Engineering topics
Publications and source records attributed to Hansen, J. E..
Intensity and polarization for meteorological spherical and nonspherical particle size parameters, comparing exact Mie scattering and ray optics
Doubling method application to multiple scattering of polarized light, studying Venus visible disk reflection of sunlight
Polarization of sunlight multiply scattered by atmosphere and cloud particles of Venus from UV to IR
Polarized light multiple scattering in planetary atmospheres, applying extended doubling method to realistic simulations with allowance for radiation polarization and azimuth dependence
Terrestrial clouds near IR light scattering compared to reflectivity of water and ice particles, discussing Mie and multiple scattering
Near infrared light scattering by terrestrial clouds
Lorentz absorption line shape computations in radiation scattered by homogeneous planetary atmosphere compared with results for isotropic scattering by van de Hulst similarity relations
Ice clouds near IR spectral reflectivity dependence on particle size, noting application to planetary atmospheres
Multiple light scattering solutions accuracy by diffraction peak omission from cloud and haze analytic phase functions compared for optically thick and thin planetary atmospheres
Radiative transfer by doubling very thin layers in problem of diffuse reflection from plane-parallel atmosphere eliminates numerically solving transfer equation
Comparing calculated and observed reflectivity for ice and water clouds
Critique of paper on water crystal existence on Venus, presenting arguments against existence of clouds of micron sized ice crystals
Near infrared spectral reflectance and scattering in ice clouds
Near IR reflectivity of ice clouds compared to observation of Venus
Comments on ice particles as major scatterers of infrared radiation from Venus atmosphere
Doubling principle providing rapid and accurate results for problem of diffuse reflection from plane parallel atmosphere
Near infrared reflectivity of ice clouds computed and compared to observations of Venus
Light density and color in earth shadow during lunar eclipse