Zobrazeno 1 - 5
of 5
pro vyhledávání: '"S. L. Freeland"'
Comparison of 30 THz impulsive burst time development to microwaves, H α , EUV, and GOES soft X-rays
Autor:
Pierre Kaufmann, D. P. Cabezas, S. L. Freeland, Marian Karlický, M. M. Cassiano, Rositsa Miteva, A. S. Kudaka, Stephen M. White, A. Kerdraon, R. Marcon, Gerard Trottet, Jean-Pierre Raulin, M. L. Luoni, L. O. T. Fernandes
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2016, 586, pp.A91. ⟨10.1051/0004-6361/201425520⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2016, 586, pp.A91. ⟨10.1051/0004-6361/201425520⟩
Astronomy and Astrophysics-A&A, 2016, 586, pp.A91. ⟨10.1051/0004-6361/201425520⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2016, 586, pp.A91. ⟨10.1051/0004-6361/201425520⟩
The recent discovery of impulsive solar burst emission in the 30 THz band is raising new interpretation challenges. One event associated with a GOES M2 class flare has been observed simultaneously in microwaves, H-alpha, EUV, and soft X-ray bands. Al
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b0ffc765ccf19ea64fd27655b06401ce
https://hal.science/hal-02460714
https://hal.science/hal-02460714
Autor:
C. G. Giménez de Castro, Adriana Valio, Jean-Pierre Raulin, S. L. Freeland, A. Marun, L. O. T. Fernandes, G. Fernandez, J. L. Aballay, A. S. Kudaka, R. Godoy, Stephen M. White, Pierre Kaufmann, R. Marcon, R. V. de Souza
Publikováno v:
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Ground- and space-based observations of solar flares from radio wavelengths to gamma-rays have produced considerable insights but raised several unsolved controversies. The last unexplored wavelength frontier for solar flares is in the range of submi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2c8cd7983a9bb74efb7d8addaf814264
http://arxiv.org/abs/1303.5894
http://arxiv.org/abs/1303.5894
Autor:
S. L. Freeland, K. Schenk, Christian Möstl, Christopher J. Davis, D. A. Biesecker, Charlie J. Farrugia, Jackie A. Davies, Charles Deehr, David F. Webb, Murray Dryer, G. Millward, C. A. de Koning, Dusan Odstrcil
Publikováno v:
Space Weather. 9
[1] The Earth-directed coronal mass ejection (CME) of 8 April 2010 provided an opportunity for space weather predictions from both established and developmental techniques to be made from near–real time data received from the SOHO and STEREO spacec
Publikováno v:
AIP Conference Proceedings.
With soft X-ray imaging we can study the entire coronal volume, except for cold inclusions such as prominences, as a function of time. This should allow us to observe the origins of coronal mass ejections. We report here an initial survey of the Yohk
Publikováno v:
The Astrophysical Journal. 470:629