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Proba-2 teams up with solar eclipse watchers
 
12 July 2010

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During the 11 July 2010 solar eclipse Proba-2's orbit crossed the path of the Moon's shadow a total of four times. Transits in between have been edited out of this SWAP animation.

Credits: ESA/ROB
 
  SWAP: observing beyond the visible
 
Proba-2
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Proba-2 is flight-testing a total of 17 technology demonstrators for future ESA missions. It also serves as a scientific platform for solar and space weather observations.

Credits: ESA/Pierre Carril
 
 
Charting the extended solar corona
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This composite mosaic image of the solar corona was made out of hundreds of individual Proba-2 SWAP images gathered in off-pointing mode shortly in advance of the 11 July 2010 solar eclipse. The result is an image with an extended field of view: a plasma structure extending up to one solar radius above the solar limb can be distinguised in the north-east direction (top left). Blocking out the solar disc gives an approximation of what people on the ground at Easter Island should have seen. Produced by Vladimir Slemzin (Lebedev Institute, Russia).

Credits: ESA/ROB Produced by Vladimir Slemzin (Lebedev Institute, Russia).
 
 
Eclipse image
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Proba-2 imaging the Sun during the solar eclipse on 11 July 2010. Experienced as a total eclipse across parts of the Pacific, Proba-2's orbit kept it outside the path of totality. The eclipse lasted through four Proba-2 orbits.

Credits: ESA/ROB
 
  DSLP and TPMU: probing ionosphere hole
 
Proba-2 instruments
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The DSLP (Dual Segmented Langmuir Probe) instrument on board the Proba-2 spacecraft at QinetiQ Space's (then Verhaert's) cleanroom facility in Kruibeke, Belgium. The two segmented Langmuir probe sensors SLPA and SLPB (see details in the left hand frames) are mounted in one of the deployable solar panels. Amplified signals measured on the sensors are led by the white-coloured harness into the DPU (digital processing unit, detailed view in the right frame) which is accomodated on the main platform inside the body of the satellite.

The DSLP is one of the four scientific experiments on board the ESA microsatellite Proba-2. The DSLP instrument has been developed and manufactured in the Czech Republic by a scientific-industrial consortium within the ESA PECS/PRODEX program. The consortium is led by the Astronomical Institute (Academy of Sciences of the Czech Republic) with technological and industrial support provided by the Research and Scientific Support Department of ESTEC/ESA (Noordwijk, Holland) and the Czech Space Research Center company (Brno, Czech Republic). As a part of the Plasma Measurement Equipment, the DSLP instrument will aim at studying characteristic macroscopic properties (e.g. density, temperature or flow dynamics) of ionospheric plasmas and, with use of SWAP and LYRA observations, try to identify observed irregularities with possible solar-terrestrial connection related to sudden space weather events. A comprehensive knowledge of the ionospheric environment is important from many not solely scientific aspects. Intense solar events cause massive geomagnetic storms that represent possible risk of damage for communication and navigation satellite systems, ground electric grids and pipelines, or even radiation hazards for humans. Detailed study of ionospheric processes and their space weather relations thus becomes an considerable issue in current space research activities.

Credits: ESA/Academy of Sciences of the Czech Republic

 


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Proba-2: science payloadsProba-2: technology demonstrationsRoyal Observatory of BelgiumROB Proba-2 science centre
 
 
 
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