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Leyte Normal UniversityTacloban City SORCE Prepared by:ArgieBalasbasMabag
SORCE(Solar Radiation and Climate Experiment)
Spacecraft: SORCE satelliteLaunch Vehicle:Pegasus XLLaunch Location: Kennedy Space Center, Cape Canaveral, FloridaLaunch Date: January 28, 2003Satellite Mass: 290 kg Power:  348 watts Communications: Redundant S-Band Transceivers Orbit: 645km, 40° inclinationMission Life: 5-year (6-year goal)
Objectives: 1. Make accurate measurements with high precision of total solar irradiance, connect them to previous TSI measurements, and continue this long-term climate record. Provide TSI with an accuracy of 0.01% (100 parts per million) based on SI units and with a long-term repeatability of 0.001%/yr.
Objectives: 2. Make daily measurements of the solar ultraviolet irradiance from 120 to 300 nm, with a spectral resolution of 1 nm. Achieve this spectral irradiance measurement with an accuracy of better than 5%, and with a long-term repeatability of 0.5%/yr. Use the solar/stellar comparison technique to relate the solar irradiance to the ensemble average flux from a number of bright, early-type stars (same stars used by the UARS SOLSTICE program)
Objectives: 3. Make the first measurements of the visible and near IR solar irradiance with sufficient precision for future climate studies. Obtain daily measurements of solar spectral irradiance between 0.3 and 2 µm with a spectral resolution of at least 1/30, an accuracy of 0.03%, and a long-term repeatability of better than 0.01%/yr.
Objectives: 4. Improve the understanding of how and why solar irradiance varies, estimate past and future solar behavior, and investigate climate responses.
Team Edward Chang SORCE Project Manager Robert CahalanSORCE Project Scientist
Team Doug Rabin SORCE Deputy Project Scientist  Don Anderson NASA Headquarters
Team Thomas SparnProgram Manager Brian BoyleSystems Engineering, Instrument Integration and Test, Mission Analysis, and Instrument Operations Manager 
Team Vanessa George Research CoordinatorLASP(Laboratory for Atmospheric and Space Physics) Ken GriestPlanning/Scheduling Engineer 
Team Barry Knapp Ground S/W Engineer/Analyst, LASP   (Laboratory for Atmospheric and Space Physics) Richard KohnertChief Systems Engineer  
Team Doug Lindholm Ground S/W Engineer/AnalystLASP (Laboratory for Atmospheric and Space Physics) Deb McCabe Flight Director,
Team Randy Meisner Ground S/W Engineer / Analyst  Chris PankratzScience Operations ManagerLASP (Laboratory for Atmospheric and Space Physics)  
Team Sean Ryan  Mission Operations Manager,  LASP (Laboratory for Atmospheric and Space Physics)  Ann Windnagel Ground S/W Engineer/Analyst LASP (Laboratory for Atmospheric and Space Physics)  
Agencies NASA Goddard Space Flight Center University of Colorado at Boulder
Agencies Orbital Sciences Corporation

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Sorce

  • 1. Leyte Normal UniversityTacloban City SORCE Prepared by:ArgieBalasbasMabag
  • 2. SORCE(Solar Radiation and Climate Experiment)
  • 3. Spacecraft: SORCE satelliteLaunch Vehicle:Pegasus XLLaunch Location: Kennedy Space Center, Cape Canaveral, FloridaLaunch Date: January 28, 2003Satellite Mass: 290 kg Power: 348 watts Communications: Redundant S-Band Transceivers Orbit: 645km, 40° inclinationMission Life: 5-year (6-year goal)
  • 4. Objectives: 1. Make accurate measurements with high precision of total solar irradiance, connect them to previous TSI measurements, and continue this long-term climate record. Provide TSI with an accuracy of 0.01% (100 parts per million) based on SI units and with a long-term repeatability of 0.001%/yr.
  • 5. Objectives: 2. Make daily measurements of the solar ultraviolet irradiance from 120 to 300 nm, with a spectral resolution of 1 nm. Achieve this spectral irradiance measurement with an accuracy of better than 5%, and with a long-term repeatability of 0.5%/yr. Use the solar/stellar comparison technique to relate the solar irradiance to the ensemble average flux from a number of bright, early-type stars (same stars used by the UARS SOLSTICE program)
  • 6. Objectives: 3. Make the first measurements of the visible and near IR solar irradiance with sufficient precision for future climate studies. Obtain daily measurements of solar spectral irradiance between 0.3 and 2 µm with a spectral resolution of at least 1/30, an accuracy of 0.03%, and a long-term repeatability of better than 0.01%/yr.
  • 7. Objectives: 4. Improve the understanding of how and why solar irradiance varies, estimate past and future solar behavior, and investigate climate responses.
  • 8. Team Edward Chang SORCE Project Manager Robert CahalanSORCE Project Scientist
  • 9. Team Doug Rabin SORCE Deputy Project Scientist  Don Anderson NASA Headquarters
  • 10. Team Thomas SparnProgram Manager Brian BoyleSystems Engineering, Instrument Integration and Test, Mission Analysis, and Instrument Operations Manager 
  • 11. Team Vanessa George Research CoordinatorLASP(Laboratory for Atmospheric and Space Physics) Ken GriestPlanning/Scheduling Engineer 
  • 12. Team Barry Knapp Ground S/W Engineer/Analyst, LASP   (Laboratory for Atmospheric and Space Physics) Richard KohnertChief Systems Engineer  
  • 13. Team Doug Lindholm Ground S/W Engineer/AnalystLASP (Laboratory for Atmospheric and Space Physics) Deb McCabe Flight Director,
  • 14. Team Randy Meisner Ground S/W Engineer / Analyst  Chris PankratzScience Operations ManagerLASP (Laboratory for Atmospheric and Space Physics)  
  • 15. Team Sean Ryan Mission Operations Manager,  LASP (Laboratory for Atmospheric and Space Physics) Ann Windnagel Ground S/W Engineer/Analyst LASP (Laboratory for Atmospheric and Space Physics)  
  • 16. Agencies NASA Goddard Space Flight Center University of Colorado at Boulder