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Coronal dimming as a proxy for stellar coronal mass ejections

Published online by Cambridge University Press:  24 September 2020

M. Jin Open the ORCID record for M. Jin [Opens in a new window] ,
M. C. M. Cheung ,
M. L. DeRosa ,
N. V. Nitta ,
C. J. Schrijver Open the ORCID record for C. J. Schrijver [Opens in a new window] ,
K. France ,
A. Kowalski ,
J. P. Mason  and
R. Osten
M. Jin
Affiliation:
SETI Institute, 189 N Bernardo Ave suite 200, Mountain View, CA94043, USA email: [email protected] Lockheed Martin Solar and Astrophysics Lab (LMSAL), 3251 Hanover St., Bldg. 252, Palo Alto, CA94304, USA
M. C. M. Cheung
Affiliation:
Lockheed Martin Solar and Astrophysics Lab (LMSAL), 3251 Hanover St., Bldg. 252, Palo Alto, CA94304, USA Hansen Experimental Physics Laboratory, Stanford University, 452 Lomita Mall, Stanford, CA94305, USA
M. L. DeRosa
Affiliation:
Lockheed Martin Solar and Astrophysics Lab (LMSAL), 3251 Hanover St., Bldg. 252, Palo Alto, CA94304, USA
N. V. Nitta
Affiliation:
Lockheed Martin Solar and Astrophysics Lab (LMSAL), 3251 Hanover St., Bldg. 252, Palo Alto, CA94304, USA
C. J. Schrijver
Affiliation:
Lockheed Martin Solar and Astrophysics Lab (LMSAL), 3251 Hanover St., Bldg. 252, Palo Alto, CA94304, USA
K. France
Affiliation:
Laboratory for Atmospheric and Space Physics, University of Colorado at Boulder, 1234 Innovation Dr, Boulder, CO80303, USA
A. Kowalski
Affiliation:
Laboratory for Atmospheric and Space Physics, University of Colorado at Boulder, 1234 Innovation Dr, Boulder, CO80303, USA
J. P. Mason
Affiliation:
Laboratory for Atmospheric and Space Physics, University of Colorado at Boulder, 1234 Innovation Dr, Boulder, CO80303, USA
R. Osten
Affiliation:
Space Telescope Science Institute, 3700 San Martin Dr, Baltimore, MD21218, USA
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Abstract

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Solar coronal dimmings have been observed extensively in the past two decades and are believed to have close association with coronal mass ejections (CMEs). Recent study found that coronal dimming is the only signature that could differentiate powerful flares that have CMEs from those that do not. Therefore, dimming might be one of the best candidates to observe the stellar CMEs on distant Sun-like stars. In this study, we investigate the possibility of using coronal dimming as a proxy to diagnose stellar CMEs. By simulating a realistic solar CME event and corresponding coronal dimming using a global magnetohydrodynamics model (AWSoM: Alfvén-wave Solar Model), we first demonstrate the capability of the model to reproduce solar observations. We then extend the model for simulating stellar CMEs by modifying the input magnetic flux density as well as the initial magnetic energy of the CME flux rope. Our result suggests that with improved instrument sensitivity, it is possible to detect the coronal dimming signals induced by the stellar CMEs.

Keywords

magnetohydrodynamics (MHD)methods: numericalsolar windSun: coronaSun: coronal mass ejections (CMEs)
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 15 , Symposium S354: Solar and Stellar Magnetic Fields: Origins and Manifestations , June 2019 , pp. 426 - 432
Copyright
© International Astronomical Union 2020

