Zobrazeno 1 - 10
of 226
pro vyhledávání: '"Charles, C. H."'
Ionospheric responses on the 21 August 2017 solar eclipse by using three-dimensional GNSS tomography
Publikováno v:
Earth, Planets and Space, Vol 74, Iss 1, Pp 1-12 (2022)
Abstract In this study, we have investigated the ionospheric responses on the August 2017 solar eclipse event by using a three-dimensional tomography algorithm with the ground-based GNSS (Global Navigation Satellite System) total electron content obs
Externí odkaz:
https://doaj.org/article/fe4cba9af4524330a65b0bc3e508f299
Akademický článek
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Publikováno v:
Terrestrial, Atmospheric and Oceanic Sciences, Vol 32, Iss 2, Pp 217-228 (2021)
The Naval Research Laboratory first-principles ionosphere model SAMI3/ESF is performed to study the interaction between the nighttime medium-scale traveling ionospheric disturbances (MSTIDs) and equatorial plasma bubbles (EPBs). The synthetic dynamo
Externí odkaz:
https://doaj.org/article/4de8a40429e84ba8a3eb2fd79bb41910
Autor:
Lee, Charles C. H.1 (AUTHOR) hau@mail.ihp.sinica.edu.tw
Publikováno v:
Global Intellectual History. Feb2023, p1-6. 6p.
Autor:
Yi Duann, Loren C. Chang, Chi-Yen Lin, Yueh-Chun Hsieh, Yun-Cheng Wen, Charles C. H. Lin, Jann-Yenq Liu
Publikováno v:
Atmosphere, Vol 14, Iss 1, p 74 (2022)
The conversion of airglow intensity to volume emission rate (VER) is a common method for studying the ionosphere, but the contribution of the intensity conversion process to the uncertainty in estimated electron or ion density is significant. The Abe
Externí odkaz:
https://doaj.org/article/78d47d480f584e64a9f0b41b680d6e37
Autor:
Jui, Charles C. H.
The Telescope Array (TA) is the largest ultrahigh energy (UHE) cosmic ray observatory in the northern hemisphere TA is a hybrid experiment with a unique combination of fluorescence detectors and a stand-alone surface array of scintillation counters.
Externí odkaz:
http://arxiv.org/abs/1110.0133
Akademický článek
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Autor:
Charles C. Ｈ. Lee
Publikováno v:
Global Intellectual History. :1-6
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e07b6e7d75bb469f9d4bdf07e4443473
https://doi.org/10.1080/23801883.2023.2183882
https://doi.org/10.1080/23801883.2023.2183882
Publikováno v:
Astrophys.J. 479 (1997) 547-559
We discuss in some detail the production of extremely high energy (EHE) neutrinos with energies above 10^18 eV. The most certain process for producing such neutrinos results from photopion production by EHE cosmic rays in the cosmic background photon
Externí odkaz:
http://arxiv.org/abs/astro-ph/9608186
Autor:
Rajesh, Panthalingal Krishanunni1, Lin, Charles C. H.1 charles@mail.ncku.edu.tw, Jia-Ting Lin1, Chi-Yen Lin2, Jia Yue3, Tomoko Matsuo4, Shih-Ping Chen1, Chia-Hung Chen1
Publikováno v:
Terrestrial, Atmospheric & Oceanic Sciences. Dec2021, Vol. 32 Issue 6, Part 1, p1-17. 17p.