Zobrazeno 1 - 10
of 288
pro vyhledávání: '"Wöger F"'
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
Autor:
Campbell, Ryan J., Keys, P H., Mathioudakis, M., Woeger, F., Schad, T. A., Tritschler, A., de Wijn, A. G., Smitha, H. N., Beck, C. A., Christian, D J., Jess, D. B., Erdelyi, R.
We present the first quiet Sun spectropolarimetric observations obtained with the Visible SpectroPolarimeter (ViSP) at the $4-$m Daniel K. Inouye Solar Telescope (DKIST). We recorded observations in a wavelength range that includes the magnetically s
Externí odkaz:
http://arxiv.org/abs/2309.05836
Autor:
Santos, J. M. da Silva, Reardon, K., Cauzzi, G., Schad, T., Pillet, V. Martinez, Tritschler, A., Wöger, F., Hofmann, R., Stauffer, J., Uitenbroek, H.
Plage regions are patches of concentrated magnetic field in the Sun's atmosphere where hot coronal loops are rooted. While previous studies have shed light on the properties of plage magnetic fields in the photosphere, there are still challenges in m
Externí odkaz:
http://arxiv.org/abs/2308.10983
Autor:
de Wijn, A. G., Casini, R., Carlile, A., Lecinski, A. R., Sewell, S., Zmarzly, P., Eigenbrot, A. D., Beck, C., Wöger, F., Knölker, M.
Publikováno v:
Solar Physics, Volume 297, Issue 2, article id.22 (2022)
The Daniel K. Inouye Solar Telescope (DKIST) Visible Spectro-Polarimeter (ViSP) is a traditional slit-scanning spectrograph, with the ability to observe solar regions up to a $120\times78~\mathrm{arcsec}^2$ area. The design implements dual-beam polar
Externí odkaz:
http://arxiv.org/abs/2203.00117
Autor:
Anan T; National Solar Observatory, Makawao, HI, USA. tanan@nso.edu., Casini R; NSF NCAR High Altitude Observatory, Boulder, CO, USA., Uitenbroek H; National Solar Observatory, Boulder, CO, USA., Schad TA; National Solar Observatory, Makawao, HI, USA., Socas-Navarro H; Instituto de Astrofísica de Canarias, Vía Láctea S/N, La Laguna, Tenerife, Spain.; Departamento de Astrofísica, Universidad de La Laguna, Tenerife, Spain., Ichimoto K; College of Science and Engineering, Ritsumeikan University, Kusatsu, Shiga, Japan., Jaeggli SA; National Solar Observatory, Makawao, HI, USA., Tiwari SK; Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, USA.; Bay Area Environmental Research Institute, NASA Research Park, Moffett Field, CA, USA., Reep JW; Institute for Astronomy, University of Hawai'i at Mānoa, Pukalani, HI, USA., Katsukawa Y; National Astronomical Observatory of Japan, Mitaka, Tokyo, Japan., Asai A; Astronomical Observatory, Kyoto University, Sakyo, Kyoto, Japan., Qiu J; Department of Physics, Montana State University, Bozeman, MT, USA., Reardon KP; National Solar Observatory, Boulder, CO, USA.; Astrophysical and Planetary Sciences Department, University of Colorado, Boulder, CO, USA., Tritschler A; National Solar Observatory, Boulder, CO, USA., Wöger F; National Solar Observatory, Boulder, CO, USA., Rimmele TR; National Solar Observatory, Boulder, CO, USA.
Publikováno v:
Nature communications [Nat Commun] 2024 Oct 11; Vol. 15 (1), pp. 8811. Date of Electronic Publication: 2024 Oct 11.
Autor:
Shetye, J., Doyle, J. G., Scullion, E., Nelson, C. J., Kuridze, D., Henriques, V., Woeger, F., Ray, T.
Chromospheric observations taken at high cadence and high spatial resolution show a range of spicule like features, including Type I, Type II (as well as RBEs and RREs) and those which seem to appear within a few seconds, which if interpreted as flow
Externí odkaz:
http://arxiv.org/abs/1601.08087
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
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