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W. Vernon Jones Senior Scientist for Suborbital Research Astrophysics Division, DH000

14 th HEAD Meeting. Chicago, IL 17 – 21 August 2014. “ Overview of the NASA Suborbital Program ”. W. Vernon Jones Senior Scientist for Suborbital Research Astrophysics Division, DH000 Science Mission Directorate NASA Headquarters August 18 , 2014. NASA ’ s Suborbital Program.

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W. Vernon Jones Senior Scientist for Suborbital Research Astrophysics Division, DH000

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  1. 14th HEAD Meeting Chicago, IL 17 – 21 August 2014 “Overview of the NASA Suborbital Program” W. Vernon Jones Senior Scientist for Suborbital Research Astrophysics Division, DH000 Science Mission Directorate NASA Headquarters August 18, 2014

  2. NASA’s Suborbital Program • NASA’s Suborbital Program, comprised of the Sounding Rocket and Balloon Projects, is managed within the Science Mission Directorate (SMD) under the tutelage of the Senior Suborbital Program Executive. • The Heliophysics Division provides oversight of Sounding Rockets. • The Astrophysics Division provides oversight of Balloons. • Flight Operations are managed through support contracts by a “Program” Office for each “Project” at the NASA/GSFC Wallops Flight Facility (WFF). • Sounding rocket flights are conducted by the NASA Sounding Rocket Operations Contract (NSROC). • Balloon flights are conducted by the Columbia Scientific Balloon Facility (CSBF).

  3. Merit of the Suborbital Program • Suborbital Projects offer flight opportunities for unique science investigations that require, or can be done in, near-space. • They offer quick access to space at much less cost than orbital missions. • They play important roles in migrating bench top technologies to space flight readiness levels. • They provide students with hands-on hardware training crucial for developing the next generation of scientists and engineers. • The time to go from concept, to detector, to flight, and data analysis is consistent with pursuit of a graduate degree. • They are the primary engine for generating new scientists with the hardware and project management skills needed to lead new space missions.

  4. Antarctica: Center Piece of NASA Ballooning • NASA-NSF/PLR Long-Duration Ballooning (LDB) provides: • – NASA’s lowest cost access to space (>= stratosphere). • – Spacecraft-scale payloads (1000 - 2000 kg science instruments). • – Recoverable/Re-usable payloads increase exposure at low cost. • The Balloon Program has focused on expanding the highly successful LDB flights OVER /AROUND Antarctica. • – Flight durations of up to 4-8 weeks. • – Flight support to 3 payload every year. • Frontier Astrophysics on Super-Pressure Balloons (SPB) will justify Ultra-Long Duration Balloon (ULDB) flights FROM Antarctica In the coming decade. • – ULDB flights from Antarctica would yield long exposures: 60 days now; 100 days soon. • • NASA is working with NSF/PLR to enable flights to leave Antarctica for possible recovery in South America, New Zealand, Australia, etc. • –Initial ULDB capability does not include payload recovery. 55-day SperTIGER Flight Dec - Feb 2013 42-day CREAM flight Dec - Jan 2004-05 54-day SPB flight Dec 09- Feb 2008-

  5. History of Antarctic Balloon Flights • 44 Antarctic Long-Duration Balloon (LDB) Flights Since 1991: • 31 single circumpolar flights with durations of 8 - 25 days. • 6 double circumpolar flights with durations of 20 - 32 days. • 5 triple circumpolar flights with durations of 35 – 55 days. • 2 super-pressure balloon (SPB) test flights: 54 days; 22 days. • Recent History and Near-Term Plan for Antarctic LDB Flights: • FY 2013 Campaign (2012-2013 Season) was most successful ever. • Super-Trans Iron Galactic Element Recorder (Super-TIGER). • Balloon Large Aperture Sub-millimeter Telescope (BLAST). • E and B EXperiment (EBEX). • FY 2014 Campaign (2013-2014 Season) was Cancelled • due to U. S. Government Shutdown October 1-16, 2013 ! • FY 2015 Campaign Candidates (2014-2015 Season): PIC 01/23/14 • – COmpton Spectroscopic Imager (COSI) on Super Pressure Balloon (SPB). • – Antarctic Impulsive Transient Antenna (ANITA). • A Large Angular Scale Millimeter-wave Polarimeter (SPIDER). • FY 2016 Campaign Candidates (2015-2016 Season) Undetermined. • Boron And Carbon Cosmic-rays in the Upper Stratosphere (BACCUS) was brought back from Christchurch, NZ, along with Spider and SPB.

