The Cosmic Particle Telescope First Results 1st Symposium on Space - - PowerPoint PPT Presentation

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The Cosmic Particle Telescope First Results 1st Symposium on Space - - PowerPoint PPT Presentation

The Cosmic Particle Telescope First Results 1st Symposium on Space Educational Activities Padova, Italy | Dec. 9-11, 2015 Presented on behalf of the CPT-SCOPE team by Anastasiya Dykyy, NTNU Trondheim, Norway and Timo A. Stein, IDEAS,


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SLIDE 1

The Cosmic Particle Telescope – First Results

1st Symposium on Space Educational Activities Padova, Italy | Dec. 9-11, 2015 Presented on behalf of the CPT-SCOPE team by Anastasiya Dykyy, NTNU Trondheim, Norway and Timo A. Stein, IDEAS, Norway timo.stein@ideas.no

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SLIDE 2

What is CPT-SCOPE?

CPT-SCOPE (Cosmic Particle Telescope):

joint Norwegian-German student project to build a low-cost, compact radiation monitor for European nano- and pico satellites … for ow a tehology deostrator to fly aoard a stratospheri alloo.

Strategy:

  • use off-the-shelf components (system)
  • use rad.-hard integrated circuit technology (detector front-end)
  • use particle telescope geometry
  • use industrial Si-detectors

Partners:

  • IDEAS, Oslo, Norway
  • NTNU, Trondheim, Norway
  • {FU, TU, BEUTH}, Berlin, Germany

rad.-hard VATA IC, credit: IDEAS particle telescope sketch

http://www.cpt-scope.com

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SLIDE 3

Objectives

Technology (primary):

  • compact radiation monitor for (near)

space applications

  • readiness of ASIC
  • particle telescope geometry

Science (secondary):

  • detection of energetic subatomic

particles in the stratosphere

Space weather, credit: S. Hill/SOHO/NASA

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SLIDE 4

CPT-SCOPE

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SLIDE 5

CPT-SCOPE

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SLIDE 6

CPT-SCOPE

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SLIDE 7

Flight test aboard BEXUS 20, Oct. 10, 2015

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SLIDE 8

Flight test aboard BEXUS 20, Oct. 10, 2015

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SLIDE 9

Flight test aboard BEXUS 20, Oct. 10, 2015

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SLIDE 10

Flight test aboard BEXUS 20, Oct. 10, 2015

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SLIDE 11

Flight test aboard BEXUS 20, Oct. 10, 2015

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SLIDE 12

Results: 25+ h operations

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SLIDE 13

Results: count rate vs. interaction depth - CA

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SLIDE 14

Results: count rate vs. interaction depth - CB

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SLIDE 15

Quick explanation

Cosmic Ray particle shower (left) and number of particles (right), credit: R. Nave, hyperphysics

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SLIDE 16

Results: Temperature vs. time - CA

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SLIDE 17

Results: Atmospheric meas. - CA

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SLIDE 18

Roadmap

CPT-SCOPE 1.0 on BEXUS 20, 10/2015 Lab Prototype 05/201515 CPT-SCOPE 2.0 aboard CubeSat, 2018 European compact radiation monitor, 2019

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SLIDE 19

Sponsors and supporters

Timo would like to thank DLR for providing a student conference sponsorship.

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SLIDE 20

Team CPT-SCOPE

Michael Beermann (N) Anastasiya Dykyy (N) Fabian Freyer (G) Lucas Kempe (G) Julian Petrasch (G) Patrick Schönberg (G) Johannes Stahn (G) Timo A. Stein (N) Anton Walter (G) Ron Wenzel (G) Grunde H. Wesenberg (G)

(G) Germany, (N) Norway

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SLIDE 21

The last slide

Contact Data: Timo A. Stein UiO / Integrated Detector Electronics AS Oslo, Norway e-mail: timo.stein@ideas.no

Thanks for your attention! ___ Questions?

http://www.cpt-scope.com