Abstract
The Coronal Multichannel Polarimeter (CoMP) measures not only the polarization of coronal emission, but also the full radiance profiles of coronal emission lines. For the first time, CoMP observations provide high-cadence image sequences of the coronal line intensity, Doppler shift, and line width simultaneously over a large field of view. By studying the Doppler shift and line width we may explore more of the physical processes of the initiation and propagation of coronal mass ejections (CMEs). Here we identify a list of CMEs observed by CoMP and present the first results of these observations. Our preliminary analysis shows that CMEs are usually associated with greatly increased Doppler shift and enhanced line width. These new observations provide not only valuable information to constrain CME models and probe various processes during the initial propagation of CMEs in the low corona, but also offer a possible cost-effective and low-risk means of space-weather monitoring.
Keywords
Coronal Magnetometry
Guest Editors: S. Tomczyk, J. Zhang, and T.S. Bastian
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Aschwanden, M.J., Fletcher, L., Schrijver, C.J., Alexander, D.: 1999, Coronal loop oscillations observed with the Transition Region and Coronal Explorer. Astrophys. J. 520, 880 – 894. doi:10.1086/307502.
Brueckner, G.E., Howard, R.A., Koomen, M.J., Korendyke, C.M., Michels, D.J., Moses, J.D., Socker, D.G., Dere, K.P., Lamy, P.L., Llebaria, A., Bout, M.V., Schwenn, R., Simnett, G.M., Bedford, D.K., Eyles, C.J.: 1995, The Large Angle Spectroscopic Coronagraph (LASCO). Solar Phys. 162, 357 – 402. doi:10.1007/BF00733434.
Chen, F., Ding, M.D., Chen, P.F.: 2010, Spectroscopic analysis of an EIT wave/dimming observed by Hinode/EIS. Astrophys. J. 720, 1254 – 1261. doi:10.1088/0004-637X/720/2/1254.
Chen, P.F., Wu, S.T., Shibata, K., Fang, C.: 2002, Evidence of EIT and Moreton waves in numerical simulations. Astrophys. J. Lett. 572, L99 – L102. doi:10.1086/341486.
Chen, Y., Feng, S.W., Li, B., Song, H.Q., Xia, L.D., Kong, X.L., Li, X.: 2011, A coronal seismological study with streamer waves. Astrophys. J. 728, 147. doi:10.1088/0004-637X/728/2/147.
Cheng, X., Zhang, J., Liu, Y., Ding, M.D.: 2011, Observing flux rope formation during the impulsive phase of a solar eruption. Astrophys. J. Lett. 732, L25. doi:10.1088/2041-8205/732/2/L25.
Culhane, J.L., Harra, L.K., James, A.M., Al-Janabi, K., Bradley, L.J., Chaudry, R.A., Rees, K., Tandy, J.A., Thomas, P., Whillock, M.C.R., Winter, B., Doschek, G.A., Korendyke, C.M., Brown, C.M., Myers, S., Mariska, J., Seely, J., Lang, J., Kent, B.J., Shaughnessy, B.M., Young, P.R., Simnett, G.M., Castelli, C.M., Mahmoud, S., Mapson-Menard, H., Probyn, B.J., Thomas, R.J., Davila, J., Dere, K., Windt, D., Shea, J., Hagood, R., Moye, R., Hara, H., Watanabe, T., Matsuzaki, K., Kosugi, T., Hansteen, V., Wikstol, Ø.: 2007, The EUV Imaging Spectrometer for Hinode. Solar Phys. 243, 19 – 61. doi:10.1007/s01007-007-0293-1.
DeForest, C.E., Howard, T.A., Tappin, S.J.: 2011, Observations of detailed structure in the solar wind at 1 AU with STEREO/HI-2. Astrophys. J. 738, 103. doi:10.1088/0004-637X/738/1/103.
Dove, J.B., Gibson, S.E., Rachmeler, L.A., Tomczyk, S., Judge, P.: 2011, A ring of polarized light: evidence for twisted coronal magnetism in cavities. Astrophys. J. Lett. 731, L1. doi:10.1088/2041-8205/731/1/L1.
