deng, H., & Hu, Y. 2017, ApJ.
[114] Yamauchi, Y., Wang, H., Jiang, Y., Schwandron, N., & Moore, R. L. 2005, ApJ, 629, 572.
[115] Zeighami, S., Ahangarzadeh Maralani, A. R., Tavabi, E., & Ajabshirizadeh, A. 2016, SoPh., 291, 847.
[116] Zeighami, S., Tavabi, E., & Amirkhanlou, E. 2020, JApA., 41, 18Z.
[117] Zeighami, S., & Tavabi, E. 2021, JESP, 44, 671.
[118] Zeighami, S., & Tavabi, E. 2021, IJAA.
[119] Zeighami, S., Tavabi, E., & Ajabshirizadeh, A. 2023, JESP.
[120] Zirker, J. B. 1962, ApJ, 135, 515.
[121] Zirker, J. B. 1962, ApJ, 136, 250.
Iranian Journal of Astronomy and Astrophysics
Volume 10, Issue 1
March 2023
Pages 11-60

Files

Share

How to cite

Statistics