Education Success Story
Physics Researcher Develops Optical Constants for Use in Space Exploration and Earth Science


“[We were] looking for a broad mathematics library that also had an easy programming language such as Java. The Quick Start guide of the JMSL Numerical Library was very useful and made learning very easy. The chart routines and math routines are also very simple to find.”
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--Marian Harrison, Physics Student, Brigham Young University

QUICK FACTS
> Physics student determining optical constants in the field of Extreme Ultraviolet Optics for use on space probes and satellites
> JMSL Library used for advanced math routines, charting feature and easy programming

THE PROBLEM
In the Department of Physics and Astronomy at Brigham Young University (BYU), students and professors are working in the field of optics to answer big questions about earth and space.

To learn about the physical properties of stars, for example, or the materials that make up the earth, scientists have begun working in the Extreme Ultraviolet range of the electromagnetic spectrum. Compared to ultraviolet light, Extreme Ultraviolet is even more difficult to detect, but has the ability to help scientists understand gases at the center of stars and at the earth’s core.

To study objects using Extreme Ultraviolet wavelengths, scientists use mirrors to manipulate light at tiny wavelengths. An optics scientist’s goal is to create the smoothest mirror possible in order to see the various spectra in their purest form. A perfectly smooth surface on a mirror is impossible, but scientists are learning new ways to minimize and account for the “roughness”, creating a more accurate picture. The mirrors can be mounted on a space probe to monitor the stars or on a satellite to monitor the earth.

Marian Harrison, a student in the BYU Department of Physics and Astronomy is studying how new materials can minimize roughness on a mirror. A material called thorium dioxide is showing the most promise for Harrison and her colleagues. But even thorium dioxide can’t create a completely smooth surface. So Harrison has created a program that can account for the roughness on a mirror.

THE SOLUTION
Harrison’s professor had been looking for a broad mathematics library that also has an easy programming language. He found the JMSL™ Numerical Library for Java™ Applications. Harrison uses the JMSL Library on a Windows PC along with Eclipse, a Java development platform. She took advantage of the Quick Start feature in the JMSL Library: “The Quick Start guide was very useful. It made learning the JMSL Library language very easy. Chart routines and math routines are also very easy to find”, says Harrison.

Using the JMSL Library, Harrison simulated a perfectly smooth mirror and an ordinary mirror coated with thorium dioxide. Harrison used the chart class to easily create images of her random surfaces. She then modeled the radiation (EUV rays) reflecting off of the surface. For the models, she used the Random, Quadrature, Spline, and Fourier Transform math routines.

Scattering Surfaces


She would collect the reflection readings from 0 to 90 degrees across the surface of the mirror. At each degree, she would collect 1000 points. Her application compares reflection from the smooth surface data to the rough surface data to get an effective reflection coefficient for the thorium dioxide. The program could apply to any kind of material, which would help scientists explore other materials for minimizing mirror roughness. Harrison has presented her findings in a Society of Physics Students session of the annual summer meeting of the American Association of Physics Teachers.

RETURN ON INVESTMENT
Marian Harrison and her professor applaud the JMSL Library for its easy programming language and structure that makes it easy to find chart routines and math routines.

 

Industry
Education

Application
Developing Optical Constants

Product
JMSL Library



Students and professors in the Brigham Young University Department of Physics and Astronomy work hand in hand to conduct research in areas such as Extreme Ultraviolet Optics and Quantum Optics.

Key Benefits

> Quick application development
> Easy programming language
> Superior charting capabilities
   
   
   
   
 
   
 
 
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