LYRA/EPT Perturba0ons Project Thanassis Katsiyannis Marie Dominique - - PowerPoint PPT Presentation

lyra ept perturba0ons project
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LYRA/EPT Perturba0ons Project Thanassis Katsiyannis Marie Dominique - - PowerPoint PPT Presentation

LYRA/EPT Perturba0ons Project Thanassis Katsiyannis Marie Dominique et al. Detec0on Algorithm Likelihood of detec0on VS Geomagne0c disturbance McIlwain L-Shells Detec0on Maps for LYRA and EPT Differences between LYRA and EPT detec0ons LYRA


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SLIDE 1

LYRA/EPT Perturba0ons Project

Thanassis Katsiyannis Marie Dominique et al.

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SLIDE 2

Detec0on Algorithm

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SLIDE 3

Likelihood of detec0on VS Geomagne0c disturbance

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SLIDE 4

McIlwain L-Shells

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SLIDE 5

Detec0on Maps for LYRA and EPT

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SLIDE 6

Differences between LYRA and EPT detec0ons

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SLIDE 7

LYRA as in-situ electron detector

  • Although not designed as such, LYRA is clearly capable of detec@ng

highly rela@vis@c electrons in situ

  • Whereas the electrons of the same energies can be detected by other

instruments, LYRA has the highest cadence

  • Even if LYRA had no advantage on the observa@on of electrons, being

able to detect in situ par@cles in an addi@onal orbit is very useful

  • Radiometers with thin metal filters will never replace dedicated in-

situ instruments, but they are a cost effec@ve way to complement them

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SLIDE 8

The PROBA-2 orbit

  • Heliosynchronous
  • Polar
  • Dawn-Dusk
  • 750 km al@tude
  • 100 min dura@on
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SLIDE 9

The LYRA instrument

Ly Hz Al Zr 120-123 nm 190-222 nm 17-80 nm + <5nm 6-20 nm + <2nm Unit1 MSM - diamond PIN- diamond MSM- diamond P-N Silicon Unit2 MSM- diamond PIN- diamond MSM- diamond MSM- diamond Unit3 P-N Silicon PIN- diamond P-N Silicon P-N Silicon