For FIRST (Far-Infrared Spectroscopy of the Troposphere)

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Launch site:Fort Sumner Municipal Airport, New Mexico, US  
Launch team: National Scientific Balloon Facility (NSBF)
Balloon: Open balloon (zero pressure)
Volume: Raven 11.820.000 cuft - (0.8 Mil.)
Serial number: W 11.82-3E-08
Flight identification number: 544N
Campaign: - 
Payload weight: 2485 lbs
Gondola weight: -
Overall weight: 3768 lbs

Succesfull launch using dynamic method by launch vehicle (Big Bill) at 13:56 utc.

After a nominal ascent phase the balloon reached the float altitude of 107.800 ft and started a drift toward the centre of the State (click the map at left to see the flight path).

Then a mid-float valve down was commanded, permitting the balloon descent to approximately 88.000 ft to facilitate the science instrument functioning.

After more than 10 hours of flight the balloon was terminated at 23:49 utc. The termination and visual parachute separation were normal and the payload touched ground at 00:32 utc (on June 8th UTC time) 44 miles northwest of Fort Sumner (34-53.6 N / 104-59.4 W).

Moderate surface winds resulted in the payload being drug for a short distance. However, only minor damage resulted.  

FIRST (Far-Infrared Spectroscopy of the Troposphere)

Responsable institution:  NASA Langley Research Center / Utah State University
Principal Investigator:  Martin Mlynczak, Ph.D.

FIRST is a new sensor designed to measure critical but previously unobserved components of the Earth’s atmosphere. It's mainly composed by a Fourier Transform Spectrometer wich gives greatest possible span of wavelengths in a single instrument along with a beamsplitter made of germanium on polypropylene with excellent response in far-IR and minimal absorption features, detectors with kilohertz sampling frequencies to record more than 1000 samples by second and with a single focal plane to simplify the optical design and calibration. At left can be seen a scheme of it (click to enlarge).

The goal of the FIRST project was to develop the technologies that will allow direct measurements of the infrared radiation leaving the Earth and its atmosphere at wavelengths longer than 15 micrometers out to as far as 100 micrometers. The portion of the infrared spectrum between 15 and 100 micrometers, which scientists refer to as the "far-infrared," has rarely been observed directly from space or from instruments on the ground or in aircraft.

Also in this flight as a Piggyback experiments from 41 schools representing 17 states were flown in a NASA Student Experiment Module. The experiments, in brick-size plastic containers inside two larger containers about the size of large briefcases, are looking at the effect of the flight environment on test articles such as materials, microscopic organisms and seeds.