Zobrazeno 1 - 10
of 2 301
pro vyhledávání: '"Harrington D"'
Publikováno v:
Patient Preference and Adherence, Vol Volume 12, Pp 929-937 (2018)
Hyekyun Rhee,1 Mona N Wicks,2 Jennifer S Dolgoff,2 Tanzy M Love,3 Donald Harrington3 1University of Rochester School of Nursing, Rochester, NY, USA; 2College of Nursing, University of Tennessee Health Science Center, Memphis, TN, USA; 3Department of
Externí odkaz:
https://doaj.org/article/f1b2cd6ab9c84ccd879696810db40522
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:
Harrington, D. M., Sueoka, S. R.
Modern observatories and instruments require optics fabricated at larger sizes with more stringent performance requirements. The Daniel K. Inouye Solar Telescope will be the world's largest solar telescope at 4.0 m aperture delivering a 300 Watt beam
Externí odkaz:
http://arxiv.org/abs/1811.10321
Autor:
Bow, S.M.A., Goddard, A., Cope, G., Sharp, N., Schick, J., Woods, C., Jeffery, K., Harrington, D., Williams, S., Rodger, A.J., Finer, S., Fowler, T., Hopkins, S., Tunkel, S.A.
Publikováno v:
In Public Health August 2022 209:46-51
Autor:
Berdyugina, S. V., Harrington, D. M., Kuzmychov, O., Kuhn, J. R., Hallinan, G., Kowalski, A. F., Hawley, S. L.
We report the first direct detection of a strong, 5 kG magnetic field on the surface of an active brown dwarf. LSR J1835+3259 is an M8.5 dwarf exhibiting transient radio and optical emission bursts modulated by fast rotation. We have detected the sur
Externí odkaz:
http://arxiv.org/abs/1709.02861
Autor:
Wade, G. A., Neiner, C., Alecian, E., Grunhut, J. H., Petit, V., de Batz, B., Bohlender, D. A., Cohen, D. H., Henrichs, H. F., Kochukhov, O., Landstreet, J. D., Manset, N., Martins, F., Mathis, S., Oksala, M. E., Owocki, S. P., Rivinius, Th., Shultz, M. E., Sundqvist, J. O., Townsend, R. H. D., ud-Doula, A., Bouret, J. -C., Braithwaite, J., Briquet, M., Carciofi, A. C., David-Uraz, A., Folsom, C. P., Fullerton, A. W., Leroy, B., Marcolino, W. L. F., Moffat, A. F. J., Nazé, Y., Aurière, M., Bagnulo, S., Bailey, J. D., Barbá, R. H., Blazère, A., Böhm, T., Catala, C., Donati, J. -F., Ferrario, L., Harrington, D., Howarth, I. D., Ignace, R., Kaper, L., Lüftinger, T., Prinja, R., Vink, J. S., Weiss, W. W., Yakunin, I.
Publikováno v:
MNRAS, 456, 2-22 (2016)
The MiMeS project is a large-scale, high resolution, sensitive spectropolarimetric investigation of the magnetic properties of O and early B type stars. Initiated in 2008 and completed in 2013, the project was supported by 3 Large Program allocations
Externí odkaz:
http://arxiv.org/abs/1511.08425
We model the full-Stokes spectrum of the brown dwarf LSR J1835+3259 in the bands of the diatomic molecules CrH, TiO, and FeH in order to infer its magnetic properties. The models are then compared to the observational data obtained with the Low Resol
Externí odkaz:
http://arxiv.org/abs/1503.06964
Autor:
Coppinger, T., Milton, K., Murtagh, E., Harrington, D., Johansen, D., Seghers, J., Skovgaard, T., Chalkley, A.
Publikováno v:
In Public Health October 2020 187:150-156
We model the spectra of two brown dwarfs observed with the low resolution spectropolarimeter LRIS (Keck observatory) during several rotational phases in order to infer their magnetic properties. The spectra modeled include the intensity signal (Stoke
Externí odkaz:
http://arxiv.org/abs/1309.4617
Context: The technique of matching synthetic spectra computed with theoretical stellar atmosphere models to the observations is widely used in deriving fundamental parameters of massive stars. When applied to binaries, however, these models generally
Externí odkaz:
http://arxiv.org/abs/1307.1970