Abstract
Motivated by dark coronal lanes in 284 Å extreme-ultraviolet (EUV) observations from the Extreme-ultraviolet Imaging Telescope on board the Solar and Heliospheric Observatory (SOHO/EIT), we construct and optimize an atmosphere model of the active region (AR) 8535 sunspot by adding a cool and dense component in the volume of plasma along open field lines determined using the potential-field source-surface (PFSS) extrapolation. Our model qualitatively reproduces the observed reduced microwave brightness temperature in the northern part of the sunspot in Very Large Array (VLA) observations from 13 May 1999 and provides a physical explanation for the coronal dark lanes. We propose the application of this method to other sunspots with such observed dark regions in the EUV or soft X-rays and with concurrent microwave observations to determine the significance of open field regions. The connection between open fields and the resulting plasma temperature and density change is of relevance for slow solar wind source investigations.
Similar content being viewed by others
References
Abbo, L., Ofman, L., Antiochos, S.K., Hansteen, V.H., Harra, L., Ko, Y.-K., Lapenta, G., Li, B., Riley, P., Strachan, L., von Steiger, R., Wang, Y.-M.: 2016, Space Sci. Rev. 201, 55. DOI.
Alissandrakis, C.E., Kundu, M.R.: 1982, Astrophys. J. 253, L49. DOI.
Alissandrakis, C.E., Kundu, M.R., Lantos, P.: 1980, Astron. Astrophys. 82, 30.
Alissandrakis, C.E., Bogod, V.M., Kaltman, T.I., Patsourakos, S., Peterova, N.G.: 2019, Solar Phys. 294, 23. DOI.
Altschuler, M.D., Newkirk, G.: 1969, Solar Phys. 9, 131. DOI.
Bale, S.D., Badman, S.T., Bonnell, J.W., Bowen, T.A., Burgess, D., Case, A.W., Cattell, C.A., Chandran, B.D.G., Chaston, C.C., Chen, C.H.K., Drake, J.F., Dudok de Wit, T., Eastwood, J.P., Ergun, R.E., Farrell, W.M., Fong, C., Goetz, K., Goldstein, M., Goodrich, K.A., Harvey, P.R., Horbury, T.S., Howes, G.G., Kasper, J.C., Kellogg, P.J., Klimchuk, J.A., Korreck, K.E., Krasnoselskikh, V.V., Krucker, S., Laker, R., Larson, D.E., MacDowall, R.J., Maksimovic, M., Malaspina, D.M., Martinez-Oliveros, J., McComas, D.J., Meyer-Vernet, N., Moncuquet, M., Mozer, F.S., Phan, T.D., Pulupa, M., Raouafi, N.E., Salem, C., Stansby, D., Stevens, M., Szabo, A., Velli, M., Woolley, T., Wygant, J.R.: 2019, Nature 576, 237. DOI.
Bezrukov, D.A., Ryabov, B.I., Shibasaki, K.: 2012, Balt. Astron. 21, 509. DOI.
Bezrukov, D., Ryabov, B., Peterova, N., Topchilo, N.: 2011, Latv. J. Phys. Tech. Sci. 48, 56. DOI.
Brosius, J.W., Landi, E.: 2005, Astrophys. J. 632, 1196. DOI.
Brosius, J.W., White, S.M.: 2004, Astrophys. J. 601, 546. DOI.
Brosius, J.W., Landi, E., Cook, J.W., Newmark, J.S., Gopalswamy, N., Lara, A.: 2002, Astrophys. J. 574, 453. DOI.
Delaboudinière, J.-P., Artzner, G.E., Brunaud, J., Gabriel, A.H., Hochedez, J.F., Millier, F., Song, X.Y., Au, B., Dere, K.P., Howard, R.A., Kreplin, R., Michels, D.J., Moses, J.D., Defise, J.M., Jamar, C., Rochus, P., Chauvineau, J.P., Marioge, J.P., Catura, R.C., Lemen, J.R., Shing, L., Stern, R.A., Gurman, J.B., Neupert, W.M., Maucherat, A., Clette, F., Cugnon, P., Van Dessel, E.L.: 1995, Solar Phys. 162, 291. DOI.
Dulk, G.A.: 1985, Annu. Rev. Astron. Astrophys. 23, 169. DOI.
Fleishman, G.D., Anfinogentov, S.A., Stupishin, A.G., Kuznetsov, A.A., Nita, G.M.: 2021, Astrophys. J. 909, 89. DOI.
Foukal, P.: 1981, In: Cram, L.E., Thomas, J.H. (eds.) The Physics of Sunspots: Proc. Sac. Peak Obs., 191.
Foukal, P.V., Huber, M.C.E., Noyes, R.W., Reeves, E.M., Schmahl, E.J., Timothy, J.G., Vernazza, J.E., Withbroe, G.L.: 1974, Astrophys. J. 193, L143. DOI.
Gary, D.E., Hurford, G.J.: 1994, Astrophys. J. 420, 903. DOI.
Gary, D.E., Keller, C.U. (eds.): 2004, Solar and Space Weather Radiophysics – Current Status and Future Developments, Kluwer, Dordrecht. DOI.
Gary, D.E., Chen, B., Dennis, B.R., Fleishman, G.D., Hurford, G.J., Krucker, S., McTiernan, J.M., Nita, G.M., Shih, A.Y., White, S.M., Yu, S.: 2018, Astrophys. J. 863, 83. DOI.
