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Project HUSP: H umidity/ U V-c S ensor P ayload

Project HUSP: H umidity/ U V-c S ensor P ayload. Team Parro Presentation of Flight Results CSBF, Palestine, TX. Flight Positions. Josh Hignight – Project manager and software development

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Project HUSP: H umidity/ U V-c S ensor P ayload

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  1. Project HUSP:Humidity/UV-c Sensor Payload Team Parro Presentation of Flight Results CSBF, Palestine, TX Team Parro: Project HUSP

  2. Flight Positions Josh Hignight – Project manager and software development Jason Rollins – Responsible for electrical work including power consumption, sensor interfacing, electrical design, and balloon sat testing Matt VanKerhkove – Thermal design and acquisition of parts for thermal needs, as well as thermal testing Tim Butler – In charge of things dealing with constrution Team Parro: Project HUSP

  3. Hypothesis There is an expected rise in humidity at the ozone layer, believed to be caused by an increase in UV-c. Team Parro: Project HUSP

  4. Payload • Humidity sensor • Temperature sensor Team Parro: Project HUSP

  5. Science • Ozone absorbs UV between 200nm and 310nm • This breaks up the ozone from O3 → O2 + O • The O then forms with water to form two hydroxyl molecules O + H2O → 2HO • Each of these OH’s then form with methane, and other pollutants to form water. Team Parro: Project HUSP

  6. Problems • UV-c leads broke before reaching a sufficient altitude • HOBO powered up at 7:30 AM and then powered downed at 7:30:05 AM Team Parro: Project HUSP

  7. Results Team Parro: Project HUSP

  8. Temperature vs AltitudeHOBO 1 & HOBO 2 Team Parro: Project HUSP

  9. Relative Humidity vs AltitudeHOBO 1 & HOBO 2 Team Parro: Project HUSP

  10. Absolute vs AltitudeHOBO 1 & HOBO 2 Team Parro: Project HUSP

  11. Acknowledgements • Dr John Wefel & Dr Greg Guzik • LA-SPACE consortium • NASA & CSBF • Dr Lee Sawyer Team Parro: Project HUSP

  12. Questions? Team Parro: Project HUSP

  13. Team Parro: Project HUSP

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  15. Team Parro: Project HUSP

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