PROPER: An Optical Propagation Library

Supporting MATLAB, Python, & IDL


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PROPER
is a set of routines to simulate the propagation of light through an optical system using Fourier transform algorithms (Fresnel, angular spectrum methods). It is currently available for IDL (Interactive Data Language), Matlab, and Python (2.7 & 3.x). It includes routines to create complex apertures, aberrated wavefronts, and deformable mirrors. It is especially useful for the simulation of high contrast imaging telescopes with coronagraphs. It is distributed as source code, is well documented with a detailed manual, and is relatively easy to use.


The current PROPER versions are:

IDL
3.2.7
15 June 2022
Matlab
3.2.7
15 June 2022
Python
3.2.7
15 June 2022


Changes/fixes in PROPER v3.2.7:

All versions:

Added option to PROP_DM to allow the user to specify their own actuator influence function.

Manual:

The manual is included with the code distribution and is also available here.

PROPER was developed by John Krist at the NASA Jet Propulsion Laboratory managed by the California Institute of Technology. The conversion to Matlab was done by Gary Gutt (JPL). The Python conversion was done by Navtej Saini with Nikta Amiri (JPL). Luis Marchen (JPL) performed function testing and some Python conversion, with William Schulze (JPL).

Please note that support for this software is provided on a time-available basis.  Due to US Government technology export control regulations, assistance from the author to non-US foreign nationals
without export licenses is limited to clarifications and bug fixes.

Download PROPER, get documentation, or submit support requests by hitting the Download button:
                 
                       Download PROPER Optical Propagation Library





Selected references to PROPER and projects that use PROPER

For citations

Krist, J., "PROPER: an optical propagation library for IDL", Proc. SPIE, 6675, 66700P (2007).
NOTE: When citing, please indicate that the new web site for PROPER is at proper-library.sourceforge.net

Verification and validation of PROPER results

Krist, J., et al., "Milestone 1 Results Report: Assessing the performance limits of internal coronagraphs through end-to-end modeling : A NASA TDEM study", exep.jpl.nasa.gov/technology (2012).

Sidick, E., et al., "HCIT contrast performance sensitivity studies: simulation versus experiment", Proc. SPIE, 8864 (2013).

End-to-end modeling of coronagraphic space telescopes


Krist, J., "End-to-end numerical modeling of AFTA coronagraphs", Proc. SPIE, 9143 (2014)
Krist, J., et al., "Assessing the performance limits of internal coronagraphs through end-to-end modeling", Proc. SPIE, 8864 (2013).
Krist, J., et al. "End-to-end simulations of different coronagraphic techniques", Proc. SPIE, 7440, 2009.

Uses of PROPER

Antichi, J., "FFREE: a Fresnel-FRee Experiment for EPICS, the EELT planets imager", Proc. SPIE, 7736 (2010).

Ingraham, P., et al. "High-Contrast Imaging Performance of a Tunable Filter for Space-Based Applications. II. Detection and Characterization Capabilities", PASP, 124 (2012).

Marois, C., et al., "A Fresnel propagation analysis of NFIRAOS/IRIS high-contrast exoplanet imaging capabilities", Proc. SPIE, 8447 (2012).

Marois, C., et al., "An end-to-end polychromatic Fresnel propagation model of GPI", Proc. SPIE, 7015 (2008).

Mawet, D., et al., "The Vector Vortex Coronagraph: sensitivity to central obscuration, low-order aberrations, chromaticism, and polarization", Proc. SPIE, 7739 (2010).


Mesa, D., et al., "Simulation of planet detection with the SPHERE integral field spectrograph", A&A, 529 (2011).


Pardini, T., et al., "The adaptive x-ray optic project at the Lawrence Livermore National Laboratory", J. Physics Conference Series, 493 (2014).

Thomas, S., "Amplitude variations on the ExAO testbed: Part II", Proc. SPIE, 6888 (2008).

Yaitskova, N., et al., "FOROS: Fresnel optical propagation code for SPHERE", Proc. SPIE, 7735 (2010).


Zimmerman, N., "Aperture mask interferometry with an integral field spectrograph", Proc. SPIE, 8445 (2012).

Updated 15 June 2022