Gelfreikh, G.B.: 2004, In: Gary, D.E., Keller, C.U. (eds.) Solar and Space Weather Radiophysics – Current Status and Future Developments, Kluwer, Dordrecht, 115. DOI.
Gibson, S.E., Kucera, T.A., White, S.M., Dove, J.B., Fan, Y., Forland, B.C., Rachmeler, L.A., Downs, C., Reeves, K.K.: 2016, Front. Astron. Space Sci. 3, 8. DOI.
Kakinuma, T., Swarup, G.: 1962, Astrophys. J. 136, 975. DOI.
Lee, J.: 2007, Space Sci. Rev. 133, 73. DOI.
Lee, J., McClymont, A.N., Mikić, Z., White, S.M., Kundu, M.R.: 1998, Astrophys. J. 501, 853. DOI.
Lee, C.O., Luhmann, J.G., Hoeksema, J.T., Sun, X., Arge, C.N., de Pater, I.: 2011, Solar Phys. 269, 367. DOI.
Loukitcheva, M.A., Iwai, K., Solanki, S.K., White, S.M., Shimojo, M.: 2017, Astrophys. J. 850, 35. DOI.
Mok, Y., Mikić, Z., Lionello, R., Downs, C., Linker, J.A.: 2016, Astrophys. J. 817, 15. DOI.
Nindos, A., Alissandrakis, C.E., Gelfreikh, G.B., Kundu, M.R., Dere, K.P., Korzhavin, A.N., Bogod, V.M.: 1996, Solar Phys. 166, 55. DOI.
Nita, G.M., Viall, N.M., Klimchuk, J.A., Loukitcheva, M.A., Gary, D.E., Kuznetsov, A.A., Fleishman, G.D.: 2018, Astrophys. J. 853, 66. DOI.
Robinson, P.A., Melrose, D.B.: 1984, Aust. J. Phys. 37, 675. DOI.
Ryabov, B.I., Shibasaki, K.: 2016, Balt. Astron. 25, 225. DOI.
Ryabov, B.I., Vrublevskis, A.: 2020, Solar Phys. 295, 4. DOI.
Ryabov, B.I., Gary, D.E., Peterova, N.G., Shibasaki, K., Topchilo, N.A.: 2015, Solar Phys. 290, 21. DOI.
Schatten, K.H., Wilcox, J.M., Ness, N.F.: 1969, Solar Phys. 6, 442. DOI.
Scherrer, P.H., Bogart, R.S., Bush, R.I., Hoeksema, J.T., Kosovichev, A.G., Schou, J., Rosenberg, W., Springer, L., Tarbell, T.D., Title, A., Wolfson, C.J., Zayer, I. (MDI Engineering Team): 1995, Solar Phys. 162, 129. DOI.
Schrijver, C.J., DeRosa, M.L.: 2003, Solar Phys. 212, 165. DOI.
Strong, K.T., Alissandrakis, C.E., Kundu, M.R.: 1984, Astrophys. J. 277, 865. DOI.
Stupishin, A.G., Kaltman, T.I., Bogod, V.M., Yasnov, L.V.: 2018, Solar Phys. 293, 13. DOI.
Tun, S.D., Gary, D.E., Georgoulis, M.K.: 2011, Astrophys. J. 728, 1. DOI.
Vourlidas, A., Bastian, T.S., Aschwanden, M.J.: 1997, Astrophys. J. 489, 403. DOI.
White, S.M., Kundu, M.R., Gopalswamy, N.: 1991, Astrophys. J. 366, L43. DOI.
Zheleznyakov, V.V.: 1962, Soviet Astron. 6, 3.
Zlotnik, E.Y., Kundu, M.R., White, S.M.: 1996, Radiophys. Quantum Electron. 39, 255. DOI.
Zlotnik, E.Y., White, S.M., Kundu, M.R.: 1998, In: Alissandrakis, C.E., Schmieder, B. (eds.) Second Advances in Solar Physics Euroconference: Three-Dimensional Structure of Solar Active Regions, ASP Conf. Series 155, 135.
Acknowledgements
Magnetic field and EUV data are provided by the SOHO/MDI and EIT consortia. SOHO is a project of international cooperation between ESA and NASA. Karl G. Jansky Very Large Array (VLA) is a component of the National Radio Astronomy Observatory, which is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. A.V. is supported by the ERDF Postdoctoral Research Aid Project No. 1.1.1.2/16/1/001, Research Application No. 1.1.1.2/VIAA/1/16/079 “Understanding Solar Magnetic Atmosphere” (USMA). A.V. and B.I.R. are thankful to the Ventspils City Council for support.
Author information
Authors and Affiliations
Corresponding author
Ethics declarations
Disclosure of Potential Conflicts of Interest
The authors declare that they have no conflicts of interest.
Additional information
Publisher’s Note
Springer Nature remains neutral with regard to jurisdictional claims in published maps and institutional affiliations.
Rights and permissions
About this article
Cite this article
Vrublevskis, A., Ryabov, B.I. & White, S.M. Reduced Microwave Brightness Temperature in a Sunspot Atmosphere Due to Open Magnetic Fields. Sol Phys 296, 144 (2021). https://doi.org/10.1007/s11207-021-01891-5
Received:
Accepted:
Published:
DOI: https://doi.org/10.1007/s11207-021-01891-5