Zobrazeno 1 - 10
of 19
pro vyhledávání: '"Mizuki YONEDA"'
Publikováno v:
Photogrammetric Engineering & Remote Sensing; 2024, Vol. 90 Issue 9, p537-551, 15p
Publikováno v:
Japanese Journal of JSCE. 79
Publikováno v:
Japanese Journal of JSCE. 79
Autor:
Yuzuru Yoshii, Yutaro Kitagawa, Masahiro Konishi, Takuya Yamashita, Kentaro Motohara, Mizuho Uchiyama, S. Koshida, Toshihiko Tanabe, Takuya Fujiyoshi, Takafumi Kamizuka, Shigeyuki Sako, Tomohiko Nakamura, Kentaro Asano, Ken Tateuchi, Mizuki Yoneda, Takashi Miyata
Publikováno v:
Publications of the Astronomical Society of Japan. 73:1638-1655
The formation of massive stars in dense and cold molecular clouds is a fundamental problem in star formation. In this work, we studied three compact massive star-forming regions, M8E, RAFGL 6366S, and IRAS 18317−0513, to investigate the environment
Publikováno v:
Astronomy & Astrophysics. 654:L7
Aims. Emission from helium atoms in Mercury’s exosphere at 58.4 nm was observed by the Mariner 10 spacecraft in the 1970s. This emission is due to resonant scattering of solar radiation. Since Mercury’s orbit is ellipsoidal, solar radiation and w
Autor:
Aljona Blöcker, Katherine de Kleer, Arielle Moullet, Peter Schilke, Lorenz Roth, Sven Thorwirth, E. Lellouch, G. Randall Gladstone, Nickolay Ivchenko, Hajime Kita, Álvaro Sánchez-Monge, Darrell F. Strobel, Mizuki Yoneda, Jérémie Boissier, Fuminori Tsuchiya, Kurt D. Retherford, Reina Hikida, Denis Grodent, Joachim Saur
Publikováno v:
Icarus. 350:113925
Io’s atmosphere is predominately SO 2 that is sustained by a combination of volcanic outgassing and sublimation. The loss from the atmosphere is the main mass source for Jupiter’s large magnetosphere. Numerous previous studies attributed various
Publikováno v:
Icarus. 261:31-33
Jupiter’s sodium nebula, which originates from Io’s volcanic gas, shows variations in its brightness due to the volcanic activity on Io. Imaging observation of D-line brightness in the sodium nebula was performed from 2013 through 2015 in a conju
Autor:
Takahiro Obara, Mizuki Yoneda, Jeff Kuhn, Svetlana Berdyugina, Hiromu Nakagawa, Takeshi Sakanoi, I. Scholl, Yasumasa Kasaba, Masato Kagitani, Shoichi Okano
Publikováno v:
SPIE Newsroom.
Autor:
T. M. Reynolds, J. H. Telting, Andrzej S. Baran, Daniel E. Reichart, Navpreet Kaur, Eda Sonbas, Stefano Ciprini, J. Lozano de Haro, T. Schweyer, Takeshi Sakanoi, WeiKang Zheng, Gary Poyner, Kiran S. Baliyan, Daniel B. Caton, Katsura Matsumoto, A. Escartin Pérez, A. W. Neely, J. Dalessio, Kozo Sadakane, Waldemar Ogloza, T. Pursimo, Jussi Harmanen, F. Garcia, V. H. Chavushyan, Byeong-Cheol Lee, Markus Mugrauer, B. Debski, S. Okano, Pauli Pihajoki, Kari Nilsson, Andrei Berdyugin, Andreas Kvammen, R. Naves Nogues, K. M. Ivarsen, H. Er, F. Alicavus, L. Tremosa Espasa, J. P. Moore, J. B. Haislip, Masato Kagitani, Elina Lindfors, L. O. Takalo, G. Hurst, R. Reinthal, V. Fallah Ramazani, Toma Tomov, Marek Drozdz, Kosmas Gazeas, Mauri Valtonen, Michal Siwak, John T. Stocke, J.-L. Salto González, William C. Keel, F. Campos, Arti Joshi, Pere Blay, J. Carrillo Gómez, J. R. Valdes, J. Valero Pérez, Iain A. Steele, Maheswar Gopinathan, M. Zejmo, Alexei V. Filippenko, M. R. Kidger, Gopal Bhatta, Dinko Dimitrov, Jan Strobl, Arti Goyal, Helen Jermak, Mizuki Yoneda, E. Gafton, F. Verrecchia, Stanisław Zoła, Judith L. Provencal, R. H. Nelson, M. Campas Torrent, J. Saario, Aaron P. LaCluyze, Vilppu Piirola, J. Krzesinski, James R. Webb, Ahmet Erdem, David Boyd, N. Karaman, F. Gómez Pinilla, Jeewan C. Pandey, A. Raj, Martin Jelínek, Achamveedu Gopakumar, René Hudec, F. C. Soldán Alfaro, S. Sadegi, M. Perri, R. Karjalainen, Sameer
Publikováno v:
Galaxies, Vol 4, Iss 4, p 41 (2016)
Galaxies; Volume 4; Issue 4; Pages: 41
Galaxies; Volume 4; Issue 4; Pages: 41
We analyse the light curve in the R band of the blazar OJ287, gathered during the 2015/2016 observing season. We did a search for quasi-periodic oscillations (QPOs) using several methods over a wide range of timescales. No statistically significant p
Autor:
Hiroaki Misawa, C. Tao, Bertrand Bonfond, Mizuki Yoneda, Masato Kagitani, S. Okano, Fuminori Tsuchiya
Publikováno v:
Geophysical Research Letters. 40:671-675
[1] Jupiter's sodium nebula showed an enhancement in late May through the beginning of June 2007. This means Io's volcanic activity and the magnetosphere's plasma content increased during this period. On the other hand, Jupiter's radio emission calle