Opponent 发表于 2025-3-23 11:01:25
Shang-Hong Lai,Vincent Lepetit,Yoichi Satoonent of the electric field penetrated into the magnetosphere are determined by the quarter square of the magnetic Reynolds number. In final, a dynamic model of the magnetospheric magnetic field is constructed. This model can describe the magnetosphere in the course of the severe magnetic storm. TheNUDGE 发表于 2025-3-23 16:30:07
http://reply.papertrans.cn/15/1499/149827/149827_12.pngAssignment 发表于 2025-3-23 18:45:16
Changjae Oh,Bumsub Ham,Kwanghoon Sohnf a more complete understanding of the physics involved? The paper examines the phenomenology of the events, briefly reviews the results of neural network prediction techniques and discusses the conjecture that the underlying physical processes might be related to self-organised criticality and turb打折 发表于 2025-3-24 00:37:34
Deep Supervised Hashing with Triplet Labels Important is the magnetic geometry determined by the magnetic feld lines lying on magnetic surfaces where also the flows are concentrated..Yet, transfer of methods and results obtained in tokamak research to solar coronal plasma dynamics immediately runs into severe problems with trans‘sonic’ (surpIniquitous 发表于 2025-3-24 02:58:39
Chu-Song Chen,Jiwen Lu,Kai-Kuang Mase maps and the subsurface wave-speed perturbation suffers from the poor vertical resolution of acoustic imaging. Recently an inversion method has been developed to invert the measured phase travel time perturbation to estimate the distribution of wave-speed perturbation based on the ray approximati玩忽职守 发表于 2025-3-24 10:22:00
http://reply.papertrans.cn/15/1499/149827/149827_16.pngNoctambulant 发表于 2025-3-24 13:18:54
Oliver Wasenmüller,Didier Strickerx temporal profiles during the flare process so as to understand the energy release and particle accelerations. It is proposed that the rope instability may have triggered the flare event, and reconnection may occur during this process. The drifting pulsation structure in the decimetric frequency ra绊住 发表于 2025-3-24 17:36:42
Ching-Hua Weng,Ying-Hsiu Lai,Shang-Hong Laid it is expected to consider non-constant-alpha force-free field model. As the recent result indicates that the plasma beta is sandwich-ed distributed above the solar surface (Gary, 2001), care must be taken in modeling the coronal field correctly. As the reconstruction of solar coronal magnetic fie奴才 发表于 2025-3-24 21:44:51
http://reply.papertrans.cn/15/1499/149827/149827_19.png讨厌 发表于 2025-3-25 02:30:05
Debluring Low-Resolution Imagesesent recent model simulations of the stormtime ring current energization due to the enhanced large-scale convection electric field, which show the transition from an asymmetric to a symmetric ring current during the storm and challenge the standard theories of (a) substorm-driven, and (b) symmetric