'Transfer equation' presentation slideshows

Lecture 3 Radiative and Convective Energy Transport

Lecture 3 Radiative and Convective Energy Transport. Mechanisms of Energy Transport Radiative Transfer Equation Grey Atmospheres Convective Energy Transport Mixing Length Theory. The Sun. I. Energy Transport.

927 views • 67 slides

Lecture 3 Radiative and Convective Energy Transport

Lecture 3 Radiative and Convective Energy Transport. Mechanisms of Energy Transport Radiative Transfer Equation Grey Atmospheres Convective Energy Transport Mixing Length Theory. The Sun. I. Energy Transport.

970 views • 67 slides

Recent results from the SIMECA code and the VLTI observations

531 views • 41 slides

Radiation Transfer

395 views • 39 slides

Notes adapted from Prof. P. Lewis plewis@geog.ucl.ac.uk

GEOGG141/ GEOG3051 Principles & Practice of Remote Sensing (PPRS) Radiative Transfer Theory at o ptical wavelengths applied to vegetation canopies: part 2. Notes adapted from Prof. P. Lewis plewis@geog.ucl.ac.uk. Dr. Mathias (Mat) Disney UCL Geography Office: 113, Pearson Building

487 views • 38 slides

Transfer equation in general curvilinear coordinates

Transfer equation in general curvilinear coordinates. Juris Freimanis Ventspils International Radio Astronomy Centre, Ventspils University College; Institute of Mathematics and Information Technology, Liepaja University e-mail: jurisf@venta.lv. Expanding the Universe

472 views • 30 slides

Basic Definitions

Basic Definitions. Specific intensity/mean intensity Flux The K integral and radiation pressure Absorption coefficient/optical depth Emission coefficient The source function The transfer equation & examples Einstein coefficients. Specific Intensity/Mean Intensity.

351 views • 16 slides

Accelerated Lambda Iteration

Accelerated Lambda Iteration. Motivation. Complete Linearization provides a solution scheme, solving the radiation transfer , the statistical equilibrium and the radiative equilibrium simultaneously.

282 views • 14 slides

Accelerated Lambda Iteration

Accelerated Lambda Iteration. Motivation. Complete Linearization provides a solution scheme, solving the radiation transfer , the statistical equilibrium and the radiative equilibrium simultaneously.

142 views • 14 slides

267 views • 12 slides

Lecture 8: Stellar Atmosphere

Lecture 8: Stellar Atmosphere. 3. Radiative transfer. Solar abundances from absorption lines. From an analysis of spectral lines, the following are the most abundant elements in the solar photosphere. Emission coefficient.

127 views • 12 slides