References

Alvarado-Gómez, J. D., Drake, J. J., Cohen, O., et al. 2018, ApJ, 862, 93CrossRefGoogle Scholar
Attrill, G. D. R., Harra, L. K., van Driel-Gesztelyi, L., & Wills-Davey, M. J. 2010, Sol. Phys., 264, 119CrossRefGoogle Scholar
Aschwanden, M. J., Nitta, N. V., Wuelser, J.-P., et al. 2009, ApJ, 706, 376CrossRefGoogle Scholar
Cheng, J. X. & Qiu, J. 2016, ApJ, 825, 37CrossRefGoogle Scholar
Cohen, O., Attrill, G. D. R., Manchester, W. B., IV, & Wills-Davey, M. J. 2009, ApJ, 705, 587-602CrossRefGoogle Scholar
Craig, N., Abbott, M., Finley, D., et al. 1997, ApJS, 113, 131CrossRefGoogle Scholar
Delaboudinière, J.-P., Artzner, G. E., Brunaud, J., et al. 1995, Sol. Phys., 162, 291CrossRefGoogle Scholar
Dissauer, K., Veronig, A. M., Temmer, M., et al. 2018, ApJ, 855, 137CrossRefGoogle Scholar
Dissauer, K., Veronig, A. M., Temmer, M., et al. 2018, ApJ, 863, 169CrossRefGoogle Scholar
Downs, C., Roussev, I. I., van der Holst, B., Lugaz, N., & Sokolov, I. V. 2012, ApJ, 750, 134CrossRefGoogle Scholar
Downs, C., Török, T., Titov, V., et al. 2015, AAS/AGU Triennial Earth-Sun Summit, 1, 304.01Google Scholar
Gibson, S. E. & Low, B. C. 1998, ApJ, 493, 460CrossRefGoogle Scholar
Hansen, R. T., Garcia, C. J., Hansen, S. F., & Yasukawa, E. 1974, 86, 500CrossRefGoogle Scholar
Harra, L. K. & Sterling, A. C. 2001, ApJ, 561, L215CrossRefGoogle Scholar
Harra, L. K., Hara, H., Imada, S., et al. 2007, 59, S801CrossRefGoogle Scholar
Harra, L. K., Schrijver, C. J., Janvier, M., et al. 2016, Sol. Phys., 291, 1761CrossRefGoogle Scholar
Harrison, R. A., Bryans, P., Simnett, G. M., & Lyons, M. 2003, A&A, 400, 1071CrossRefGoogle Scholar
Hudson, H. S., Acton, L. W., & Freeland, S. L. 1996, ApJ, 470, 629CrossRefGoogle Scholar
Imada, S., Hara, H., Watanabe, T., et al. 2007, 59, S793CrossRefGoogle Scholar
Jin, M., Ding, M. D., Chen, P. F., Fang, C., & Imada, S. 2009, ApJ, 702, 27CrossRefGoogle Scholar
Jin, M., Schrijver, C. J., Cheung, M. C. M., et al. 2016, ApJ, 820, 16CrossRefGoogle Scholar
Jin, M., Manchester, W. B., van der Holst, B., et al. 2017a, ApJ, 834, 172CrossRefGoogle Scholar
Jin, M., Manchester, W. B., van der Holst, B., et al. 2017b, ApJ, 834, 173CrossRefGoogle Scholar
France, K., Arulanantham, N., Fossati, L., et al. 2018, ApJS, 239, 16CrossRefGoogle Scholar
France, K., Fleming, B. T., Drake, J. J., et al. 2019, Proc. SPIE 11118, UV, X-Ray, and Gamma-Ray Space Instrumentation for Astronomy XXI, 1111808Google Scholar
Krista, L. D. & Reinard, A. 2013, ApJ, 762, 91CrossRefGoogle Scholar
Krista, L. D. & Reinard, A. A. 2017, ApJ, 839, 50CrossRefGoogle Scholar
Lemen, J. R., Title, A. M., Akin, D. J., et al. 2012, Sol. Phys., 275, 17Google Scholar
Lugaz, N., Manchester, IV, W. B., & Gombosi, T. I. 2005, ApJ, 634, 651CrossRefGoogle Scholar
Manchester, W. B., Gombosi, T. I., Roussev, I., de Zeeuw, D. L., Sokolov, I. V., Powell, K. G., Tóth, G., & Opher, M. 2004a, Journal of Geophysical Research (Space Physics), 109, 1102CrossRefGoogle Scholar
Manchester, W. B., Gombosi, T. I., Roussev, I., Ridley, A., de Zeeuw, D. L., Sokolov, I. V., Powell, K. G., & Tóth, G. 2004b, Journal of Geophysical Research (Space Physics), 109, 2107Google Scholar
Manchester, IV, W. B., van der Holst, B., & Lavraud, B. 2014, Plasma Physics and Controlled Fusion, 56, 064006CrossRefGoogle Scholar
Mason, J. P., Woods, T. N., Caspi, A., Thompson, B. J., & Hock, R. A. 2014, ApJ, 789, 61CrossRefGoogle Scholar
Mason, J. P., Woods, T. N., Webb, D. F., et al. 2016, ApJ, 830, 20CrossRefGoogle Scholar
Oran, R., van der Holst, B., Landi, E., et al. 2013, ApJ, 778, 176CrossRefGoogle Scholar
Oran, R., Landi, E., van der Holst, B., et al. 2015, ApJ, 806, 55CrossRefGoogle Scholar
Pesnell, W. D., Thompson, B. J., & Chamberlin, P. C. 2012, Sol. Phys., 275, 3CrossRefGoogle Scholar
Reinard, A. A. & Biesecker, D. A. 2008, ApJ, 674, 576–585CrossRefGoogle Scholar
Rust, D. M. & Hildner, E. 1976, Sol. Phys., 48, 381CrossRefGoogle Scholar
Schrijver, C. J., Aulanier, G., Title, A. M., Pariat, E., & Delannée, C. 2011, ApJ, 738, 167CrossRefGoogle Scholar
Sokolov, I. V., van der Holst, B., Oran, R., et al. 2013, ApJ, 764, 23CrossRefGoogle Scholar
Sterling, A. C. & Hudson, H. S. 1997, ApJ, 491, L55CrossRefGoogle Scholar
Sterling, A. C., Hudson, H. S., Thompson, B. J., & Zarro, D. M. 2000, ApJ, 532, 628CrossRefGoogle Scholar
Tian, H., McIntosh, S. W., Xia, L., He, J., & Wang, X. 2012, ApJ, 748, 106CrossRefGoogle Scholar
Thompson, B. J., Plunkett, S. P., Gurman, J. B., et al. 1998, Geophys. Res. Lett., 25, 2465CrossRefGoogle Scholar
Thompson, B. J., Gurman, J. B., Neupert, W. M., et al. 1999, ApJ, 517, L151CrossRefGoogle Scholar
Thompson, B. J., Cliver, E. W., Nitta, N., Delannée, C., & Delaboudinière, J.-P. 2000, Geophys. Res. Lett., 27, 1431CrossRefGoogle Scholar
Tóth, G., et al. 2012, Journal of Computational Physics, 231, 870CrossRefGoogle Scholar
van der Holst, B., Sokolov, I. V., Meng, X., et al. 2014, ApJ, 782, 81CrossRefGoogle Scholar
Woods, T. N., Hock, R., Eparvier, F., et al. 2011, ApJ, 739, 59CrossRefGoogle Scholar
Woods, T. N., Eparvier, F. G., Hock, R., et al. 2012, Sol. Phys., 275, 115CrossRefGoogle Scholar
Zarro, D. M., Sterling, A. C., Thompson, B. J., Hudson, H. S., & Nitta, N. 1999, ApJ, 520, L139CrossRefGoogle Scholar
Zhukov, A. N. & Auchère, F. 2004, A&A, 427, 705CrossRefGoogle Scholar