Where’s the Hidden Planet?
Don’t see it? We can.
With CODE V Beam Synthesis Propagation, you can too.
Go to www.opticalres.com/bsp to find out how.
CODE V’s Beam Synthesis
Propagation TM (BSP), developed for
NASA to detect Earth-sized planets
outside our solar system, delivers
groundbreaking accuracy and ease of
use for beam propagation analysis.
• Simplified setup. BSP’s
unprecedented Pre-Analysis feature
determines recommended settings
for accurate results, making it
the easiest-to-use beam propagation
tool on the market, and saving
countless hours in setup.
• Efficient, accurate answers.
BSP’s advanced and highly efficient
algorithms can produce more
accurate results more quickly than
any other commercially available
beam propagation tool.
• Comprehensive design support.
BSP is fully integrated with
CODE V, providing the most fully
featured optical design and analysis
environment available — for both
planet hunting and down-to-earth
applications.
Why compromise with another
beam propagation tool when you
can get the right answers more
easily with BSP?
BSP supports full-vector field propagation.
This decibel-scale plot shows the Z-component
of the focal plane intensity of a Ritchey-Chrétien
telescope for linearly polarized light.
Corporate Headquarters: 3280 East Foothill Boulevard, Pasadena, CA 91107-3103 (626) 795-9101
Fax (626) 795-0184 E-mail: info@opticalres.com Web: www.opticalres.com
Offices: Tucson, AZ | Westborough, MA
©2009 Optical Research Associates. CODE V is a registered trademark of Optical Research Associates.
Beam Synthesis Propagation is a trademark of Optical Research Associates.
