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IDEE, The Electron Spectrometer for the Taranis Mission J.-A. Sauvaud 1 , P. Devoto, A. Fedorov 1 , G. Orttner 1 , O. Chasselat 1 , K. Wong 1 , L. Prech 2 , Z. Nemecek 2 , 1 IRAP/CNRS-U. of Toulouse 2 Charles University, Prague Chibis international workshop, Tarusa, 13-15 february 2013

IDEE, The Electron Spectrometer for the Taranis Mission J.-A. Sauvaud 1, P. Devoto, A. Fedorov 1, G. Orttner 1, O. Chasselat 1, K. Wong 1, L. Prech 2,

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Page 1: IDEE, The Electron Spectrometer for the Taranis Mission J.-A. Sauvaud 1, P. Devoto, A. Fedorov 1, G. Orttner 1, O. Chasselat 1, K. Wong 1, L. Prech 2,

IDEE, The Electron Spectrometer for the Taranis Mission

J.-A. Sauvaud1, P. Devoto, A. Fedorov1, G. Orttner1,

O. Chasselat1, K. Wong1, L. Prech2, Z. Nemecek2,

1 IRAP/CNRS-U. of Toulouse

2 Charles University, Prague

Chibis international workshop, Tarusa, 13-15 february 2013

Page 2: IDEE, The Electron Spectrometer for the Taranis Mission J.-A. Sauvaud 1, P. Devoto, A. Fedorov 1, G. Orttner 1, O. Chasselat 1, K. Wong 1, L. Prech 2,

IDEE conception

3 objectives:

-Pitch-angle Distribution of Radiation Belt Electrons (wave particle interactions)

-Lightning-induced Electron Precipitation (LEP)

-Relativistic Runaway Electrons (RRE)

Page 3: IDEE, The Electron Spectrometer for the Taranis Mission J.-A. Sauvaud 1, P. Devoto, A. Fedorov 1, G. Orttner 1, O. Chasselat 1, K. Wong 1, L. Prech 2,

W= 3.5 eV/e--hole pair

The spectrometers uses semi-conductors as particle detectors

DEMETER and TARANIS

Page 4: IDEE, The Electron Spectrometer for the Taranis Mission J.-A. Sauvaud 1, P. Devoto, A. Fedorov 1, G. Orttner 1, O. Chasselat 1, K. Wong 1, L. Prech 2,

WAVE PARTICLE INTERACTIONS

1. Cyclotron resonance

Page 5: IDEE, The Electron Spectrometer for the Taranis Mission J.-A. Sauvaud 1, P. Devoto, A. Fedorov 1, G. Orttner 1, O. Chasselat 1, K. Wong 1, L. Prech 2,

ELECTRON FLUXES AT 650 KM ALTITUDE (200 keV)

Electron interaction with VLF

NWC

Page 6: IDEE, The Electron Spectrometer for the Taranis Mission J.-A. Sauvaud 1, P. Devoto, A. Fedorov 1, G. Orttner 1, O. Chasselat 1, K. Wong 1, L. Prech 2,

‘Cyclotron’ induced structures

Sauvaud et al., 2008

Effect of VLF transmitter 19.8 kHz

Note the large difference of slopes in the inner belt as compared to the ‘cyclotron slope’

Page 7: IDEE, The Electron Spectrometer for the Taranis Mission J.-A. Sauvaud 1, P. Devoto, A. Fedorov 1, G. Orttner 1, O. Chasselat 1, K. Wong 1, L. Prech 2,

Electrons Protons

Drift resonance: ULF-particle INTERACTIONS

Page 8: IDEE, The Electron Spectrometer for the Taranis Mission J.-A. Sauvaud 1, P. Devoto, A. Fedorov 1, G. Orttner 1, O. Chasselat 1, K. Wong 1, L. Prech 2,

LIGHTENING ELECTRON PRECIPITATION / VLF-ELECTRON INTERACTION

2 s

Voss et al, Nature, 1984.

