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诺森太阳耀斑环:观测与理解:observations and interpretations
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新春将至,本公司假期时间为:2025年1月23日至2025年2月7日。2月8日订单陆续发货,期间带来不便,敬请谅解!
1 Introduction
References
2 Theory of MW Emissions of Solar Flaring Loops
2.1 Observational Characteristics of Solar Microwave Emissions
2.1.1 Intensity, Polarization, and Spectrum of MW
Emission
2.1.2 Radiation Transfer
2.1.3 Thermal and Nonthermal (NT) Emission
2.2 Gyrosynchrotron (GS) Emission
2.2.1 Emissivity and Self-absorption Coefficient
2.2.2 Formation of GS Spectrum
2.. Influence of Magnetic Field Strength
2.2.4 Influence of Self-Absorption
2.2.5 Influence of High Plasma Density: Razin Effect
2.2.6 Razin Effect and Electron Power-Law Index
2.2.7 Plasma Density Increase on the Late Decay Phase..
2.2.8 Influence of Plasma Inhomogeneity on GS Spectrum
. Effects of Electron Pitch-Angle Anisotropy
..1 Parameters of Numerical Simulation
..2 Pitch-Angle Distributions of Sinu Type
.. Effect of Pitch-Angle Distribution Shape: Gaussian
Loss-Cone
..4 Effect of Pitch-Angle Distribution Shape: Beam-like
Distribution
..5 Discussion
2.4 Trapping and Transport Effects
2.4.1 Dependence on the Position of Acceleration/Injection
Site
2.4.2 Spectral an Polarization Responses to Specific Electron
Distributions
2.4.3 Diagnostic Potential
2.5 Effects of Other Parameters on GS Emission
2.5.1 Spectral Shape
2.5.2 Radio Flux Density
2.5.3 Spectral Index
2.5.4 Turnover Frequency
2.6 Numerical Codes for Fast GS Emission Calculations
References
3 Observations and Explanations of MW Emissions in Solar Flaring
Loops
3.1 Studies on Spatially Unresolvable Observations
3.1.1 Flattened Spectra in Solar Radio Bursts at Cm and Mm
Bands and Dynamics of Energetic Electrons in Flaring
Loops
3.1.2 Dynamics of Peak Frequency in Solar MW Bursts:
Self-absorption and Razin Effect
3.1.3 Optically Thin Emission, Power-Law Distribution of
Flares, and Occurrence Rate of Flares
3.2 Spatial Distribution of Microwave Brightness
3.2.1 Nonthermal MW Source at the Top of Extended Flaring
Guangli Huang、Victor F.Melnikov、
Haisheng Ji、Zongjun Ning编著的《太阳耀斑环--
观测与理解(英文版)(精)》提供了典型的太阳事件的
分析结果,统计分析,高能和磁场的诊断以及全
球行为太阳耀斑的循环,例如收缩和膨胀。特别注意
用微波、硬X线、光学和EUV辐分析太阳耀斑回路
,以及它们的辐理论和加速/传输理论。结果
关于非热的俯仰角各向异对其影响的研究微波
和硬X线辐、X线和微波的新光谱行为带,以及
与扩张环的收缩有关的结果,被广泛讨论。太理
学文献。这本书对和研究人员很有用。在太阳
和太空物理学中。
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