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The Observation of Radiofrequency Radiation
k Antenna Relationships 6
Electromagnetic Wave Propagation in
2 other sections not shown
absorption coefficient aerial atoms Aust Aust0 average bandwidth brightness temperature charge collisions components constant contribution corona corresponding Crab Nebula curl degree of polarization determined direction of propagation distribution effect electric vector electromagnetic field emission encounter encounter0 energy equation factor formula Fourier frequency function galactic gauss given gives gyrating electrons hence incident integral intensity interferometer interstellar Lorentz magnetic field medium motion neutral hydrogen number density observed obtained Oort optical depth optical thickness parallel plane plasma oscillations polarisation Poynting flux radial velocities radiant power radiation field RADIO ASTRONOMY RADIO ASTRONOMY Chapter ratio ray trajectories refractive index regions relation relatively uninhibited result sin2 Smerd solar solid angle spectral spectrum spin temperature synchrotron Synchrotron Radiation telescope tensor tion transverse uniform uninhibited propagation unit vave vhere vith wave wavelengths Westfold whence zero