2. THERMISTOR
SENSOR PROTOTYPE
FOR WFIRST
PROGRAM
WFIRST temperature sensor employed a negative temperature coefficient
(NTC) thermistor
Additional circuitry, such as operational amplifiers, bipolar junction transistors,
were employed to stabilize and linearize the NTC thermistor voltage signal
A Raspberry Pi was programmed to emulate the operations of a computer
system the sensor would be operated by
These operations included coordination of an ADC with conversion of
resultant binary signal into decimal and hexadecimal form
I assisted in the construction of the prototype with trouble shooting and
addressment of technical issues related to circuit design
Also, I programmed the Raspberry Pi to coordinate ADC operation, read and
convert resultant data
Further assisted in the construction of a Thermal Vacuum Chamber and in
testing that ranged from -330° to 60° Fahrenheit
Performed in 2018
Part of internship for then
Harris, now L3Harris
WFIRST has since been
renamed Nancy Grace Roman
Space Telescope
4. UTILITY OF A DIFFRACTION BAND
While a beautiful display of optical principles, diffraction bands are very useful in characterizing optical
transducers
A diffraction grating was constructed with index cards to create a diffraction band
Central maximum is high in intensity, but subsequent bands decrease by decreasing amounts
By the eight and ninth bands the difference in intensity is very slight
Resolution was characterized by measuring change in resistance that occurred with the smallest intensity
change
The range of light intensity associated with a diffraction band allows for characterization of a photoresistors
full-scale-output
5. RESULTS
An approximation of the photoresistors response
to illuminance was able to be made
The smallest change in light intensity that
generated an observable change in resistance
was 0.04 Lux