Details of the balloon and launch operations
Launch site:European Space Range, Kiruna, Sweden
Launch team: CNES
Balloon: Open balloon model 150z 150.000 m3
Serial number: 150Z Nº 19
Flight identification number: -
Campaign: ILAS VALIDATION 97
Payload weight: 894 kgs
Gondola weight: 556 kgs
Overall weight: -
Description of the payload or experiment
LPMA (Limb Profile Monitor of the Atmosphere) + CAESR
Responsable institution: Laboratoire de Physique Moléculaire et Applications - CNRS
Principal Investigator: Claude Camy-Peyret
The LPMA instrument (Limb Profile Monitor of the Atmosphere) is a high spectral resolution Fourier transform spectrometer operating in absorption against the sun. The objective is to record limb atmospheric spectra in selected intervals from the thermal infrared to the near-infrared.
The instrument is composed by a commercial BOMEM DA2 spectrometer customized for balloon operations. A specially designed two detectors output optics enables to cover simultaneously two spectral regions making it possible to sample simultaneously the two interferograms detected during the same scan of the moving mirror and allowing to collect information on atmospheric species absorbing in widely different spectral regions.
In order to reach a good signal to noise ratio spectra performance, the interferometer must be feeded with a stable solar beam exactly aligned along the optical axis of the instrument. To be able to do this, two sub-systems of the gondola are needed:
- a primary pointing system initially developed by the Observatory of Geneva for astronomical payloads, controling the azimuth of the gondola and maintaining the sun in the field of view of the instrument even during ascent in the dense layers of the upper troposphere or lower stratosphere where this is a rather difficult achievement.
- a suntracker (also known as a heliostat) developed in cooperation with the Institut d'Electronique el de Micro-electronique du Nord performing the fine pointing of the acquisition mirror through 2 axes servo-controlled gimbal compensating for the residual motions of the payload and maintaining a jitter of the solar beam direction at the input of the interferometer of less than 1 arc min.
In addition it is possible to accomodate on the gondola another instrument of the class 30-50 kg wich can benefit from their good pointing capabilities.
In this flight also was part of the scientific payload onboard the gondola the University of Denver's Cold Atmospheric Emission Spectral Radiometer (CAESR), a cryogenically cooled medium resolution grating spectral radiometer recording atmospheric thermal emission in the direction opposite to the sun.
Performance in flight and data obtained
>> No data available
External references and bibliographical sources
- LPMA project Laboratoire de Physique Moléculaire pour l'Atmosphère et l'Astrophysique