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pro vyhledávání: '"Drummond, R A"'
Akademický článek
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Autor:
Jerzykiewicz, M., Handler, G., Daszynska-Daszkiewicz, J., Pigulski, A., Poretti, E., Rodriguez, E., Amado, P. J., Kolaczkowski, Z., Uytterhoeven, K., Dorokhova, T. N., Dorokhov, N. I., Lorenz, D., Zsuffa, D., Kim, S. -L., Bourge, P. -O., Acke, B., De Ridder, J., Verhoelst, T., Drummond, R., Movchan, A. I., Lee, J. -A., Steslicki, M., Molenda-Zakowicz, J., Garrido, R., Kim, S. -H., Michalska, G., Paparo, M., Antoci, V., Aerts, C.
A multisite photometric campaign for the Beta Cephei and eclipsing variable 16 Lacertae is reported. 749 h of high-quality differential photoelectric Stromgren, Johnson and Geneva time-series photometry were obtained with ten telescopes during 185 ni
Externí odkaz:
http://arxiv.org/abs/1508.05250
Publikováno v:
IEEE Open Access Journal of Power and Energy, Vol 8, Pp 377-388 (2021)
Modeling the unintended common- and differential-mode (CM and DM) behavior of multi-converter power electronic-based systems can be a challenge. Chief among the issues is the need for detailed knowledge of the converter hardware to determine model pa
Externí odkaz:
https://doaj.org/article/ba59dd5703554acabb47a53002259d8a
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
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K zobrazení výsledku je třeba se přihlásit.
Publikováno v:
IEEE Open Access Journal of Power and Energy, Vol 7, Pp 163-172 (2020)
Modeling the common-mode behavior of power electronic systems can be a challenge. This research aims to simplify the process by developing a modeling approach based on Thévenin common-mode equivalent circuits. The Thévenin common-mode equivalent
Externí odkaz:
https://doaj.org/article/5ae2e27ef94340a5ad69053619278457
Autor:
Saesen, S., Pigulski, A., Carrier, F., Michalska, G., Aerts, C., De Ridder, J., Briquet, M., Handler, G., Kolaczkowski, Z., Acke, B., Bauwens, E., Beck, P. G., Blom, Y., Blommaert, J., Broeders, E., Cherix, M., Davignon, G., Debosscher, J., Degroote, P., Decin, L., Dehaes, S., De Meester, W., Deroo, P., Desmet, M., Drummond, R., Eggen, J. R., Fu, J., Gazeas, K., Gelven, G. A., Gielen, C., Huygen, R., Jiang, X., Kalomeni, B., Kim, S. -L., Kim, D. H., Kopacki, G., Kwon, J. -H., Ladjal, D., Lee, C. -U., Lee, Y. -J., Lefever, K., Leitner, A., Lenz, P., Liakos, A., Lorenz, D., Narwid, A., Niarchos, P., Oestensen, R., Poretti, E., Prins, S., Provencal, J., Antolin, E. Puga, Puschnig, J., Raskin, G., Reed, M. D., Reyniers, M., Schmidt, E., Schmitzberger, L., Spano, M., Steininger, B., Steslicki, M., Uytterhoeven, K., Vanautgaerden, J., Vandenbussche, B., Van Helshoecht, V., Vanhollebeke, E., Van Winckel, H., Verhoelst, T., Vuckovic, M., Waelkens, C., Wolf, G. W., Yakut, K., Zhang, C., Zima, W.
Publikováno v:
Astronomische Nachrichten 331, No. 9/10, 1080 - 1083 (2010)
As a result of the variability survey in Chi Persei and NGC6910, the number of Beta Cep stars that are members of these two open clusters is increased to twenty stars, nine in NGC6910 and eleven in Chi Persei. We compare pulsational properties, in pa
Externí odkaz:
http://arxiv.org/abs/1004.2853
Autor:
Saesen, S., Carrier, F., Pigulski, A., Aerts, C., Handler, G., Narwid, A., Fu, J. N., Zhang, C., Jiang, X. J., Vanautgaerden, J., Kopacki, G., Stȩślicki, M., Acke, B., Poretti, E., Uytterhoeven, K., Gielen, C., Østensen, R., De Meester, W., Reed, M. D., Kołaczkowski, Z., Michalska, G., Schmidt, E., Yakut, K., Leitner, A., Kalomeni, B., Cherix, M., Spano, M., Prins, S., Van Helshoecht, V., Zima, W., Huygen, R., Vandenbussche, B., Lenz, P., Ladjal, D., Antolín, E. Puga, Verhoelst, T., De Ridder, J., Niarchos, P., Liakos, A., Lorenz, D., Dehaes, S., Reyniers, M., Davignon, G., Kim, S. -L., Kim, D. H., Lee, Y. -J., Lee, C. -U., Kwon, J. -H., Broeders, E., Van Winckel, H., Vanhollebeke, E., Waelkens, C., Raskin, G., Blom, Y., Eggen, J. R., Degroote, P., Beck, P., Puschnig, J., Schmitzberger, L., Gelven, G. A., Steininger, B., Blommaert, J., Drummond, R., Briquet, M., Debosscher, J.
CONTEXT: Recent progress in the seismic interpretation of field beta Cep stars has resulted in improvements of the physics in the stellar structure and evolution models of massive stars. Further asteroseismic constraints can be obtained from studying
Externí odkaz:
http://arxiv.org/abs/1001.1116
Autor:
Cuypers, J., Aerts, C., De Cat, P., De Ridder, J., Goossens, K., Schoenaers, C., Uytterhoeven, K., Acke, B., Davignon, G., Debosscher, J., Decin, L., De Meester, W., Deroo, P., Drummond, R., Kolenberg, K., Lefever, K., Raskin, G., Reyniers, M., Saesen, S., Vandenbussche, B., Van Malderen, R., Verhoelst, T., Van Winckel, H., Waelkens, C.
Gamma Doradus stars are excellent targets for asteroseismology since the gravity modes present in these stars probe the deep stellar interiors. Mode identification will improve the knowledge of these stars considerably. A selected group of Gamma Dora
Externí odkaz:
http://arxiv.org/abs/0903.5213
Autor:
Samadi, R., Fialho, F., Costa, J. E. S., Drummond, R., Da Silva, L. Pinheiro, Baudin, F., Boumier, P., Jorda, L.
We present here the set of corrections that will be applied to the raw data of the CoRoT mission. The aim is to correct the data for instrumental and environmental perturbations as well as to optimize the duty-cycle, in order to reach the expected pe
Externí odkaz:
http://arxiv.org/abs/astro-ph/0703354