Zobrazeno 1 - 10
of 19
pro vyhledávání: '"Quanlin Fan"'
Autor:
Weiqun GAN, Quanlin FAN
Publikováno v:
Chinese Journal of Space Science. 42:608
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::dd7dd477a953f3ca27ac4b3619a9b60f
https://doi.org/10.11728/cjss2022.04.yg11
https://doi.org/10.11728/cjss2022.04.yg11
Publikováno v:
Advances in Space Research. 36:2363-2367
A so-called “ISF” prediction method for geomagnetic disturbances caused by solar wind storms blowing to the Earth is suggested. The method is based on a combined approach of solar activity, interplanetary scintillation (I) and geomagnetic disturb
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3c1db63f998d6992d8f9bbc73b0ef8e4
https://doi.org/10.1016/j.asr.2004.04.019
https://doi.org/10.1016/j.asr.2004.04.019
Publikováno v:
Physics of Plasmas. 11:5605-5614
Turbulent reconnection process in a one-dimensional current sheet is investigated by means of a two-dimensional compressible one-fluid magnetohydrodynamic simulation with spatially uniform, fixed resistivity. Turbulence is set up by adding to the she
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::5182fea42edce3c55a5a90c66b273e53
https://doi.org/10.1063/1.1806827
https://doi.org/10.1063/1.1806827
Publikováno v:
Physics of Plasmas. 10:4575-4578
The dynamics of small-scale explosive phenomena in the lower corona have been simulated by solving the compressible magnetohydrodynamic equations. Numerical results show that the magnetic reconnections in a long coronal current sheet consist of a ser
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::07d88e177824ede8732de97fcb1668eb
https://doi.org/10.1063/1.1620999
https://doi.org/10.1063/1.1620999
Publikováno v:
Space Science Reviews. 107:327-334
Recent progress in space weather research are briefly presented here from three aspects: establishment or improvement in observation systems, such as extra-soft X-ray detector and γ-ray detector onboard the spacecraft ‘Shen Zhou 2’, new solar ra
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::2727388ce0ef8f346f67c8a236794b65
https://doi.org/10.1023/a:1025525201204
https://doi.org/10.1023/a:1025525201204
Publikováno v:
Advances in Space Environment Research-Volume I ISBN: 9781402012785
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1b1c850733cd799576edf261c1f87286
https://doi.org/10.1007/978-94-007-1069-6_31
https://doi.org/10.1007/978-94-007-1069-6_31
Publikováno v:
Advances in Space Environment Research-Volume I ISBN: 9781402012785
It has been believed that three-dimensional, numerical, magnetohydrodynamic (MHD) modelling must play a crucial role in a seamless forecasting system. This system refers to space weather originating on the sun; propagation of disturbances through the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3444ca0fb1d05b0f57baf19dea2c5eda
https://doi.org/10.1007/978-94-007-1069-6_5
https://doi.org/10.1007/978-94-007-1069-6_5
Publikováno v:
Advances in Space Environment Research-Volume I ISBN: 9781402012785
Interplanetary magnetic reconnection(IMR) phenomena are explored based on the observational data with various time resolutions from Helios, IMP-8, ISEE3, Wind, etc. We discover that the observational evidence of the magnetic reconnection may be found
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::7ddc0e4c8bd4b21b60ffa6f2e013226e
https://doi.org/10.1007/978-94-007-1069-6_12
https://doi.org/10.1007/978-94-007-1069-6_12
Publikováno v:
Chinese Journal of Space Science. 26:161
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1b9383cb0d0c120f864a910df99aa744
https://doi.org/10.11728/cjss2006.03.161
https://doi.org/10.11728/cjss2006.03.161
Publikováno v:
Physics of Plasmas. 12:052901
In this paper, a possible two-step solar magnetic energy release process attributed to turbulent magnetic reconnection is investigated by magnetohydrodynamic simulation for the purpose of accounting for the closely associated observational features i
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e17abd728cb13d365a67046d0539bfd8
https://doi.org/10.1063/1.1862249
https://doi.org/10.1063/1.1862249