Bright 30THz impulsive solar bursts
Impulsive 30THz continuum bursts have been recently observed in solar flares, utilizing small telescopes with a unique and relatively simple optical setup concept. The most intense burst was observed together with a GOES X2 class event on 27 October 2014, also detected at two subterahertz (sub-THz)...
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Blackwell Publishing Ltd
2015
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| LEADER | 13634caa a22012017a 4500 | ||
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| 001 | PAPER-24698 | ||
| 003 | AR-BaUEN | ||
| 005 | 20230518205636.0 | ||
| 008 | 190411s2015 xx ||||fo|||| 00| 0 eng|d | ||
| 024 | 7 | |2 scopus |a 2-s2.0-85027943720 | |
| 040 | |a Scopus |b spa |c AR-BaUEN |d AR-BaUEN | ||
| 100 | 1 | |a Kaufmann, P. | |
| 245 | 1 | 0 | |a Bright 30THz impulsive solar bursts |
| 260 | |b Blackwell Publishing Ltd |c 2015 | ||
| 270 | 1 | 0 | |m Kaufmann, P.; Center of Radio Astronomy and Astrophysics, Engineering School, Mackenzie Presbyterian UniversityBrazil; email: pierrekau@gmail.com |
| 506 | |2 openaire |e Política editorial | ||
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| 520 | 3 | |a Impulsive 30THz continuum bursts have been recently observed in solar flares, utilizing small telescopes with a unique and relatively simple optical setup concept. The most intense burst was observed together with a GOES X2 class event on 27 October 2014, also detected at two subterahertz (sub-THz) frequencies, Reuven Ramaty High Energy Solar Spectroscopic Imager X-rays and Solar Dynamics Observatory/Helioseismic and Magnetic Imager and EUV. It exhibits strikingly good correlation in time and in space with white-light flare emission. It is likely that this association may prove to be very common. All three 30THz events recently observed exhibited intense fluxes in the range of 10 4 solar flux units, considerably larger than those measured for the same events at microwave and submillimeter wavelengths. The 30THz burst emission might be part of the same spectral burst component found at sub-THz frequencies. The 30THz solar bursts open a promising new window for the study of flares at their origin. Key Points 30THz impulsive solar bursts THz solar flare spectral component THz and white-light flares ©2015. American Geophysical Union. All Rights Reserved. |l eng | |
| 593 | |a Center of Radio Astronomy and Astrophysics, Engineering School, Mackenzie Presbyterian UniversitySão Paulo, Brazil | ||
| 593 | |a Center of Semiconductor Components, State University of Campinas, Campinas, Brazil | ||
| 593 | |a Air Force Research Laboratories, Space Vehicles Dir., Albuquerque, New Mexico, United States | ||
| 593 | |a Gleb Wataghin Physics Institute, State University of Campinas, Campinas, Brazil | ||
| 593 | |a Bernard Lyot Solar Observatory, Campinas, Brazil | ||
| 593 | |a Observatorio Astronõmico Felix Aguilar, Universidad Nacional de San Juan, San Juan, Argentina | ||
| 593 | |a Instituto de Astronomia y Física Del Espacio, CONICET-Universidad de Buenos Aires, Buenos Aires, Argentina | ||
| 593 | |a Instituto de Ciencias Astronomicas, De la Tierra y Del Espacio, CONICET, San Juan, Argentina | ||
| 593 | |a Complejo Astronomico El Leoncito, CONICET, San Juan, Argentina | ||
| 690 | 1 | 0 | |a 30THZ SOLAR BURSTS |
| 690 | 1 | 0 | |a MID-IR SOLAR PHYSICS |
| 690 | 1 | 0 | |a SOLAR FLARES |
| 690 | 1 | 0 | |a THZ BURST EMISSION |
| 700 | 1 | |a White, S.M. | |
| 700 | 1 | |a Marcon, R. | |
| 700 | 1 | |a Kudaka, A.S. | |
| 700 | 1 | |a Cabezas, D.P. | |
| 700 | 1 | |a Cassiano, M.M. | |
| 700 | 1 | |a Francile, C. | |
| 700 | 1 | |a Fernandes, L.O.T. | |
| 700 | 1 | |a Hidalgo Ramirez, R.F. | |
| 700 | 1 | |a Luoni, M. | |
| 700 | 1 | |a Marun, A. | |
| 700 | 1 | |a Pereyra, P. | |
| 700 | 1 | |a De Souza, R.V. | |
| 773 | 0 | |d Blackwell Publishing Ltd, 2015 |g v. 120 |h pp. 4155-4163 |k n. 6 |p J. Geophys. Res. Space Phys. |x 21699380 |w (AR-BaUEN)CENRE-418 |t Journal of Geophysical Research: Space Physics | |
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