  6. FY-13 Antarctic Campaign: 2012-13 Season Three balloon payloads launched in Dec. 2012 collectively flew 96 days! Super-TIGER: 55+ DaysBLAST-Pol: 16+ DaysEBEX: 25+ Days EBEX BLAST

  7. SuperTIGER Exceeded 2008-09 SPB Flight Record • 2008-09 SPB Test • 54 days of flight: • Balloon remained pressurized- no apparent gas loss. • It could have flown indefinitely. • 2012-13 SuperTIGER • 55 days of flight: • Vented Zero-Pressure balloon in equilibrium with the atmosphere. • The altitude changed with air temperature/pressure.

  8. Scientific Research Balloons: How Big?

  9. Evolution to Super Pressure Ballooning • Long Duration Balloon (LDB) flights employing conventional, zero-pressure balloons have a proven history of scientific discovery, with many cited achievements. • Most high priority projects are proposing multiple LDB missions. • Super-pressure balloons are major technological advance. • - They offer an order of magnitude increase in flight capability. • They enable Ultra Long Duration Balloon (ULDB) flights (60-100 days). • They open areas of exploration closed to zero-pressure balloons, e.g., LDB flights in non-polar-regions. • Costs to convert most LDB payloads for ULDB flights are modest. • LDB and ULDB together form a science opportunity continuum. • - They offer significant science at fraction of the cost of a space mission. • - ULDB missions may be acceptable alternative to some Small Explorer (SMEX) missions.. • Balloon payloads have been solicited as Missions of Opportunity in Explorer AO’s. • - Two balloon missions (ANITA, GUSSTO) selected for Phase A studies, but neither was down-selected for flight.

  10. Super Pressure Balloon (SPB)“ First New Balloon Design in more than 60 Years ” Pumpkin Shape H/D = 0.623 • Schematic / Statistics • Volume = 420,150 m3 (14.837 MCF) • Diameter = 105.832 m • Height = 65.946 m • Number of gores = 230 • Gore length stressed = 139.023 m • Gore width stressed = 1.471 m • Film thickness 38 microns (1.5 mil) • Photograph of 7 MCF SPB at float • Altitude: ~33.87 km (~111,100 ft) • 54-day test flight 12/28/08 – 2/20/09 • 22-day flight of 14.8 MCF with 4000 lb payload during January 2011

  11. Sounding Rocket Program Overview • The NASA Sounding Rocket Program supports an on-going flight manifest of approximately 20-25 flights per year. • The sounding rocket program operates in a “higher risk / lower consequence” environment that enables low cost access to space for scientific research, instrument development, and training. • Customers include Heliophysics, Astrophysics, and other NASA and non-NASA customers. • Stable of launch vehicles based on surplus & commercial rocket motors • Payloads weights up to 2000 lbs. • World-wide operations conducted at fixed and temporary launch sites. Scientific Instrument SRP Subsystems SRP Subsystems

  12. World-wide Launch Operations Poker Flat Research Range, Alaska Esrange, Sweden Andoya Rocket Range, Nroway Because many scientific investigations rely on in-situ measurements, launch operations must be conducted from sites around the world. Wallops Flight Facility, USA

  13. Example Astrophysics Sounding Rocket Payload * The Cosmic Infrared Background Experiment (CIBER) from Caltech was first flown from White Sands Missile Range on February 25, 2009. * CIBER’s high sensitivity observations in a short sounding rocket flight eliminated the atmospheric airglow emission that makes absolute spectroscopy and high-fidelity degree-scale imaging virtually impossible from a ground based or balloon-borne platform. * The complex Attitude Control System (ACS) mission profile required pointing at seven different targets!

  14. Thank You !

  15. Key Events in a Balloon Launch Sequence 0

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