Titlebook: Advances in Space Environment Research; Volume I A. C.-L. Chian,I. H. Cairns,Y. Yan Book 2003 Springer Science+Business Media Dordrecht 200

Opponent

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. The

NUDGE

Assignment

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

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’ (surp

Iniquitous

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

玩忽職守

Noctambulant

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

絆住

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

討厭

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