Zobrazeno 1 - 10
of 158
pro vyhledávání: '"Fleishman, G."'
Autor:
Musset, S., Jol, P., Sankar, R., Alnahari, S., Kapsiak, C., Ostlund, E., Lasko, K., Glesener, L., Fortson, L., Fleishman, G. D., Panesar, N. K., Zhang, Y., Jeunon, M., Hurlburt, N.
Publikováno v:
A&A 688, A127 (2024)
Context. Solar coronal jets seen in EUV are ubiquitous on the Sun, have been found in and at the edges of active regions, at the boundaries of coronal holes, and in the quiet Sun. Jets have various shapes, sizes, brightness, velocities and duration i
Externí odkaz:
http://arxiv.org/abs/2309.14871
Strong coronal magnetic field, when present, manifests itself as bright microwave sources at high frequencies produced by gyroresonant (GR) emission mechanism in thermal coronal plasma. The highest frequency at which this emission is observed is prop
Externí odkaz:
http://arxiv.org/abs/2301.08922
Autor:
Lysenko, A. L., Ulanov, M. V., Kuznetsov, A. A., Fleishman, G. D., Frederiks, D. D., Kashapova, L. K., Sokolova, Z. Ya., Svinkin, D. S., Tsvetkova, A. E.
Publikováno v:
Astrophys. J. Supplement Series, 262 (2022) 32-39
We present a database of solar flares registered by the Konus-Wind instrument during more than 27 years of operation, from 1994 November to now (2022 June). The constantly updated database (hereafter KW-Sun) contains over 1000 events detected in the
Externí odkaz:
http://arxiv.org/abs/2209.07593
Autor:
Gibson, S. E., Malanushenko, A., de Toma, G., Tomczyk, S., Reeves, K., Tian, H., Yang, Z., Chen, B., Fleishman, G., Gary, D., Nita, G., Pillet, V. M., White, S., Bąk-Stęślicka, U., Dalmasse, K., Kucera, T., Rachmeler, L. A., Raouafi, N. E., Zhao, J.
Magnetism defines the complex and dynamic solar corona. Coronal mass ejections (CMEs) are thought to be caused by stresses, twists, and tangles in coronal magnetic fields that build up energy and ultimately erupt, hurling plasma into interplanetary s
Externí odkaz:
http://arxiv.org/abs/2012.09992
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
Kontar, E. P., Motorina, G. G., Jeffrey, N. L. S., Tsap, Y. T., Fleishman, G. D., Stepanov, A. V.
Publikováno v:
A&A 620, A95 (2018)
Observations of solar flares at sub-THz frequencies (mm and sub-mm wavelengths) over the last two decades often show a spectral component rising with frequency. Unlike a typical gyrosynchrotron spectrum decreasing with frequency, or a weak thermal co
Externí odkaz:
http://arxiv.org/abs/1810.03922
Publikováno v:
Solar Physics, 2017, Volume 292, Issue 9, article id. #137, 13 pp
The new generations of multiwavelength radioheliographs with high spatial resolution will employ microwave imaging spectropolarimetry to recover flare topology and plasma parameters in the flare sources and along the wave propagation paths. The recor
Externí odkaz:
http://arxiv.org/abs/1709.06252
Autor:
Shimojo, M., Bastian, T. S., Hales, A. S., White, S. M., Iwai, K., Hills, R. E., Hirota, A., Phillips, N. M., Sawada, T., Yagoubov, P., Siringo, G., Asayama, S., Sugimoto, M., Brajsa, R., Skokic, I., Barta, M., Kim, S., de Gregorio, I., Corder, S. A., Hudson, H. S., Wedemeyer, S., Gary, D. E., De Pontieu, B., Loukitcheva, M., Fleishman, G. D., Chen, B., Kobelski, A., Yan, Y.
Publikováno v:
Solar Physics Vol. 292: 87. (2017)
Observations of the Sun at millimeter and submillimeter wavelengths offer a unique probe into the structure, dynamics, and heating of the chromosphere; the structure of sunspots; the formation and eruption of prominences and filaments; and energetic
Externí odkaz:
http://arxiv.org/abs/1704.03236
Autor:
Wedemeyer, S., Fleck, B., Battaglia, M., Labrosse, N., Fleishman, G., Hudson, H., Antolin, P., Alissandrakis, C., Ayres, T., Ballester, J., Bastian, T., Black, J., Benz, A., Brajsa, R., Carlsson, M., Costa, J., DePontieu, B., Doyle, G., de Castro, G. Gimenez, Gunár, S., Harper, G., Jafarzadeh, S., Loukitcheva, M., Nakariakov, V., Oliver, R., Schmieder, B., Selhorst, C., Shimojo, M., Simões, P., Soler, R., Temmer, M., Tiwari, S., Van Doorsselaere, T., Veronig, A., White, S., Yagoubov, P., Zaqarashvili, T.
This document was created by the Solar Simulations for the Atacama Large Millimeter Observatory Network (SSALMON) in preparation of the first regular observations of the Sun with the Atacama Large Millimeter/submillimeter Array (ALMA), which are anti
Externí odkaz:
http://arxiv.org/abs/1601.00587
Autor:
Wedemeyer, S., Bastian, T., Brajsa, R., Hudson, H., Fleishman, G., Loukitcheva, M., Fleck, B., Kontar, E. P., De Pontieu, B., Yagoubov, P., Tiwari, S. K., Soler, R., Black, J. H., Antolin, P., Scullion, E., Gunar, S., Labrosse, N., Ludwig, H. -G., Benz, A. O., White, S. M., Hauschildt, P., Doyle, J. G., Nakariakov, V. M., Ayres, T., Heinzel, P., Karlicky, M., Van Doorsselaere, T., Gary, D., Alissandrakis, C. E., Nindos, A., Solanki, S. K., van der Voort, L. Rouppe, Shimojo, M., Kato, Y., Zaqarashvili, T., Perez, E., Selhorst, C. L., Barta, M.
The Atacama Large Millimeter/submillimeter Array (ALMA) is a new powerful tool for observing the Sun at high spatial, temporal, and spectral resolution. These capabilities can address a broad range of fundamental scientific questions in solar physics
Externí odkaz:
http://arxiv.org/abs/1504.06887