Zobrazeno 1 - 10
of 869
pro vyhledávání: '"Rimmelé, T."'
Autor:
Schad, T. A., Fehlmann, A., Dima, G. I., Kuhn, J. R., Scholl, I. F., Harrington, D., Rimmele, T., Tritschler, A., Paraschiv, A. R.
We report commissioning observations of the Si X 1430 nm solar coronal line observed coronagraphically with the Cryogenic Near-Infrared Spectropolarimeter (Cryo-NIRSP) at the National Science Foundation's Daniel K. Inouye Solar Telescope (DKIST). The
Externí odkaz:
http://arxiv.org/abs/2402.09632
Autor:
Kuridze, D., Uitenbroek, H., Wöger, F., Mathioudakis, M., Morgan, H., Campbell, R., Fischer, C., Cauzzi, G., Schad, T., Reardon, K., Santos, J. M. da Silva, Beck, C., Tritschler, A., Rimmele, T.
The strongly coupled hydrodynamic, magnetic, and radiation properties of the plasma in the solar chromosphere makes it a region of the Sun's atmosphere that is poorly understood. We use data obtained with the high-resolution Visible Broadband Imager
Externí odkaz:
http://arxiv.org/abs/2402.04545
Publikováno v:
Solar Physics, 2015, 290, 6, 1871
Long-exposure spectro-polarimetry in the near-infrared is a preferred method to measure the magnetic field and other physical properties of solar prominences. In the past, it has been very difficult to observe prominences in this way with sufficient
Externí odkaz:
http://arxiv.org/abs/1508.01826
Autor:
Bruder, N., Vaisse, C., Bechis, C., Bernard, L., Leone, M., Poirier, M., Vincent, A., Abdelkrim, N., Paugam, C., Lion, F., Montravers, P., Langeron, O., Raux, M., Baussier, M., Xu, K., Bart, F., Dagois, S., Plaud, B., Rabuel, C., Roland, E., Biais, M., Nouette-Gaulain, K., Cabart, A., Hanouz, J.L., Lambert, C., Godet, T., Thibault, S., Bouhemad, B., Chambade, E., Bouzat, P., Garot, M., Lebuffe, G., Lallemant, F., Lemery, C., Tavernier, B., de Jong, A., Jaber, S., Verzilli, D., Delannoy, M., Meistelman, C., Carles, M., Tran, L., Bertran, S., Cuvillon, P., Ripart, J., Simon-Pene, S., Boisson, M., Debaene, B., Beloeil, H., Godet, G., Collange, O., Mertes, P.M., Diemunsch, P., Joganah, D., Oehlkern, L., Baulieu, M., Beauchesne, B., Beraud, A.M., Berthier-Berrada, S., Bien, J.Y., Dupont, G., Gavory, J., Lambert, P., Lanoiselée, J., Zufferey, P., Ferré, F., Martin, C., Minville, V., Planté, B., Baffeleuf, B., Ben Abdelkarim, M., David, J.S., Incagnoli, P., Khaled, M., Laplace, M.C., Lefevre, M., Piriou, V., Aubrun, F., Cero, V., Delsuc, C., Faulcon, C., Meuret, P., Rimmelé, T., Truc, C., Molliex, Serge, Passot, Sylvie, Morel, Jerome, Futier, Emmanuel, Lefrant, Jean Yves, Constantin, Jean Michel, Le Manach, Yannick, Pereira, Bruno
Publikováno v:
In Anaesthesia Critical Care & Pain Medicine February 2019 38(1):15-23
We propose a method to derive the line-of-sight magnetic flux density from measurements in the chromospheric Ca II IR line at 854.2 nm. The method combines two well-understood techniques, the center-of-gravity and bisector methods, in a single hybrid
Externí odkaz:
http://arxiv.org/abs/0912.3467
We use joint observations obtained with the Hinode space observatory and the Interferometric Bidimensional Spectrometer (IBIS) installed at the DST of the NSO/SP to investigate the morphology and dynamics of (a) non-magnetic and (b) magnetic regions
Externí odkaz:
http://arxiv.org/abs/0912.3285
Publikováno v:
Astrophys.J.706:148-157,2009
The Interferometric Bidimensional Spectrometer (IBIS) installed at the Dunn Solar Telescope of the NSO/SP is used to investigate the morphology and dynamics of the lower chromosphere and the virtually non-magnetic fluctosphere below. The study addres
Externí odkaz:
http://arxiv.org/abs/0910.1381
Akademický článek
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Autor:
Sankarasubramanian, K., Rimmele, T.
Over the last few years, several interesting observations were obtained with the help of solar Adaptive Optics (AO). In this paper, few observations made using the solar AO are enlightened and briefly discussed. A list of disadvantages with the curre
Externí odkaz:
http://arxiv.org/abs/0801.3125
Autor:
Cauzzi, G., Reardon, K. P., Uitenbroek, H., Cavallini, F., Falchi, A., Falciani, R., Janssen, K., Rimmele, T., Vecchio, A., Woeger, F.
(Abridged) Aims: In this paper, we seek to establish the suitability of imaging spectroscopy performed in the Ca II 854.2 nm line as a means to investigate the solar chromosphere at high resolution. Methods: We utilize monochromatic images obtained w
Externí odkaz:
http://arxiv.org/abs/0709.2417