Data of the stratospheric balloon launched on 12/12/2003
For TRACER (Transition Radiation Array for Cosmic Energetic Radiation)

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Details of the balloon and launch operations


 
Launch site:Williams Field, McMurdo Base, Antarctica  
Launch team: National Scientific Balloon Facility (NSBF)
Balloon: Open balloon (zero pressure)
Volume: Raven W 39.570.000 cuft - (0.8 mil)
Serial number: -
Flight identification number: 526N
Campaign: - 
Payload weight: 3550 lbs
Gondola weight: -
Overall weight: 5966 lbs

The balloon was launched on December 12th at 6:09 UTC by dynamic method assited by launch vehicle. Following a nominal ascent phase, the balloon reached float altitude of 125.000 feet at 00:30 local time starting an anti-clockwise flight trajectory over the antarctic plateau.

After a few days of flight without incidents,on december 15th the balloon cross over the Vostok lake (considered the coldest place on earth) thus the balloon get cold and droped altitude to 120,000 ft. but continuing his travel until on December 20th it passed over the Ronne Ice Shelf. The more sunlight reflected off the ice warmed the balloon and thus it regained altitude to over 127,000 ft.

Fronm there, the travel continued without troubles until December 23th when the science team lose contact with TRACER instrument apparently due to the failure of the primary power system. This led to terminate the data taking phase of the flight.

On December 26th the balloon completed the full circle around the pole and passed within 80 miles of McMurdo Station at the same level flight of 127,000 ft. It appeared as a large white object in the sky remaining almost stalled for a period of hours over the Royal Society Mountains. Finally on December 27th the flight was terminated when the balloon was over Victoria Land on the East Antarctic Plateau. After separation, the instrument parachuted to earth but after landing the parachute failed to get dettached from it, so the wind inflated again the parachute's canopy resulting in the payload beeing dragged six miles across the snow. Finally the gondola stoped his drag within 100 miles of McMurdo Station.

A Twin Otter plane located the gondola on December 28th thanks to the 10 foot wide furrow in the snow. Although the incident the instrument itself was intact and was secured by the rescue team wich landed nearby and recovered the science data Hard Disks. The following days, bad weather conditions prevented the recovery of the rest of the payload wich lasted in the snow until January 2004 when the operation was completed and the instrument was shiped back to United States.  

Images


Click to enlarge.

View of the flight line

The balloon already inflated waiting for launch. In the background a smoke trail from Mt. Erebuz

The instrument in the landing site after stop the sailing over the ice

The trail left by TRACER on the plateau after being dragged by the undetached parachute. The technician holds in her hands some components of the instrument left in the ground due to dragging.

Due to the height of the landing place, some personel is wearing air masks

© John W.Epstein

Description of the payload or experiment


TRACER (Transition Radiation Array for Cosmic Energetic Radiation)

Responsable institution:  University of Chicago
Principal Investigator:  Prof. Dietrich Müller

An instrument created to make direct measurements of heavy cosmic ray nuclei (oxygen to iron) in the energy range of several eV. It measures the nuclear charge, the energy, and the trajectory of the cosmic ray particles through the instrument. For charge measurements, two layers of plastic scintillators (2 x 2 m2), and one Cerenkov counter (2 x 2 m2) are used. The two scintillators are placed on top and bottom of the detector stack acting as instrument trigger, and the Cerenkov counter made of acrylic plastic located at the bottom of the detector is used to reject non-relativistic particles. At left can be seen an sketch of the several layers that compose the instrument (click to enlarge).

For the energy measurement it uses a transition radiation detector system which determines the Lorentz factor. This approach permits the construction of large-area detectors without requiring an exorbitant detector mass.

To determine the trajectory of the incoming particles TRACER have eight double layers of proportional tubes which are oriented alternately in two orthogonal directions to permit corrections in the data pathlength variations.  

Performance in flight and data obtained


This was the first long duration antarctic flight of the instrument. TRACER sampled over 50 Million heavy Cosmic Rays during the entire 14 days flight.

External references and bibliographical sources


  The Response of the TRACER Detector: Design, Calibrations and Measurements 29th International Cosmic Ray Conference 2005, Pune, India
  TRACER web site University of Chicago
 A New Detector for Measurments of the Composition of Heavy Cosmic Ray Nuclei beyond TeV-Energies 26th International Cosmic Ray Conference 2005, Salt Lake City, Utah
 Antarctic Balloon Flight and Data Analysis of TRACER 29th International Cosmic Ray Conference 2005, Pune, India
 Balloons up and away: TRACER takes flight Article on TRACER from the Antarctic Sun magazine
 Chicago instrument will advance study of high-energy cosmic rays Article at Chicago Chronicle
 Cosmic ray composition at high energies: Results from the TRACER project 36th COSPAR Scientific Assembly. Held 16 - 23 July 2006, in Beijing, China
 Energy Spectra of Heavy Cosmic Ray Nuclei from 0.5 GeV/amu to 10,000 GeV/amu 29th International Cosmic Ray Conference 2005, Pune, India
 Large Area Transition Radiation Detectors for Cosmic Ray Observations in Space 27th International Cosmic Ray Conference 2005, Hamburg, Germany
 Measurements with TRACER: Discussion of Results and Future Prospects 29th International Cosmic Ray Conference 2005, Pune, India

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