Edwin, P.M., Roberts, B.: 1983, Wave propagation in a magnetic cylinder. Solar Phys. 88, 179 – 191. doi:10.1007/BF00196186.
Elmore, D.F., Burkepile, J.T., Darnell, J.A., Lecinski, A.R., Stanger, A.L.: 2003, Calibration of a ground-based solar coronal polarimeter. In: Fineschi, S. (ed.) Soc. Photo-Optical Instrument. Eng. (SPIE) CS-4843, 66 – 75. doi:10.1117/12.459279.
Feng, S.W., Chen, Y., Li, B., Song, H.Q., Kong, X.L., Xia, L.D., Feng, X.S.: 2011, Streamer wave events observed in solar cycle 23. Solar Phys. 272, 119 – 136. doi:10.1007/s11207-011-9814-6.
Forland, B., Rachmeler, L.A., Gibson, S.E., Dove, J.: 2011, Cavity magnetic observations: a survey using AIA and CoMP data. AGU Fall Meeting Abstracts, B1951.
Gibson, S.E., Foster, D., Burkepile, J., de Toma, G., Stanger, A.: 2006, The calm before the storm: the link between quiescent cavities and coronal mass ejections. Astrophys. J. 641, 590 – 605. doi:10.1086/500446.
Giordano, S., Ciaravella, A., Raymond, J., Ko, Y.K., Suleiman, R.: 2013, UVCS/SoHO catalog of coronal mass ejections from 1996 to 2005: spectroscopic proprieties. J. Geophys. Res. 118, 967 – 981. doi:10.1002/jgra.50166.
Gopalswamy, N., Lara, A., Yashiro, S., Kaiser, M.L., Howard, R.A.: 2001, Predicting the 1-AU arrival times of coronal mass ejections. J. Geophys. Res. 106, 29207 – 29218. doi:10.1029/2001JA000177.
Gosling, J.T., McComas, D.J., Phillips, J.L., Bame, S.J.: 1991, Geomagnetic activity associated with Earth passage of interplanetary shock disturbances and coronal mass ejections. J. Geophys. Res. 96, 7831 – 7839. doi:10.1029/91JA00316.
Harra, L.K., Sterling, A.C.: 2003, Imaging and spectroscopic investigations of a solar coronal wave: properties of the wave front and associated erupting material. Astrophys. J. 587, 429 – 438. doi:10.1086/368079.
Harrison, R.A., Bryans, P., Simnett, G.M., Lyons, M.: 2003, Coronal dimming and the coronal mass ejection onset. Astron. Astrophys. 400, 1071 – 1083. doi:10.1051/0004-6361:20030088.
Hassler, D.M., Dammasch, I.E., Lemaire, P., Brekke, P., Curdt, W., Mason, H.E., Vial, J.C., Wilhelm, K.: 1999, Solar wind outflow and the chromospheric magnetic network. Science 283, 810. doi:10.1126/science.283.5403.810.
Howard, T.A., Webb, D.F., Tappin, S.J., Mizuno, D.R., Johnston, J.C.: 2006, Tracking halo coronal mass ejections from 0 – 1 AU and space weather forecasting using the Solar Mass Ejection Imager (SMEI). J. Geophys. Res. 111, 4105. doi:10.1029/2005JA011349.
Jin, M., Ding, M.D., Chen, P.F., Fang, C., Imada, S.: 2009, Coronal mass ejection induced outflows observed with Hinode/EIS. Astrophys. J. 702, 27 – 38. doi:10.1088/0004-637X/702/1/27.
Ko, Y.K., Raymond, J.C., Lin, J., Lawrence, G., Li, J., Fludra, A.: 2003, Dynamical and physical properties of a post-coronal mass ejection current sheet. Astrophys. J. 594, 1068 – 1084. doi:10.1086/376982.
