Zobrazeno 1 - 10
of 9 287
pro vyhledávání: '"Imamura T"'
Publikováno v:
Patient Preference and Adherence, Vol Volume 18, Pp 91-92 (2024)
Naoya Kataoka, Teruhiko Imamura Second Department of Internal Medicine, University of Toyama, Toyama, JapanCorrespondence: Teruhiko Imamura, Second Department of Internal Medicine, University of Toyama, 2630 Sugitani Toyama, Toyama, 930-0194, Japan,
Externí odkaz:
https://doaj.org/article/309dc48b17644f2698fa48a646cd4ae4
Publikováno v:
Clinical Ophthalmology, Vol Volume 13, Pp 2445-2449 (2019)
Shumpei Obata,1 Tomoaki Higashiyama,1 Taku Imamura,1 Masashi Kakinoki,1 Takahide Yanagi,2 Yoshihiro Maruo,2 Masahito Ohji1 1Department of Ophthalmology, Shiga University of Medical Science, Otsu, Japan; 2Department of Pediatrics, Shiga University of
Externí odkaz:
https://doaj.org/article/d898a328897644628afeffa2d8aef362
Autor:
Jain, Richa N., Choudhary, R. K., Bhardwaj, Anil, Imamura, T., Sharma, Anshuman, Parikh, Umang M.
The solar inner corona is a region that plays a critical role in energizing the solar wind and propelling it to supersonic and supra-Alfvenic velocities. Despite its importance, this region remains poorly understood because of being least explored du
Externí odkaz:
http://arxiv.org/abs/2308.12596
Autor:
Peralta, J., Cidadão, A., Morrone, L., Foster, C., Bullock, M., Young, E. F., Garate-Lopez, I., Sánchez-Lavega, A., Horinouchi, T., Imamura, T., Kardasis, E., Yamazaki, A., Watanabe, S.
Publikováno v:
A&A 672, L2 (2023)
First identified in 2016 by JAXA's Akatsuki mission, the discontinuity/disruption is a recurrent wave observed to propagate during decades at the deeper clouds of Venus (47--56 km above the surface), while its absence at the clouds' top ($\sim$70 km)
Externí odkaz:
http://arxiv.org/abs/2302.04689
Publikováno v:
Nature Communications 11 (2020) 5720
Terrestrial exoplanets orbiting within or near their host stars' habitable zone are potentially apt for life. It has been proposed that time-series measurements of reflected starlight from such planets will reveal their rotational period, main surfac
Externí odkaz:
http://arxiv.org/abs/2011.09271
Autor:
Peralta, J., Navarro, T., Vun, C. W., Sánchez-Lavega, A., McGouldrick, K., Horinouchi, T., Imamura, T., Hueso, R., Boyd, J. P., Schubert, G., Kouyama, T., Satoh, T., Iwagami, N., Young, E. F., Bullock, M. A., Machado, P., Lee, Y. J., Limaye, S. S., Nakamura, M., Tellmann, S., Wesley, A., Miles, P.
Publikováno v:
Geophysical Research Letters, Volume 47, Issue 11, 16 June 2020, e2020GL087221
Planetary-scale waves are thought to play a role in powering the yet-unexplained atmospheric superrotation of Venus. Puzzlingly, while Kelvin, Rossby and stationary waves manifest at the upper clouds (65--70 km), no planetary-scale waves or stationar
Externí odkaz:
http://arxiv.org/abs/2005.13540
Global structure of thermal tides in the upper cloud layer of Venus revealed by LIR onboard Akatsuki
Autor:
Kouyama, T., Taguchi, M., Fukuhara, T., Imamura, T., Horinouchi, T., Sato, T. M., Murakami, S., Hashimoto, G. L., Lee, Y. J., Futaguchi, M., Yamada, T., Akiba, M., Satoh, T., Nakamura, M.
Longwave Infrared Camera (LIR) onboard Akatsuki first revealed the global structure of the thermal tides in the upper cloud layer of Venus. The data were acquired over three Venusian years, and the analysis was done over the areas from the equator to
Externí odkaz:
http://arxiv.org/abs/1905.08947
Autor:
Peralta, J., Sánchez-Lavega, A., Horinouchi, T., McGouldrick, K., Garate-Lopez, I., Young, E. F., Bullock, M. A., Lee, Y. J., Imamura, T., Satoh, T., Limaye, S. S.
Publikováno v:
Icarus (2019)
During the years 2016 to 2018, the instruments Akatsuki/IR2 (JAXA) and IRTF/SpeX (NASA) acquired a large set of images at 1.74, 2.26 and 2.32 {\mu}m to study the nightside mid-to-lower clouds (48-60 km) of Venus. Here we summarize the rich variety of
Externí odkaz:
http://arxiv.org/abs/1905.08913
Autor:
Peralta, J., Iwagami, N., Sánchez-Lavega, Lee, Y. J., Hueso, R., Narita, M., Imamura, T., Miles, P., Wesley, A., Kardasis, E., Takagi, S.
Publikováno v:
Geophysical Research Letters, 46, (2019)
The Venusian atmosphere is covered by clouds with super-rotating winds whose accelerating mechanism is still not well understood. The fastest winds, occurring at the cloud tops ($\sim$70 km height), have been studied for decades thanks to their visua
Externí odkaz:
http://arxiv.org/abs/1903.02883
Autor:
Horinouchi, T., Murakami, S., Satoh, T., Peralta, J., Ogohara, K., Kouyama, T., Imamura, T., Kashimura, H., Limaye, S. S., McGouldrick, K., Nakamura, M., Sato, T. M., Sugiyama, K., Takagi, M., Watanabe, S., Yamada, M., Yamazaki, A., Young, E. F.
Publikováno v:
Nature Geoscience, Vol. 10, (2017) doi:10.1038/ngeo3016
The Venusian atmosphere is in a state of superrotation where prevailing westward winds move much faster than the planet's rotation. Venus is covered with thick clouds that extend from about 45 to 70 km altitude, but thermal radiation emitted from the
Externí odkaz:
http://arxiv.org/abs/1709.02216