Zobrazeno 1 - 10
of 10
pro vyhledávání: '"Ji, Shuchen"'
Publikováno v:
Nature Communications; 11/25/2024, Vol. 15 Issue 1, p1-13, 13p
Millisecond radio spikes on long centimetre and short decimetre wavelengths and occurrence frequency
Publikováno v:
Astrophysics and Space Science. 190:33-41
High time-resolution data observed in two periods, respectively, by three frequencies (1.42, 2.84, and 3.67 GHz) or four frequencies (1.42, 2.00, 2.84, and 4.00 GHz) of fast sampling radiotelescopes were processed. Obtained were some significant resu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::281e1cc661a64807a2f32ad04683f235
https://doi.org/10.1007/bf00644564
https://doi.org/10.1007/bf00644564
Publikováno v:
ICMMT'98. 1998 International Conference on Microwave and Millimeter Wave Technology. Proceedings (Cat. No.98EX106).
Phoenix II microwave spectrometer of Yunnan Observatory was founded in 1994. It has been operating at four frequencies of 1.42, 2.13, 2.84 and 4.26 GHz with both time constant of one second and one millisecond. Therefore, the instrument has the capab
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::72a66d0edc637cadb99d562f73c16c91
https://doi.org/10.1109/icmmt.1998.768256
https://doi.org/10.1109/icmmt.1998.768256
Publikováno v:
ICMMT'98 1998 International Conference on Microwave & Millimeter Wave Technology Proceedings (Cat No98EX106); 1998, p185-188, 4p
Publikováno v:
Chinese Astronomy and Astrophysics. 12:152-158
A radio intensity measurement was performed with a radio telescope of 8.2cm wavelength when the track of total solar eclipse passed over Yunnan Observatory on Feb 16, 1980. Some preliminary results deduced from this observation are discussed. The cor
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::46a574c58ede4181143935f0f987c3f2
https://doi.org/10.1016/0275-1062(88)90011-2
https://doi.org/10.1016/0275-1062(88)90011-2
Publikováno v:
Chinese Astronomy and Astrophysics. 9:232-240
We construct a magnetic loop model for the slowly varying radio sources on the Sun based on the gyro-radiation mechanism and the radio data at 2.0, 3.2, 8.2 and 21 cm obtained during the total eclipse of 1980 Feb. 16. The model explains several detai
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a00df7bd574a18e79de75fe218ff6bb9
https://doi.org/10.1016/0275-1062(85)90044-x
https://doi.org/10.1016/0275-1062(85)90044-x
Autor:
M. Pick, Ji Shuchen
Publikováno v:
Vistas in Astronomy. 31:109-111
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::01a981dcacff5ac3b5fa631b301d17d7
https://doi.org/10.1016/0083-6656(88)90185-7
https://doi.org/10.1016/0083-6656(88)90185-7
Publikováno v:
Astrophysics and Space Science; May 1993, Vol. 203 Issue: 2 p241-246, 6p
Publikováno v:
Astrophysics and Space Science; February 1993, Vol. 200 Issue: 2 p239-250, 12p
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