Kohl, J.L., Esser, R., Gardner, L.D., Habbal, S., Daigneau, P.S., Dennis, E.F., Nystrom, G.U., Panasyuk, A., Raymond, J.C., Smith, P.L., Strachan, L., van Ballegooijen, A.A., Noci, G., Fineschi, S., Romoli, M., Ciaravella, A., Modigliani, A., Huber, M.C.E., Antonucci, E., Benna, C., Giordano, S., Tondello, G., Nicolosi, P., Naletto, G., Pernechele, C., Spadaro, D., Poletto, G., Livi, S., von der Lühe, O., Geiss, J., Timothy, J.G., Gloeckler, G., Allegra, A., Basile, G., Brusa, R., Wood, B., Siegmund, O.H.W., Fowler, W., Fisher, R., Jhabvala, M.: 1995, The Ultraviolet Coronagraph Spectrometer for the Solar and Heliospheric Observatory. Solar Phys. 162, 313 – 356. doi:10.1007/BF00733433.
Landi, E., Raymond, J.C., Miralles, M.P., Hara, H.: 2010, Physical conditions in a coronal mass ejection from Hinode, Stereo, and SOHO observations. Astrophys. J. 711, 75 – 98. doi:10.1088/0004-637X/711/1/75.
Lemen, J.R., Title, A.M., Akin, D.J., Boerner, P.F., Chou, C., Drake, J.F., Duncan, D.W., Edwards, C.G., Friedlaender, F.M., Heyman, G.F., Hurlburt, N.E., Katz, N.L., Kushner, G.D., Levay, M., Lindgren, R.W., Mathur, D.P., McFeaters, E.L., Mitchell, S., Rehse, R.A., Schrijver, C.J., Springer, L.A., Stern, R.A., Tarbell, T.D., Wuelser, J.P., Wolfson, C.J., Yanari, C., Bookbinder, J.A., Cheimets, P.N., Caldwell, D., Deluca, E.E., Gates, R., Golub, L., Park, S., Podgorski, W.A., Bush, R.I., Scherrer, P.H., Gummin, M.A., Smith, P., Auker, G., Jerram, P., Pool, P., Soufli, R., Windt, D.L., Beardsley, S., Clapp, M., Lang, J., Waltham, N.: 2012, The Atmospheric Imaging Assembly (AIA) on the Solar Dynamics Observatory (SDO). Solar Phys. 275, 17 – 40. doi:10.1007/s11207-011-9776-8.
Lin, J., Ko, Y.K., Sui, L., Raymond, J.C., Stenborg, G.A., Jiang, Y., Zhao, S., Mancuso, S.: 2005, Direct observations of the magnetic reconnection site of an eruption on 2003 November 18. Astrophys. J. 622, 1251 – 1264. doi:10.1086/428110.
Liu, Y., Luhmann, J.G., Lin, R.P., Bale, S.D., Vourlidas, A., Petrie, G.J.D.: 2009, Coronal mass ejections and global coronal magnetic field reconfiguration. Astrophys. J. Lett. 698, L51 – L55. doi:10.1088/0004-637X/698/1/L51.
Low, B.C., Hundhausen, J.R.: 1995, Magnetostatic structures of the solar corona. 2: The magnetic topology of quiescent prominences. Astrophys. J. 443, 818 – 836. doi:10.1086/175572.
McIntosh, S.W., de Pontieu, B., Tomczyk, S.: 2008, A coherence-based approach for tracking waves in the solar corona. Solar Phys. 252, 321 – 348. doi:10.1007/s11207-008-9257-x.
McIntosh, S.W., de Pontieu, B., Leamon, R.J.: 2010, The impact of new EUV diagnostics on CME-related kinematics. Solar Phys. 265, 5 – 17. doi:10.1007/s11207-010-9538-z.
Mierla, M., Schwenn, R., Teriaca, L., Stenborg, G., Podlipnik, B.: 2005, Using LASCO-C1 spectroscopy for coronal diagnostics. Adv. Space Res. 35, 2199 – 2203. doi:10.1016/j.asr.2005.04.031.
