Zobrazeno 1 - 10
of 85
pro vyhledávání: '"Bloomfield, D. S."'
Autor:
Georgoulis, M. K., Bloomfield, D. S., Piana, M., Massone, A. M., Soldati, M., Gallagher, P. T., Pariat, E., Vilmer, N., Buchlin, E., Baudin, F., Csillaghy, A., Sathiapal, H., Jackson, D. R., Alingery, P., Benvenuto, F., Campi, C., Florios, K., Gontikakis, C., Guennou, C., Guerra, J. A., Kontogiannis, I., Latorre, V., Murray, S. A., Park, S. -H., von Stachelski, S., Torbica, A., Vischi, D., Worsfold, M.
Publikováno v:
Journal of Space Weather and Space Climate, 2021
The EU funded the FLARECAST project, that ran from Jan 2015 until Feb 2018. FLARECAST had a R2O focus, and introduced several innovations into the discipline of solar flare forecasting. FLARECAST innovations were: first, the treatment of hundreds of
Externí odkaz:
http://arxiv.org/abs/2105.05993
Autor:
Morton, R. J., Scullion, E., Bloomfield, D. S., McLaughlin, J. A., Regnier, S., McIntosh, S. W., Tomczyk, S., Young, P.
Determining the mechanisms responsible for the heating of the coronal plasma and maintaining and accelerating the solar wind are long standing goals in solar physics. There is a clear need to constrain the energy, mass and momentum flux through the s
Externí odkaz:
http://arxiv.org/abs/1611.06149
Autor:
Barnes, G., Leka, K. D., Schrijver, C. J., Colak, T., Qahwaji, R., Ashamari, O. W., Yuan, Y., Zhang, J., McAteer, R. T. J., Bloomfield, D. S., Higgins, P. A., Gallagher, P. T., Falconer, D. A., Georgoulis, M. K., Wheatland, M. S., Balch, C., Dunn, T., Wagner, E. L.
Solar flares produce radiation which can have an almost immediate effect on the near-Earth environment, making it crucial to forecast flares in order to mitigate their negative effects. The number of published approaches to flare forecasting using ph
Externí odkaz:
http://arxiv.org/abs/1608.06319
Context. The Sun is an active source of radio emission ranging from long duration radio bursts associated with solar flares and coronal mass ejections to more complex, short duration radio bursts such as solar S bursts, radio spikes and fibre bursts.
Externí odkaz:
http://arxiv.org/abs/1604.04788
Autor:
Byrne, J. P., Long, D. M., Gallagher, P. T., Bloomfield, D. S., Maloney, S. A., McAteer, R. T. J., Morgan, H., Habbal, S. R.
The study of solar eruptive events and associated phenomena is of great importance in the context of solar and heliophysics. Coronal mass ejections (CMEs) and coronal waves are energetic manifestations of the restructuring of the solar magnetic field
Externí odkaz:
http://arxiv.org/abs/1307.8155
Autor:
Seaton, D. B., Berghmans, D., Nicula, B., Halain, J. -P., De Groof, A., Thibert, T., Bloomfield, D. S., Raftery, C. L., Gallagher, P. T., Auchère, F., Defise, J. -M., D'Huys, E., Lecat, J. -H., Mazy, E., Rochus, P., Rossi, L., Schühle, U., Slemzin, V., Yalim, M. S., Zender, J.
The Sun Watcher with Active Pixels and Image Processing (SWAP) is an EUV solar telescope on board ESA's Project for Onboard Autonomy 2 (PROBA2) mission launched on 2 November 2009. SWAP has a spectral bandpass centered on 17.4 nm and provides images
Externí odkaz:
http://arxiv.org/abs/1208.4631
Autor:
Jess, D. B., McAteer, R. T. J., Mathioudakis, M., Keenan, F. P., Andic, A., Bloomfield, D. S.
High-cadence optical observations of an H-alpha blue-wing bright point near solar AR NOAA 10794 are presented. The data were obtained with the Dunn Solar Telescope at the National Solar Observatory/Sacramento Peak using a newly developed camera syste
Externí odkaz:
http://arxiv.org/abs/0709.2268
High-cadence, synchronized, multiwavelength optical observations of a solar active region (NOAA 10794) are presented. The data were obtained with the Dunn Solar Telescope at the National Solar Observatory/Sacramento Peak using a newly developed camer
Externí odkaz:
http://arxiv.org/abs/0707.2716
Publikováno v:
Astronomy and Astrophysics (2007) 469, 1155-1161
Aims: The primary objective of this study is to search for and identify wave modes within a sunspot penumbra. Methods: Infrared spectropolarimetric time series data are inverted using a model comprising two atmospheric components in each spatial pixe
Externí odkaz:
http://arxiv.org/abs/0705.0481