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First radio burst imaging observation from Mingantu Ultrawide Spectral Radioheliograph

Published online by Cambridge University Press:  09 September 2016

Yihua Yan ,
Linjie Chen ,
Sijie Yu  and
CSRH Team
Yihua Yan
Affiliation:
Key Laboratory of Solar Activity, Chinese Academy of Sciences, Beijing, 100012, China email: yyh@nao.cas.cn
Linjie Chen
Affiliation:
Key Laboratory of Solar Activity, Chinese Academy of Sciences, Beijing, 100012, China email: yyh@nao.cas.cn
Sijie Yu
Affiliation:
Key Laboratory of Solar Activity, Chinese Academy of Sciences, Beijing, 100012, China email: yyh@nao.cas.cn
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Abstract

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The Chinese Spectral Radioheliograph (CSRH) with two arrays in 400MHz-2GHz/2-15GHz ranges with 64/520 frequency channels have been established in Mingantu Observing Station, Inner Mongolia of China, since 2013 and is in test observations now. CSRH is renamed as Mingantu Ultrawide SpEctral Radioheliograph (MUSER) after its accomplishment. We introduce the progress and current status of MUSER. The first burst imaging results of MUSER is presented.

Keywords

Radioheliographsolar radio burstsflaresCMEscoronal magnetic field
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , Symposium S320: Solar and Stellar Flares and their Effects on Planets , August 2015 , pp. 427 - 435
Copyright
Copyright © International Astronomical Union 2016 

References

Aschwanden, M. J. & Benz, A. O. 1997, ApJ, 480, 825 CrossRefGoogle Scholar
Aschwanden, M. J. 2005, Physics of the Solar Corona, Springer, Berlin, 2005.Google Scholar
Bastian, T. S., Benz, A. O., & Gary, D. E. 1998, ARAA, 36, 131 CrossRefGoogle Scholar
Bastian, T. S. 2003, Proc. SPIE, 4853, 98 Google Scholar
Benz, A. O. 2009, § 4.1.2.8 in Landolt-Bornstein - Group VI Astronomy and Astrophysics Numerical Data and Functional Relationships in Science and Technology, vol. 4B, edited by Trumper, J.E., 1Google Scholar
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, Solar Phys. 162, 357.CrossRefGoogle Scholar
Chen, Bin, Bastian, T. S., White, S. M., Gary, D. E., Perley, R., Rupen, M., & Carlson, B. 2013, ApJL, 763, L21 CrossRefGoogle Scholar
Du, Jing; Yan, Yihua; Wang, Wei; Liu, Donghao, 2015, PASA, 32, 24 Google Scholar
Gary, D. E. 2003, J KAS, 36, 135 Google Scholar
Gary, D. E. & Keller, C. U. 2004, Solar and space weather radiophysics, Kluwer, Dordrecht, 2004 Google Scholar
Grechnev, V. V., Lesovoi, S. V., & Smolkov, G. Ya., et al. 2003, SolPhys, 216, 239 Google Scholar
Hudson, H. & Vilmer, N. 2007, Lect Notes Phys, 725, 81 Google Scholar
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, Solar Phys. 275, 17.CrossRefGoogle Scholar
Sha, Li, Yan, Yi-hua, Chen, Zhi-jun, Wang, Wei and Liu, Dong-hao, 2015a, RAA Google Scholar
Sha, Li, Yan, Yi Hua, Chen, Zhi Jun, Wang, Wei and Zhang, FuShun, 2015b, PASA Google Scholar
LIU Dong-hao, YAN Y-i hua, ZHAO An, WANG Wei, 2013, ACTA ELECTRONICA SINICA, 41, 570 Google Scholar
Nakajima, H., Nishio, M., & Enome, S., et al. 1994, Proc. IEEE, 82, 705 CrossRefGoogle Scholar
Nakariakov, V., Bisi, M. M., Browning, P. K., Maia, D., Kontar, E. P., Oberoi, D., Gallagher, P. T., Cairns, I. H., & Ratcliffe, H.: 2015, Advancing Astrophysics with the Square Kilometre Array (AASKA14), 169.CrossRefGoogle Scholar
Nakariakov, V. M., Kashapova, L. K. & Yan, Y.-H.: 2014, Research in Astronomy and Astrophysics 14, 001.CrossRefGoogle Scholar
Napier, J. P., Thompson, A. R., & Ekers, R. D. 1983, Proc. IEEE, 71, 1295 CrossRefGoogle Scholar
Olsson, R., Kildal, P. S., & Weinreb, S. 2006, IEEE Trans Ant Prop, 54, 368 Google Scholar
Pick, Monique, Vilmer, Nicole 2008, Astron Astrophys Rev, 16, 1 CrossRefGoogle Scholar
Pohjolainen, S., Karlický, M., van Driel-Gesztelyi, L. & Mandrini, C. H.: 2015, Solar Phys. 290, 1.CrossRefGoogle Scholar
Radioheliograph Group 1989, SolPhys, 120, 193 Google Scholar
Ramesh, R., Subramanian, K. R., Sundararajan, M. S., & Sastry, Ch. V. 1998, SolPhys, 181, 439 Google Scholar
Scherrer, P. H., Schou, J., Bush, R. I., Kosovichev, A. G., Bogart, R. S., Hoeksema, J. T., Liu, Y., Duvall, T. L., Zhao, J., Title, A. M., Schrijver, C. J., Tarbell, T. D. & Tomczyk, S.: 2012, Solar Phys. 275, 207.CrossRefGoogle Scholar
Wang, W., Yan, Y. H., Liu, D. H., Chen, Z. J., Su, C., Liu, F., Geng, L. H., Chen, L. J., and Du, J., 2013, PASJ, 65, A18 Google Scholar
Yan, Y. H., Wang, W., Liu, F., Geng, L. H., Chen, Z. J., & Zhang, J. 2013, in Solar and Astrophysical Dynamos and Magnetic Activity, Proc. IAU Symposium, vol. 294, edited by Kosovichev, A.G., de Gouveia Dal Pino, E.M., & Yan, Y., 489Google Scholar
Yan, Y. H., Zhang, J., Wang, W., Liu, F., Chen, Z. J., & Ji, G. S. 2009, Earth Moon Planet, 104, 97 CrossRefGoogle Scholar
Yan, Y. H., Zhang, J., & Huang, G., et al. 2004, Proc. 2004 Asia-Pacific Radio Science Conference, Qingdao, China, IEEE, Beijing, p. 391 CrossRefGoogle Scholar