Zobrazeno 1 - 10
of 1 224
pro vyhledávání: '"Barrera L"'
Autor:
Stober J., Barrera L., Behler K., Bock A., Buhler A., Eixenberger H., Giannone L., Kasparek W., Maraschek M., Mlynek A., Monaco F., Poli E., Rapson C.J., Reich M., Schubert M., Treutterer W., Wagner D., Zohm H.
Publikováno v:
EPJ Web of Conferences, Vol 87, p 02017 (2015)
On ASDEX Upgrade a concept for real-time stabilization of NTMs has been realized and successfully applied to (3,2)- and (2,1)-NTMs. Since most of the work has meanwhile been published elsewhere, a short summary with the appropriate references is give
Externí odkaz:
https://doaj.org/article/b155ee302ae84b9ebf00163131dd2d94
Akademický článek
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Autor:
Alcántara-Mejía, V.A., Rodríguez-Mercado, J.J., Mateos-Nava, R.A., Álvarez-Barrera, L., Santiago-Osorio, E., Bonilla-González, E., Altamirano-Lozano, M.A.
Publikováno v:
In Toxicology Reports December 2024 13
Akademický článek
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Comet 67P/Churyumov-Gerasimenko was selected in 2003 as the new target of the Rosetta mission. It has since been the subject of a detailed campaign of observations to characterise its nucleus and activity. Here we present previously unpublished data
Externí odkaz:
http://arxiv.org/abs/1307.7978
Autor:
Rivinius, Th., Townsend, R. H. D., Kochukhov, O., Štefl, S., Baade, D., Barrera, L., Szeifert, Th.
The spectral and magnetic properties and variability of the B2Vnp emission-line magnetosphere star HR7355 were analyzed. The object rotates at almost 90% of the critical value, meaning it is a magnetic star for which oblateness and gravity darkening
Externí odkaz:
http://arxiv.org/abs/1211.0208
FN CMa is visually double with a separation of about 0.6arcsec. Sixty high-cadence VLT/UVES spectra permit the A and B components to be disentangled, as the relative contribution of each star to the total light entering the spectrograph fluctuates be
Externí odkaz:
http://arxiv.org/abs/1009.3512
The B2Vn star HR 7355 is found to be a He-rich magnetic star. Spectropolarimetric data were obtained with FORS1 at UT2 on Paranal observatory to measure the disk-averaged longitudinal magnetic field at various phases of the presumed 0.52 d cycle. A v
Externí odkaz:
http://arxiv.org/abs/1003.3601
Autor:
Solano, E. R., Lomas, P. J., Alper, B., Xu, G. S., Andrew, Y., Arnoux, G., Boboc, A., Barrera, L., Belo, P., Beurskens, M. N. A., Brix, M., Crombe, K., de la Luna, E., Devaux, S., Eich, T., Gerasimov, S., Giroud, C., Harting, D., Howell, D., Huber, A., Kocsis, G., Korotkov, A., Lopez-Fraguas, A., Nave, M. F. F., Rachlew, E., Rimini, F., Saarelma, S., Sirinelli, A., Thomsen, H., Zabeo, L., Zarzoso, D., contributors, JET EFDA
Publikováno v:
Phys. Rev. Lett. 104, 185003 (2010)
we report the identification of a localised current structure inside the JET plasma. It is a field aligned closed helical ribbon, carrying current in the same direction as the background current profile (co-current), rotating toroidally with the ion
Externí odkaz:
http://arxiv.org/abs/0910.5873
Photometric surveys of transNeptunian objects (TNOs) and Centaurs have suggested possible correlations between some orbital parameters and surface colors of classical objects, scattered disk objects (SDOs), and Centaurs. However, larger sample sizes
Externí odkaz:
http://arxiv.org/abs/0812.4525