Nakariakov, V.M., Ofman, L.: 2001, Determination of the coronal magnetic field by coronal loop oscillations. Astron. Astrophys. 372, L53 – L56. doi:10.1051/0004-6361:20010607.
O’Dwyer, B., Del Zanna, G., Mason, H.E., Weber, M.A., Tripathi, D.: 2010, SDO/AIA response to coronal hole, quiet Sun, active region, and flare plasma. Astron. Astrophys. 521, A21. doi:10.1051/0004-6361/201014872.
Patsourakos, S., Vourlidas, A.: 2009, “Extreme ultraviolet waves” are waves: first quadrature observations of an extreme ultraviolet wave from STEREO. Astrophys. J. Lett. 700, L182 – L186. doi:10.1088/0004-637X/700/2/L182.
Peter, H., Judge, P.G.: 1999, On the Doppler shifts of solar ultraviolet emission lines. Astrophys. J. 522, 1148 – 1166. doi:10.1086/307672.
Plunkett, S.P., Brueckner, G.E., Dere, K.P., Howard, R.A., Koomen, M.J., Korendyke, C.M., Michels, D.J., Moses, J.D., Moulton, N.E., Paswaters, S.E., St. Cyr, O.C., Socker, D.G., Wang, D., Simnett, G.M., Bedford, D.K., Biesecker, D.A., Eyles, C.J., Tappin, S.J., Schwenn, R., Lamy, P.L., Llebaria, A.: 1997, The relationship of green-line transients to white-light coronal mass ejections. Solar Phys. 175, 699 – 718. doi:10.1023/A:1004981125702.
Rachmeler, L.A., Gibson, S.E., Dove, J.B., DeVore, C.R., Fan, Y.: 2013, Polarimetric properties of flux ropes and sheared arcades in coronal prominence cavities. Solar Phys. accepted.
Reiner, M.J., Vourlidas, A., Cyr, O.C.S., Burkepile, J.T., Howard, R.A., Kaiser, M.L., Prestage, N.P., Bougeret, J.L.: 2003, Constraints on coronal mass ejection dynamics from simultaneous radio and white-light observations. Astrophys. J. 590, 533 – 546. doi:10.1086/374917.
Schmit, D.J., Gibson, S.E., Tomczyk, S., Reeves, K.K., Sterling, A.C., Brooks, D.H., Williams, D.R., Tripathi, D.: 2009, Large-scale flows in prominence cavities. Astrophys. J. Lett. 700, L96 – L98. doi:10.1088/0004-637X/700/2/L96.
Schwenn, R., Inhester, B., Plunkett, S.P., Epple, A., Podlipnik, B., Bedford, D.K., Eyles, C.J., Simnett, G.M., Tappin, S.J., Bout, M.V., Lamy, P.L., Llebaria, A., Brueckner, G.E., Dere, K.P., Howard, R.A., Koomen, M.J., Korendyke, C.M., Michels, D.J., Moses, J.D., Moulton, N.E., Paswaters, S.E., Socker, D.G., St. Cyr, O.C., Wang, D.: 1997, First view of the extended green-line emission corona at solar activity minimum using the LASCO-C1 coronagraph on SOHO. Solar Phys. 175, 667 – 684. doi:10.1023/A:1004948913883.
Shen, Y., Liu, Y.: 2012, Evidence for the wave nature of an extreme ultraviolet wave observed by the Atmospheric Imaging Assembly on board the Solar Dynamics Observatory. Astrophys. J. 754, 7. doi:10.1088/0004-637X/754/1/7.
Su, Y., van Ballegooijen, A.: 2012, Observations and magnetic field modeling of a solar polar crown prominence. Astrophys. J. 757, 168. doi:10.1088/0004-637X/757/2/168.
Temmer, M., Veronig, A.M., Kontar, E.P., Krucker, S., Vršnak, B.: 2010, Combined STEREO/RHESSI study of coronal mass ejection acceleration and particle acceleration in solar flares. Astrophys. J. 712, 1410 – 1420. doi:10.1088/0004-637X/712/2/1410.