Page 9: IDEE, The Electron Spectrometer for the Taranis Mission J.-A. Sauvaud 1, P. Devoto, A. Fedorov 1, G. Orttner 1, O. Chasselat 1, K. Wong 1, L. Prech 2,
Page 10: IDEE, The Electron Spectrometer for the Taranis Mission J.-A. Sauvaud 1, P. Devoto, A. Fedorov 1, G. Orttner 1, O. Chasselat 1, K. Wong 1, L. Prech 2,

Lightning induced electron precipitation (DEMETER - above Europe: weak energy, critical time resolution of electron data )

DEMETER

Page 11: IDEE, The Electron Spectrometer for the Taranis Mission J.-A. Sauvaud 1, P. Devoto, A. Fedorov 1, G. Orttner 1, O. Chasselat 1, K. Wong 1, L. Prech 2,
Page 12: IDEE, The Electron Spectrometer for the Taranis Mission J.-A. Sauvaud 1, P. Devoto, A. Fedorov 1, G. Orttner 1, O. Chasselat 1, K. Wong 1, L. Prech 2,

Distribution of lightnings, winter 2008-2009

Page 13: IDEE, The Electron Spectrometer for the Taranis Mission J.-A. Sauvaud 1, P. Devoto, A. Fedorov 1, G. Orttner 1, O. Chasselat 1, K. Wong 1, L. Prech 2,

ELECTRONS

Page 14: IDEE, The Electron Spectrometer for the Taranis Mission J.-A. Sauvaud 1, P. Devoto, A. Fedorov 1, G. Orttner 1, O. Chasselat 1, K. Wong 1, L. Prech 2,

Terrestrial gamma flashes energy spectrum

RHESSI10 msec

Parent electrons:dJ/dE=2.2 10-3 exp(-E/7.2)

TGF

Υ spectrum

Page 15: IDEE, The Electron Spectrometer for the Taranis Mission J.-A. Sauvaud 1, P. Devoto, A. Fedorov 1, G. Orttner 1, O. Chasselat 1, K. Wong 1, L. Prech 2,

Computed TGF Electrons

Lehtinen et al., 2010; Carlson et al., 2011

Page 16: IDEE, The Electron Spectrometer for the Taranis Mission J.-A. Sauvaud 1, P. Devoto, A. Fedorov 1, G. Orttner 1, O. Chasselat 1, K. Wong 1, L. Prech 2,

Carlson et al., 2011

Page 17: IDEE, The Electron Spectrometer for the Taranis Mission J.-A. Sauvaud 1, P. Devoto, A. Fedorov 1, G. Orttner 1, O. Chasselat 1, K. Wong 1, L. Prech 2,

SAMPEX electron bursts possibly related to TGF

Lehtinen et al.

Page 18: IDEE, The Electron Spectrometer for the Taranis Mission J.-A. Sauvaud 1, P. Devoto, A. Fedorov 1, G. Orttner 1, O. Chasselat 1, K. Wong 1, L. Prech 2,

DEMETERRRE

Part

/(cm

2.s.

sr.k

eV)

Electron fluxes

Expected TGF electrons

The electrons that escape to satellie altitude are most likely secondary electrons produced by TGF

Page 19: IDEE, The Electron Spectrometer for the Taranis Mission J.-A. Sauvaud 1, P. Devoto, A. Fedorov 1, G. Orttner 1, O. Chasselat 1, K. Wong 1, L. Prech 2,

Can a detector like IDP

(DEMETER) do that?

Relativistic Runaway Electrons (RRE) Not enough Geometrical Factor

Lightning-induced Electron Precipitation (LEP)Time resolution not adequate

Pitch-angle Distribution of Radiation Belt Electrons No angular channels

Page 20: IDEE, The Electron Spectrometer for the Taranis Mission J.-A. Sauvaud 1, P. Devoto, A. Fedorov 1, G. Orttner 1, O. Chasselat 1, K. Wong 1, L. Prech 2,

The resulting IDEE sensor for TARANIS

Page 21: IDEE, The Electron Spectrometer for the Taranis Mission J.-A. Sauvaud 1, P. Devoto, A. Fedorov 1, G. Orttner 1, O. Chasselat 1, K. Wong 1, L. Prech 2,

IDEE

2 detector planes: Si + CdTe (coincidence for direction), large section of CdTe for RRE

Page 22: IDEE, The Electron Spectrometer for the Taranis Mission J.-A. Sauvaud 1, P. Devoto, A. Fedorov 1, G. Orttner 1, O. Chasselat 1, K. Wong 1, L. Prech 2,

ADDING SEPARATION INTO THE COLLIMATOR = angular separation of low energy electrons

