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EUSO-Balloon is a balloon-borne experiment performed in collaboration with the French Space Agency CNES. It was equipped with one full original JEM-EUSO PDM (photon detection module with 2304 pixels) and with an optical system made of two Fresnel lenses, with a side of 1 meter covering a field of view of 12 degrees. In addition to the main instrument, a stand-alone and waterproof infrared camera was on board.

The EUSO-Balloon payload in Timmins (CA).
The EUSO-Balloon payload in Timmins (CA). The optical system consists of two lenses of one square meter built in RIKEN and a focal surface of multi anode photomultipliers On top is the float to avoid sinking.

On the moonless night of August 25, 2014, the instrument, installed on board a Gondola, has been brought by a stratospheric balloon to a float altitude of 38 km for more than 5 hours before descending to ground. The flight has been performed by the balloon division of the French Space Agency CNES from Timmins Balloon base (Ontario, Canada) [ref.1]. The payload electronics draws from the experience of several balloon campaigns to study the antiparticle component in cosmic rays with a magnetic spectrometer in the year 1989-1998 (TS93, Caprice-94, 98…).

All the subsystems of EUSO-Balloon behaved in flight according to their nominal requirements, performing full scale end-to-end test of most of the key technologies and instrumentation of JEM-EUSO detectors.
A detailed and precise measurement of the UV background in different atmospheric and ground conditions was achieved. The instrument proved even the capability of detecting Extensive Air Showers by observing calibrated UV–led and Xe flashers and tracks of a laser shots emitted from a NASA-funded helicopter, which flew under the balloon for about two hours.

In addition,  the UV emissions from northern Canada were sampled for the first time with a temporal resolution from 2.5ms to 1 s and a spatial resolution of 1km.

Image of a helicopter event
Image of a helicopter event. The flasher signals move from  left to right.
he intensity map of UV background in photons m-2sr-1ns-1 in logarithmic scale
he intensity map of UV background in photons m-2sr-1ns-1 in logarithmic scale. The bright areas with high intensities represent artificial light in Timmins with neighborhoods, mines, and airport. The red and light blue areas are related to cloud coverage.
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Transport
Reference
  1. J. H., et al. The EUSO-Balloon pathnder. Experimental Astronomy, 40:281{299, November 2015. doi: 10.1007/s10686-015-9467-9.