Summery:
Our experiment utilized a Geiger counter as well as several thermistors to measure the Temperature and radiation during the eclipse.

How to interpret:
time -> number of seconds sense the pi started up (we started at about t-30 before flight)
t0 -> External Control Temperature
t1 -> Internal Control Temperature
t2 -> Internal MLI temp
t3 -> Internal AMLI temp
pressure -> unused, our BMP was inaccurate
rad dynamic -> number of pulses from t<100
rad static -> number of pulses from t=500
rad static per min -> normalized number of pulses ((rad static / 500)*60)
pulses -> number of pulses sense last poll

The CSV files are in this format:
<time> <t0> <t0> <t0> <t0> <pressure> <rad dynamic> <rad static> <rad static per min> <#pulses>

Credits:
Professor Ryan Schrenk
Professor Liam Williams
Holy Negussie
Elijah Mister
Owen Coffee
Ryan Rich
Daniel Geer
Eddie Zhou
James Gross
Chris Pyatt
Taylor Fryer
Zoe Denito
Anastasia Ericson

Any Questions please email:
Daniel Geer - dgeer@captechu.edu