太阳耀斑环——观测与理解 科学出版社 rb mobi 在线 下载 lit txt 网盘 pdf

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，高能电子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射线、光学和EUV辐射分析太阳耀斑回路，以及它们的辐射理论和电子加速/传输理论。结果关于非热电子的俯仰角各向异性对其影响的研究微波和硬X射线辐射、X射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。太阳物理学文献。这本书对研究生和研究人员很有用。在太阳和太空物理学中。

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

2.2.3 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

2.3 Effects of Electron Pitch-Angle Anisotropy

2.3.1 Parameters of Numerical Simulation

2.3.2 Pitch-Angle Distributions of Sinu Type

2.3.3 Effect of Pitch-Angle Distribution Shape: Gaussian

Loss-Cone

2.3.4 Effect of Pitch-Angle Distribution Shape: Beam-like

Distribution

2.3.5 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

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