The 2D axisymmetric Approximation

For more info about our services contact : help@bestpfe.com

Table of contents

1. Introduction 
2. Wave Propagation and Resonances in Ionospheric Cavities 
2.1. The Resonant Cavity
2.1.1. Basic Description
2.1.2. General Formalism
2.2. Energy Sources and Global Circuit
3. Numerical Model for Ionospheric Planetary Cavities
3.1. Numerical Tool
3.1.1. The 2D axisymmetric Approximation
3.1.2. The 3D Model
3.1.3. Boundary and Continuity Conditions
3.1.4. Eigenfrequency Analysis
3.1.5. Time harmonic Propagation Analysis
3.1.6. Accuracy and Numerical Solvers
3.2. Cavity Parameterization
3.2.1. Parameter Description
3.2.2. Cavity Description
3.2.2.1. Venus
3.2.2.2. Earth
3.2.2.3. Mars
3.2.2.4. Jupiter
3.2.2.5. Io and Europa
3.2.2.6. Saturn
3.2.2.7. Uranus
3.2.2.8. Neptune
3.3. Results
4. Titan Electromagnetic Environment Characterization
4.1. The Cassini-Huygens Mission
4.2. The Permittivity, Waves and Altimetry Analyzer
4.2.1. Instrument Configuration
4.2.2. Relaxation Probe
4.2.3. Mutual Impedance Probe
4.2.4. Dipole Antenna
4.2.5. Acoustic Sensor
4.2.6. Radar
4.3. Experimental Results
4.3.1. Data Synopsis
4.3.2. Relaxation Data
4.3.3. Radar Data
4.3.4. Extremely Low Frequency Spectra
4.3.5. Very Low Frequency Spectra
4.3.6. Mutual Impedance Data
4.3.7. Lightning Data
4.3.8 Acoustic Spectra
4.4. PWA Data Analysis
5. Prospective Space Instrumentation and Missions
5.1. Planetary Surfaces Dielectric Properties Measurement
5.2. Dielectric Properties of Water, Ice, and Soils
5.2.1. Polarization Mechanisms and Effects
5.2.1.1. Polarization Theory
5.2.1.2. Frequency Effects
5.2.1.3. Temperature Effects
5.2.1.4. Composition Effects
5.2.2. Water Dielectric Properties
5.2.3. Ice Dielectric Properties
5.2.4. Water and Ice Dielectric Signatures in Soils
5.3. Subsurface Permittivity Probe
5.3.1. General Description
5.3.2. Electrodes
5.3.3. Electronics
5.3.4. Signal Processing
5.3.5. Operation
5.4. Laboratory Experiments
5.4.1. Experimental Setup and Instrument Calibration
5.4.2. Soil Analogues Testing
5.4.3. Results
5.4.3.1. Gravimetric Water Content
5.4.3.2. Stratigraphic Measurements
5.5. Probe Modelling
5.6. Future Missions
6. Conclusions
7. References