0000000000985167

AUTHOR

M. D. Sabau

showing 2 related works from this author

The Modular X- and Gamma-Ray Sensor (MXGS)of the ASIM Payload on the International Space Station

2019

The Modular X- and Gamma-ray Sensor (MXGS) is an imaging and spectral X- and Gamma-ray instrument mounted on the starboard side of the Columbus module on the International Space Station. Together with the Modular Multi-Spectral Imaging Assembly (MMIA) (Chanrion et al. this issue) MXGS constitutes the instruments of the Atmosphere-Space Interactions Monitor (ASIM) (Neubert et al. this issue). The main objectives of MXGS are to image and measure the spectrum of X- and γ-rays from lightning discharges, known as Terrestrial Gamma-ray Flashes (TGFs), and for MMIA to image and perform high speed photometry of Transient Luminous Events (TLEs) and lightning discharges. With these two instruments sp…

Modular Multi-Spectral Imaging AssemblyPhysics - Instrumentation and Detectors010504 meteorology & atmospheric sciencesModular X- and Gamma-ray SensorFOS: Physical sciencesTerrestrial Gamma-ray FlashesInternational Space Station01 natural sciencesPhysics - Space Physics0103 physical sciencesInternational Space Station010303 astronomy & astrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Atmosphere-Space Interaction Monitor0105 earth and related environmental sciencesRemote sensingPhysicsbusiness.industryPayloadGamma rayX- and Gamma-ray detector for spaceAstronomy and AstrophysicsInstrumentation and Detectors (physics.ins-det)Modular designLightningSpace Physics (physics.space-ph)Photometry (astronomy)Space and Planetary ScienceTransient (oscillation)Astrophysics - Instrumentation and Methods for Astrophysicsbusiness
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The Spanish infrared camera onboard the EUSO-BALLOON (CNES) flight on August 24, 2014

2015

The EUSO-Balloon (CNES) campaign was held during Summer 2014 with a launch on August 24. In the gondola, next to the Photo Detector Module (PDM), a completely isolated Infrared camera was allocated. Also, a helicopter which shooted flashers flew below the balloon. We have retrieved the Cloud Top Height (CTH) with the IR camera, and also the optical depth of the nonclear atmosphere have been inferred with two approaches: The first one is with the comparison of the brightness temperature of the cloud and the real temperature obtained after the pertinent corrections. The second one is by measuring the detected signal from the helicopter flashers by the IR Camera, considering the energy of the …

Aeronáutica
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