Zobrazeno 1 - 10
of 933
pro vyhledávání: '"Thomas, R. J."'
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
Abbasi, R. U., Abu-Zayyad, T., Allen, M., Barcikowski, E., Belz, J. W., Bergman, D. R., Blake, S. A., Byrne, M., Cady, R., Cheon, B. G., Chiba, J., Chikawa, M., Fujii, T., Fukushima, M., Furlich, G., Goto, T., Hanlon, W., Hayashi, Y., Hayashida, N., Hibino, K., Honda, K., Ikeda, D., Inoue, N., Ishii, T., Ito, H., Ivanov, D., Jeong, S., Jui, C. C. H., Kadota, K., Kakimoto, F., Kalashev, O., Kasahara, K., Kawai, H., Kawakami, S., Kawata, K., Kido, E., Kim, H. B., Kim, J. H., Kishigami, S. S., Krehbiel, P. R., Kuzmin, V., Kwon, Y. J., Lan, J., LeVon, R., Lundquist, J. P., Machida, K., Martens, K., Matuyama, T., Matthews, J. N., Minamino, M., Mukai, K., Myers, I., Nagataki, S., Nakamura, R., Nakamura, T., Nonaka, T., Ogio, S., Ohnishi, M., Ohoka, H., Oki, K., Okuda, T., Ono, M., Onogi, R., Oshima, A., Ozawa, S., Park, I. H., Pshirkov, M. S., Remington, J., Rison, W., Rodeheffer, D., Rodriguez, D. C., Rubtsov, G., Ryu, D., Sagawa, H., Saito, K., Sakaki, N., Sakurai, N., Seki, T., Sekino, K., Shah, P. D., Shibata, F., Shibata, T., Shimodaira, H., Shin, B. K., Shin, H. S., Smith, J. D., Sokolsky, P., Springer, R. W., Stokes, B. T., Stroman, T. A., Takai, H., Takeda, M., Takeishi, R., Taketa, A., Takita, M., Tameda, Y., Tanaka, H., Tanaka, K., Tanaka, M., Thomas, R. J., Thomas, S. B., Thomson, G. B., Tinyakov, P., Tkachev, I., Tokuno, H., Tomida, T., Troitsky, S., Tsunesada, Y., Uchihori, Y., Udo, S., Urban, F., Vasiloff, G., Wong, T., Yamamoto, M., Yamane, R., Yamaoka, H., Yamazaki, K., Yang, J., Yashiro, K., Yoneda, Y., Yoshida, S., Yoshii, H., Zundel, Z.
Publikováno v:
J. Geophys. Res. Atmos., 123 (2018)
Bursts of gamma ray showers have been observed in coincidence with downward propagating negative leaders in lightning flashes by the Telescope Array Surface Detector (TASD). The TASD is a 700~square kilometer cosmic ray observatory located in southwe
Externí odkaz:
http://arxiv.org/abs/1705.06258
Autor:
Marisaldi, M., Østgaard, N., Mezentsev, A., Lang, T., Grove, J. E., Shy, D., Heymsfield, G. M., Krehbiel, P., Thomas, R. J., Stanley, M., Sarria, D., Schultz, C., Blakeslee, R., Quick, M. G., Christian, H., Adams, I., Kroodsma, R., Lehtinen, N., Ullaland, K., Yang, S.
Publikováno v:
Nature; Oct2024, Vol. 634 Issue 8032, p57-60, 4p
Publikováno v:
Journal of Horticultural Sciences, Vol 17, Iss 1 (2022)
Immature inflorescence with outer spathe length of 5.5 cm size collected from West Coast Tall cultivar of coconut was used as the explant and rachillae bits were inoculated in Y3 media supplemented with 2, 4-D (1 mg L-1). The cultures were incubated
Externí odkaz:
https://doaj.org/article/42ebdf2725ed42488239d66c5c6833ac
Autor:
Keenan, F. P., Milligan, R. O., Jess, D. B., Aggarwal, K. M., Mathioudakis, M., Thomas, R. J., Brosius, J. W., Davila, J. M.
Theoretical emission-line ratios involving Fe XI transitions in the 257-407 A wavelength range are derived using fully relativistic calculations of radiative rates and electron impact excitation cross sections. These are subsequently compared with bo
Externí odkaz:
http://arxiv.org/abs/1001.3627
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Fully relativistic calculations of radiative rates and electron impact excitation cross sections for Fe X are used to derive theoretical emission-line ratios involving transitions in the 174-366 A wavelength range. A comparison of these with solar ac
Externí odkaz:
http://arxiv.org/abs/0806.3354
Spectroscopic measurements of AR NOAA 10871, obtained with the Extreme Ultraviolet Normal Incidence Spectrograph (EUNIS) sounding rocket instrument on 2006 April 12, reveal velocity oscillations in the He II 303.8 Angstrom emission line formed at T ~
Externí odkaz:
http://arxiv.org/abs/0804.1629
Publikováno v:
Current Science, 2018 Mar 01. 114(5), 964-970.
Externí odkaz:
https://www.jstor.org/stable/26495188
Publikováno v:
Mon.Not.Roy.Astron.Soc.376:205-214,2007
Recent fully relativistic calculations of radiative rates and electron impact excitation cross sections for Fe {\sc xiii} are used to generate emission-line ratios involving 3s$^{2}$3p$^{2}$--3s3p$^{3}$ and 3s$^{2}$3p$^{2}$--3s$^{2}$3p3d transitions
Externí odkaz:
http://arxiv.org/abs/astro-ph/0612493