Tian, H., Tu, C., Marsch, E., He, J., Kamio, S.: 2010, The nascent fast solar wind observed by the EUV imaging spectrometer on board Hinode. Astrophys. J. Lett. 709, L88 – L93. doi:10.1088/2041-8205/709/1/L88.
Tian, H., McIntosh, S.W., Xia, L., He, J., Wang, X.: 2012a, What can we learn about solar coronal mass ejections, coronal dimmings, and extreme-ultraviolet jets through spectroscopic observations? Astrophys. J. 748, 106. doi:10.1088/0004-637X/748/2/106.
Tian, H., McIntosh, S.W., Wang, T., Ofman, L., De Pontieu, B., Innes, D.E., Peter, H.: 2012b, Persistent Doppler shift oscillations observed with Hinode/EIS in the solar corona: spectroscopic signatures of Alfvénic waves and recurring upflows. Astrophys. J. 759, 144. doi:10.1088/0004-637X/759/2/144.
Tomczyk, S., McIntosh, S.W.: 2009, Time–distance seismology of the solar corona with CoMP. Astrophys. J. 697, 1384 – 1391. doi:10.1088/0004-637X/697/2/1384.
Tomczyk, S., McIntosh, S.W., Keil, S.L., Judge, P.G., Schad, T., Seeley, D.H., Edmondson, J.: 2007, Alfvén waves in the solar corona. Science 317, 1192. doi:10.1126/science.1143304.
Tomczyk, S., Card, G.L., Darnell, T., Elmore, D.F., Lull, R., Nelson, P.G., Streander, K.V., Burkepile, J., Casini, R., Judge, P.G.: 2008, An instrument to measure coronal emission line polarization. Solar Phys. 247, 411 – 428. doi:10.1007/s11207-007-9103-6.
Van Doorsselaere, T., Nakariakov, V.M., Verwichte, E.: 2008, Detection of waves in the solar corona: kink or Alfvén? Astrophys. J. Lett. 676, L73 – L75. doi:10.1086/587029.
Wang, T.J., Solanki, S.K.: 2004, Vertical oscillations of a coronal loop observed by TRACE. Astron. Astrophys. 421, L33 – L36. doi:10.1051/0004-6361:20040186.
Wang, Y.M., Ye, P.Z., Wang, S., Zhou, G.P., Wang, J.X.: 2002, A statistical study on the geoeffectiveness of Earth-directed coronal mass ejections from March 1997 to December 2000. J. Geophys. Res. 107, 1340. doi:10.1029/2002JA009244.
White, R.S., Verwichte, E.: 2012, Transverse coronal loop oscillations seen in unprecedented detail by AIA/SDO. Astron. Astrophys. 537, A49. doi:10.1051/0004-6361/201118093.
Zhang, M., Low, B.C.: 2005, The hydromagnetic nature of solar coronal mass ejections. Annu. Rev. Astron. Astrophys. 43, 103 – 137. doi:10.1146/annurev.astro.43.072103.150602.
Zhang, J., Dere, K.P., Howard, R.A., Kundu, M.R., White, S.M.: 2001, On the temporal relationship between coronal mass ejections and flares. Astrophys. J. 559, 452 – 462. doi:10.1086/322405.
Zhang, J., Richardson, I.G., Webb, D.F., Gopalswamy, N., Huttunen, E., Kasper, J.C., Nitta, N.V., Poomvises, W., Thompson, B.J., Wu, C.C., Yashiro, S., Zhukov, A.N.: 2007, Solar and interplanetary sources of major geomagnetic storms (Dst=−100 nT) during 1996 – 2005. J. Geophys. Res. 112(11), 10102. doi:10.1029/2007JA012321.
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Tian, H., Tomczyk, S., McIntosh, S.W., Bethge, C., de Toma, G., Gibson, S. (2013). Observations of Coronal Mass Ejections with the Coronal Multichannel Polarimeter. In: Tomczyk, S., Zhang, J., Bastian, T. (eds) Coronal Magnetometry. Springer, New York, NY. https://doi.org/10.1007/978-1-4939-2038-9_11
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