: Explores the conditions required for a cosinusoidal object to result in a cosinusoidal image.
The width of the function in the space domain ($a$) is inversely proportional to the width of the spectrum in the frequency domain. : Explores the conditions required for a cosinusoidal
: Deepens comprehension of the optical self-imaging phenomenon (the Talbot Effect). : Explores the conditions required for a cosinusoidal
The solutions follow the exact structure of the third edition textbook: : Explores the conditions required for a cosinusoidal
by Joseph W. Goodman was compiled and copyrighted by the author himself. It is designed specifically for professors and teaching assistants to aid in the instruction of advanced undergraduate and graduate-level optical physics and engineering courses.