Plasma Astrophysics under Extreme Conditions

理论物理学的一个新分支--量子等离子体动力学(QPD)将应用于磁场和密度极端条件下的等离子体、等离子体-中微子效应和非线性辐射。 太阳耀斑中的磁能耗散归因于由电流细丝激发的大量耦合的、局部的、瞬变的、反常的阻性区域。该模型将包括Alfvenic锋面的非局部能量释放，磁零点的3D重联，以及电子的整体能化。 “”一致性吗？将量化相干辐射源，并将制定一个解释高度间歇性波增长的模型。

A new branch of theoretical physics, quantum plasmadynamics (QPD), will be applied to plasmas under extreme conditions of magnetic field and density, to plasma-neutrino effects and nonlinear radiation. Magnetic energy dissipation in solar flares will be attributed to a large number of coupled, local, transient, anomalously resistive regions excited by current filamentation. The model will include nonlocal energy release at Alfvenic fronts, 3D reconnection at magnetic nulls, and bulk energization of electrons. `Coherence? in sources of coherent emission will be quantified and a model for its interpretation for highly intermittent wave growth will be formulated.