Zobrazeno 1 - 10
of 371
pro vyhledávání: '"FUV instrument"'
Autor:
Frey, H. U.1 (AUTHOR) hfrey@ssl.berkeley.edu, Mende, S. B.1 (AUTHOR), Meier, R. R.2 (AUTHOR), Kamaci, U.3 (AUTHOR), Urco, J. M.3,4 (AUTHOR), Kamalabadi, F.3 (AUTHOR), England, S. L.5 (AUTHOR), Immel, T. J.1 (AUTHOR)
Publikováno v:
Space Science Reviews. Apr2023, Vol. 219 Issue 3, p1-21. 21p.
Akademický článek
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Autor:
Stephen B. Mende, Claire Poppett, Jerôme Loicq, Pascal Blain, Richard Desselle, Isabelle Domken, Yvan Stockman, Etienne Renotte, Lionel Clermont, Cathy Chou, Harald U. Frey, Kodi Rider, Christian Kintziger
Publikováno v:
SPIE Proceedings.
The optical calibration of the ICON-FUV instrument requires designing specific ground support equipment (GSE). The ICON-FUV instrument is a spectrographic imager that operates on two specific wavelengths in the UV (135.6 nm and 157 nm). All the opera
Conference
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Autor:
den Herder, Jan-Willem A., Takahashi, Tadayuki, Bautz, Marshall, Loicq, Jerome, Blain, Pascal, Kintziger, Christian, Desselle, Richard, Stockman, Yvan, Domken, Isabelle, Renotte, Etienne, Clermont, Lionel, Rider, Kodi, Chou, Cathy, Poppett, Claire, Frey, Harald U., Mende, Stephen B.
Publikováno v:
Proceedings of SPIE; July 2016, Vol. 9905 Issue: 1 p99052W-99052W-15, 9806164p
Autor:
H. Kil, Stephen B. Mende, Yongliang Zhang, Harald U. Frey, Thomas J. Immel, Larry J. Paxton, C.-I. Meng
Publikováno v:
Journal of Geophysical Research. 108
[1] Data from the IMAGE SI-13 instrument are used to study depletions in the OI 135.6 nm dayglow intensity due to two magnetic storms observed on 8 June and 15 July 2000. Results show that the SI-13 instrument is sensitive to changes in the 135.6 nm
Autor:
H. U. Frey, S. B. Mende, R. R. Meier, U. Kamaci, J. M. Urco, F. Kamalabadi, S. L. England, T. J. Immel
Publikováno v:
Space science reviews, vol 219, iss 3
The NASA Ionospheric Connection Explorer (ICON) was launched in October 2019 and has been observing the upper atmosphere and ionosphere to understand the sources of their strong variability, to understand the energy and momentum transfer, and to dete
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8d953db416498f9b32e98b1280ad12d6
https://escholarship.org/uc/item/7xh3k29g
https://escholarship.org/uc/item/7xh3k29g
Autor:
Zhen-Wei Han, Ke-Fei Song, Hong-Ji Zhang, Miao Yu, Ling-Ping He, Quan-Feng Guo, Xue Wang, Yang Liu, Bo Chen
Publikováno v:
Sensors, Vol 20, Iss 20, p 5958 (2020)
The radiation intensity of observed auroras in the far-ultraviolet (FUV) band varies dramatically with location for aerospace applications, requiring a photon counting imaging apparatus with a wide dynamic range. However, combining high spatial resol
Externí odkaz:
https://doaj.org/article/e8db10179c7d4f88be6c50e6e4e91883
Autor:
Mende, S. B.1 (AUTHOR) mende@ssl.berkeley.edu, Frey, H. U.1 (AUTHOR), England, S. L.2 (AUTHOR), Immel, T. J.1 (AUTHOR), Eastes, R. W.3 (AUTHOR)
Publikováno v:
Space Science Reviews. Dec2022, Vol. 218 Issue 8, p1-24. 24p.
Autor:
He Lingping, Song Kefei, Quan-Feng Guo, Xue Wang, Yang Liu, Miao Yu, Zhang Hongji, Zhen-Wei Han, Bo Chen
Publikováno v:
Sensors
Volume 20
Issue 20
Sensors, Vol 20, Iss 5958, p 5958 (2020)
Sensors (Basel, Switzerland)
Volume 20
Issue 20
Sensors, Vol 20, Iss 5958, p 5958 (2020)
Sensors (Basel, Switzerland)
The radiation intensity of observed auroras in the far-ultraviolet (FUV) band varies dramatically with location for aerospace applications, requiring a photon counting imaging apparatus with a wide dynamic range. However, combining high spatial resol