Infrared polarimetry and the galactic magnetic field. II. Improved models

Keyphrases

• ISM 100%
• Infrared Polarimetry 100%
• Random Component 100%
• Galactic Magnetic Fields 100%
• Optical Depth 66%
• Path Length 66%
• Interstellar Polarization 66%
• Constant Component 66%
• Magnetic Field 33%
• Field Lines 33%
• Alfvn Waves 33%
• Observed Trends 33%
• Magnetic Energy 33%
• Magnetic Field Strength 33%
• Energy Density 33%
• Contracting out 33%
• Line-of-sight 33%
• Equipartition 33%
• Position Angle 33%
• Dark Clouds 33%
• Molecular Clouds 33%
• Two-component Model 33%
• Random Phase 33%
• Wave Model 33%
• Cloud Formation 33%
• Decorrelation 33%
• Turbulent Energy 33%
• One-dimensional Compression 33%
• Cloudlet 33%
• Cloud Contracts 33%
• Low Filling Ratio 33%

Physics

• Polarimetry 100%
• Interstellar Magnetic Field 100%
• Magnetic Field 100%
• Position Angle 50%
• Dark Interstellar Clouds 50%
• Flux Density 50%
• Field Strength 50%
• Line of Sight 50%
• Molecular Clouds 50%