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COBRAT project: LONG DURATION FLIGHTS OF STRATOSPHERIC BALLOONS FOR THE STUDY OF HIGH ENERGY PHENOMENA Jean-Baptiste RENARDElena SERAN Gwenaël BERTHETMichel.

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Presentation on theme: "COBRAT project: LONG DURATION FLIGHTS OF STRATOSPHERIC BALLOONS FOR THE STUDY OF HIGH ENERGY PHENOMENA Jean-Baptiste RENARDElena SERAN Gwenaël BERTHETMichel."— Presentation transcript:

1 COBRAT project: LONG DURATION FLIGHTS OF STRATOSPHERIC BALLOONS FOR THE STUDY OF HIGH ENERGY PHENOMENA Jean-Baptiste RENARDElena SERAN Gwenaël BERTHETMichel GODEFROY Valéry CATOIREFrancis VIVAT Nathalie HURET Dominique LAGOUTTE Pierre-Louis BLELLY François LEFEUVRE Jean-André SAUVAUD Aurélie MARCHAUDON François FORME Jean-Louis PINCON Claude ROBERT Torsten NEUBERT Michel TAGGER Serge SOULA

2 This is a starting project, linked with TARANIS satellite (CNES) and ASIM instrument onboard ISS (ESA) High energy phenomena in the middle and upper stratosphere above thunderstorms Discharges above thunderstorms

3 t=1.66 mst=2.06 mst=2.26 mst=2.46 mst=2.66 ms t=3.06 ms t=3.46 ms t=3.66 ms t=7.86 mst=6.26 ms t=4.66 mst=4.06 ms 40 km 45 km 50 km 55 km 60 km 65 km 70 km 75 km 80 km 40 km 45 km 50 km 55 km 60 km 65 km 70 km 75 km 80 km Fast camera imaging of a sprite

4 TARANIS and ASIM : Instruments for the measurements of Transient Luminous Events (TEL) and of Terrestrial Gamma-ray Flashes (TGF) Launch around 2012...

5 TARANIS: - cameras and photometers - X and Gamma rays detectors - measurements of high-energy electrons - measurements of electric and magnetic fieldsASIM: - observations from the lowest available orbit (350-450 km) - spectroscopic imaging mission - cameras and photometers - X and Gamma Ray detectors

6 Production of NOx (NO+NO 2 ) in the upper stratosphere by high energy phenomena, for ex. after strong solar eruption (high energy protons) Detection using satellite instruments over polar cap GOMOS onboard Envisat Nighttime measurements

7 Smaller enhancements expected during TLE/TGF events Satellite data are difficult to use for detection of such « local » NOx enhancements - Line of sight of several hundreds of km in the stratosphere (=> dilution of the absolute values of the enhancements) - Need of daytime and nighttime measurements (long persistence of the enhancements due to the absence of photochemistry)

8 Best solution : Use of instruments onboard stratospheric balloons up to altitude of 40 km Remote sensing and in-situ measurements Gondolas of ~200 kg ? Need of “long duration flights” (at least several days) to stay close to thunderstorm areas BSO (zero pressure) balloons COBRAT Project (Coupled Observations from Balloon Related to ASIM and Taranis): Measurements of stratospheric chemistry and of TLE and TGF (+ imaging measurements from ground)

9 Several gondolas with different instruments coming from different European teams - Measurements of stratospheric species by in-situ and remote sensing techniques - Detection of terrestrial gamma rays flashes - Electric fields measurements - Detection of TLE by fast cameras

10 Terrestrial Gamma-ray Flashes - Balloons can allow to perform in situ measurements - Between 20 and 40 km, good probability of detecting TGF - Use of an already existing balloon-borne instrument (that needs to be improved …) ? Electric fields measurements - Instrument needs to be defined … Detection of TLE ATLEC - Use of fast cameras ATLEC (Atmospheric Transient Luminous Event Camera) …


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