Zobrazeno 1 - 7
of 7
pro vyhledávání: '"Huaan Lin"'
Autor:
Bo Chen, Fei Wei, Jie Liu, Huaan Lin, Wang Shijin, Jilong Peng, Ke‐Ping Qiu, Zhu Guangwu, Baoquan Li, Chang‐Sheng Ma, Yan Gong, Yu‐Hua Tang, Ling‐Gao Kong, Jing‐Hong Shao
Publikováno v:
Chinese Journal of Geophysics. 48:257-265
The Solar X-EUV imaging telescope (XEIT), which operates in the 4-100Awavelength bands and the 195A EUV emission line, is designed to monitor and predict solar activities resulting in variations of space weather. The XEIT is dedicated to space weathe
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::28187863199f69e46bc49dd9ed8796e0
https://doi.org/10.1002/cjg2.649
https://doi.org/10.1002/cjg2.649
Autor:
Huaan Lin, Long Xu, Shujuan Wang, Chengming Tan, Shijin Wang, Ruizhen Zhao, Yihua Yan, Qijun Fu
Publikováno v:
Solar Physics. 204:153-164
25 MHz–7.6 GHz global and detailed (fine structure – FS) radio spectra are presented, which were observed in the NOAA 9077 active region for the Bastille Day (14 July 2000) flare at 10:10–11:00 UT. Besides broadband radio bursts, high-resolutio
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ade3b35a999c99509ff7424624c81df2
https://doi.org/10.1023/a:1014278511984
https://doi.org/10.1023/a:1014278511984
Publikováno v:
SPIE Proceedings.
Solar Extreme Ultravoilet (EUV) irradiance is one of the most important energy input source for the upper atmosphere. It's responsible for the variation of the composition of upper atmosphere, vertical profile of the atmosphere density and ionosphere
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d4d1fab1ee38ac148434e59603e90b4d
https://doi.org/10.1117/12.807146
https://doi.org/10.1117/12.807146
Autor:
Huaan Lin, Danilo Freitas, Matilde T. D. Castanheira, Fei Wei, R.M.C. da Silva, C.A.N. Conde, N.F.C. Mendes, J.F.C.A. Veloso
Publikováno v:
IEEE Nuclear Science Symposium Conference Record, 2005.
The study of solar X-ray emissions can be very useful to predict and prevent the undesirable consequences of charged particles generated by solar flares on Earth, since charged particles take about 20 to 40 hours to reach Earth, while X-rays that are
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::5334d0db89f8a392ae59ef6fd5297fdd
https://doi.org/10.1109/nssmic.2005.1596294
https://doi.org/10.1109/nssmic.2005.1596294
Publikováno v:
Chinese Journal of Space Science. 26:370
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::9e414be986a602a679c04acf4f7a2fcf
https://doi.org/10.11728/cjss2006.05.370
https://doi.org/10.11728/cjss2006.05.370
Publikováno v:
Science in China Series G. 48:26
The space environment monitor (SEM) aboard FY-2 satellite consists of the high energy particle detector (HEPD) and the solar X-ray flux detector (SXFD). The SEM can provide real-time monitoring of flare and solar proton event for its operation at geo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c14a1694f737a5c9b175d52852415c1c
https://doi.org/10.1360/03yw0246
https://doi.org/10.1360/03yw0246
Autor:
Mendes, N.F.C., da Silva, R.M.C., Castanheira, M.T.D., Veloso, J.F.C.A., Freitas, D.S.A.P., Conde, C.A.N., Fei Wei, Huaan Lin
Publikováno v:
IEEE Nuclear Science Symposium Conference Record, 2005; 2005, p467-470, 4p