Page 23: IDEE, The Electron Spectrometer for the Taranis Mission J.-A. Sauvaud 1, P. Devoto, A. Fedorov 1, G. Orttner 1, O. Chasselat 1, K. Wong 1, L. Prech 2,
Page 24: IDEE, The Electron Spectrometer for the Taranis Mission J.-A. Sauvaud 1, P. Devoto, A. Fedorov 1, G. Orttner 1, O. Chasselat 1, K. Wong 1, L. Prech 2,
Page 25: IDEE, The Electron Spectrometer for the Taranis Mission J.-A. Sauvaud 1, P. Devoto, A. Fedorov 1, G. Orttner 1, O. Chasselat 1, K. Wong 1, L. Prech 2,
Page 26: IDEE, The Electron Spectrometer for the Taranis Mission J.-A. Sauvaud 1, P. Devoto, A. Fedorov 1, G. Orttner 1, O. Chasselat 1, K. Wong 1, L. Prech 2,

Objectif - Runaway Relativistic Electrons

Possible RRE spectrum (Red)

Where we can distinguish a RRE spectrum from the bkg electrons.

(After DEMETER data)

Page 27: IDEE, The Electron Spectrometer for the Taranis Mission J.-A. Sauvaud 1, P. Devoto, A. Fedorov 1, G. Orttner 1, O. Chasselat 1, K. Wong 1, L. Prech 2,

Runaway Relativistic Electrons

Possible RRE spectrum (Red)Detection of RRE8 horizontal bands, 8 CdTe cells in eachthickness 6mm to stop electrons up to 4 Mev

Page 28: IDEE, The Electron Spectrometer for the Taranis Mission J.-A. Sauvaud 1, P. Devoto, A. Fedorov 1, G. Orttner 1, O. Chasselat 1, K. Wong 1, L. Prech 2,

IDEE-TARANIS

Page 29: IDEE, The Electron Spectrometer for the Taranis Mission J.-A. Sauvaud 1, P. Devoto, A. Fedorov 1, G. Orttner 1, O. Chasselat 1, K. Wong 1, L. Prech 2,

IDEE

Page 30: IDEE, The Electron Spectrometer for the Taranis Mission J.-A. Sauvaud 1, P. Devoto, A. Fedorov 1, G. Orttner 1, O. Chasselat 1, K. Wong 1, L. Prech 2,
Page 31: IDEE, The Electron Spectrometer for the Taranis Mission J.-A. Sauvaud 1, P. Devoto, A. Fedorov 1, G. Orttner 1, O. Chasselat 1, K. Wong 1, L. Prech 2,
Page 32: IDEE, The Electron Spectrometer for the Taranis Mission J.-A. Sauvaud 1, P. Devoto, A. Fedorov 1, G. Orttner 1, O. Chasselat 1, K. Wong 1, L. Prech 2,

CdTe

Page 33: IDEE, The Electron Spectrometer for the Taranis Mission J.-A. Sauvaud 1, P. Devoto, A. Fedorov 1, G. Orttner 1, O. Chasselat 1, K. Wong 1, L. Prech 2,

CdTe

Page 34: IDEE, The Electron Spectrometer for the Taranis Mission J.-A. Sauvaud 1, P. Devoto, A. Fedorov 1, G. Orttner 1, O. Chasselat 1, K. Wong 1, L. Prech 2,

Response to RRE event

Geant-4 simulation20 counts/event

Measurable signalfor CdTe only

Page 35: IDEE, The Electron Spectrometer for the Taranis Mission J.-A. Sauvaud 1, P. Devoto, A. Fedorov 1, G. Orttner 1, O. Chasselat 1, K. Wong 1, L. Prech 2,

Response to associated Gamma rays

Geant-4 simulation

when gamma onlyare received, the measured signal isvery weak.

Gammas will notdisturbed electronmeasurements.

Page 36: IDEE, The Electron Spectrometer for the Taranis Mission J.-A. Sauvaud 1, P. Devoto, A. Fedorov 1, G. Orttner 1, O. Chasselat 1, K. Wong 1, L. Prech 2,

STATUS OF THE EXPERIMENT

Sensor head design: performed

Electronic design: performed. ASIC developedDPU: performed (Charles university)

Modes: defined

Burst trigger: ready

Thermal study: made

EQM: made