Zobrazeno 1 - 10
of 677
pro vyhledávání: '"Ghazaryan, S"'
Autor:
Zhang, H., Pilgram, J. J., Constantin, C. G., Rovige, L., Heuer, P. V., Ghazaryan, S., Kaloyan, M., Dorst, R. S., Schaeffer, D. B., Niemann, C.
We present the first two-dimensional (2D) optical Thomson scattering measurements of electron density and temperature in laser-produced plasmas. The novel instrument directly measures $n_e(x,y)$ and $T_e(x,y)$ in two dimensions over large spatial reg
Externí odkaz:
http://arxiv.org/abs/2305.07843
Autor:
Pilgram, J. J., Adams, M. B. P., Constantin, C. G., Heuer, P. V., Ghazaryan, S., Kaloyan, M., Dorst, R. S., Schaeffer, D. B., Tzeferacos, P., Niemann, C.
In this paper we present a high-repetition-rate experimental platform for examining the spatial structure and evolution of Biermann generated magnetic fields in laser-produced plasmas. We have extended the work of prior experiments, which spanned ove
Externí odkaz:
http://arxiv.org/abs/2111.02670
Autor:
Kaloyan, M., Ghazaryan, S., Constantin, C. G., Dorst, R. S., Heuer, P. V., Pilgram, J. J., Schaeffer, D. B., Niemann, C.
We present optical Thomson scattering measurements of electron density and temperature in a large-scale (~2 cm) exploding laser plasma produced by irradiating a solid target with a high energy (5-10 J) laser pulse at high repetition rate (1 Hz). The
Externí odkaz:
http://arxiv.org/abs/2105.12666
To enlarge our database of Chemically Peculiar (CP) stars, we compiled published data concerning the He-weak and He-rich stars observed by high-resolution spectroscopy techniques during last decades. Twenty He-weak and 28 He-rich stars have been adde
Externí odkaz:
http://arxiv.org/abs/1906.06984
This talk is devoted to the statistical analysis of the new catalogue of Chemically Peculiar stars compiled from papers, where chemical abundances of those stars were given. The catalogue contains chemical abundances and physical parameters of 428 st
Externí odkaz:
http://arxiv.org/abs/1812.04885
In this paper we present a new catalogue of Chemically Peculiar (CP) stars obtained by compiling publications in which abundances of metals are provided. Our catalogue includes 428 stars for which the data were obtained through spectroscopic observat
Externí odkaz:
http://arxiv.org/abs/1807.06902
Autor:
H1 collaboration, Andreev, V., Baghdasaryan, A., Begzsuren, K., Belousov, A., Bertone, V., Bolz, A., Boudry, V., Brandt, G., Brisson, V., Britzger, D., Buniatyan, A., Bylinkin, A., Bystritskaya, L., Campbell, A. J., Avila, K. B. Cantun, Cerny, K., Chekelian, V., Contreras, J. G., Cvach, J., Currie, J., Dainton, J. B., Daum, K., Diaconu, C., Dobre, M., Dodonov, V., Eckerlin, G., Egli, S., Elsen, E., Favart, L., Fedotov, A., Feltesse, J., Fleischer, M., Fomenko, A., Gabathuler, E., Gayler, J., Gehrmann, T., Ghazaryan, S., Goerlich, L., Gogitidze, N., Gouzevitch, M., Grab, C., Grebenyuk, A., Greenshaw, T., Grindhammer, G., Gwenlan, C., Haidt, D., Henderson, R. C. W., Hladky, J., Hoffmann, D., Horisberger, R., Hreus, T., Huber, F., Huss, A., Jacquet, M., Janssen, X., Jung, A. W., Jung, H., Kapichine, M., Katzy, J., Kiesling, C., Klein, M., Kleinwort, C., Kogler, R., Kostka, P., Kretzschmar, J., Krücker, D., Krüger, K., Landon, M. P. J., Lange, W., Laycock, P., Lebedev, A., Levonian, S., Lipka, K., List, B., List, J., Lobodzinski, B., Malinovski, E., Martyn, H. -U., Maxfield, S. J., Mehta, A., Meyer, A. B., Meyer, H., Meyer, J., Mikocki, S., Morozov, A., Müller, K., Naumann, Th., Newman, P. R., Niebuhr, C., Niehues, J., Nowak, G., Olsson, J. E., Ozerov, D., Pascaud, C., Patel, G. D., Perez, E., Petrukhin, A., Picuric, I., Pirumov, H., Pitzl, D., Plačakytė, R., Polifka, R., Rabbertz, K., Radescu, V., Raicevic, N., Ravdandorj, T., Reimer, P., Rizvi, E., Robmann, P., Roosen, R., Rostovtsev, A., Rotaru, M., Šálek, D., Sankey, D. P. C., Sauter, M., Sauvan, E., Schmitt, S., Schoeffel, L., Schöning, A., Sefkow, F., Shushkevich, S., Soloviev, Y., Sopicki, P., South, D., Spaskov, V., Specka, A., Steder, M., Stella, B., Straumann, U., Sutton, M. R., Sykora, T., Thompson, P. D., Traynor, D., Truöl, P., Tsakov, I., Tseepeldorj, B., Valkárová, A., Vallée, C., Van Mechelen, P., Vazdik, Y., Wegener, D., Wünsch, E., Žáček, J., Zhang, Z., Žlebčík, R., Zohrabyan, H., Zomer, F.
The strong coupling constant $\alpha_s(M_Z)$ is determined from inclusive jet and dijet cross sections in neutral-current deep-inelastic $ep$ scattering (DIS) measured at HERA by the H1 collaboration using next-to-next-to-leading order (NNLO) QCD pre
Externí odkaz:
http://arxiv.org/abs/1709.07251
Akademický článek
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Autor:
Morel, T., Briquet, M., Auvergne, M., Alecian, G., Ghazaryan, S., Niemczura, E., Fossati, L., Lehmann, H., Hubrig, S., Ulusoy, C., Damerdji, Y., Rainer, M., Poretti, E., Borsa, F., Scardia, M., Schmid, V. S., Van Winckel, H., De Smedt, K., Papics, P. I., Gameiro, J. F., Waelkens, C., Fagas, M., Kaminski, K., Dimitrov, W., Baglin, A., Michel, E., Dumortier, L., Fremat, Y., Hensberge, H., Jorissen, A., Van Eck, S.
The existence of pulsations in HgMn stars is still being debated. To provide the first unambiguous observational detection of pulsations in this class of chemically peculiar objects, the bright star HD 45975 was monitored for nearly two months by the
Externí odkaz:
http://arxiv.org/abs/1311.4370
Autor:
Chilingarian, A. A., Gharagyozyan, G. V., Ghazaryan, S. S., Hovsepyan, G. G., Mamidjanyan, E. A., Melkumyan, L. G., Sokhoyan, S. H.
Using the EAS size spectra measured with the MAKET ANI array on Mt. Aragats, Armenia (3200m a.s.l.) in the range of the shower size 10^5 - 10^7 for different angles-of-incidence, the EAS attenuation length has been determined applying different analy
Externí odkaz:
http://arxiv.org/abs/astro-ph/0002076