Challenges in coronagraph optical design
RA Chipman - Optical Modeling and Performance Predictions …, 2017 - spiedigitallibrary.org
The point spread function (PSF) for astronomical telescopes and instruments depends not
only on geometric aberrations and scalar wave diffraction, but also on the apodization and …
only on geometric aberrations and scalar wave diffraction, but also on the apodization and …
Challenges in coronagraph optical design
RA Chipman - Society of Photo-Optical Instrumentation …, 2017 - ui.adsabs.harvard.edu
The point spread function (PSF) for astronomical telescopes and instruments depends not
only on geometric aberrations and scalar wave diffraction, but also on the apodization and …
only on geometric aberrations and scalar wave diffraction, but also on the apodization and …
Challenges in coronagraph optical design
RA Chipman - 2017 - repository.arizona.edu
The point spread function (PSF) for astronomical telescopes and instruments depends not
only on geometric aberrations and scalar wave diffraction, but also on the apodization and …
only on geometric aberrations and scalar wave diffraction, but also on the apodization and …
Challenges in coronagraph optical design
R Chipman - Proc. of SPIE Vol - spiedigitallibrary.org
The point spread function (PSF) for astronomical telescopes and instruments depends not
only on geometric aberrations and scalar wave diffraction, but also on the apodization and …
only on geometric aberrations and scalar wave diffraction, but also on the apodization and …