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IDEE, The Electron Spectrometer of the Taranis Mission
J.-A. Sauvaud1, A. Fedorov1, P. Devoto1, C. Jacquey1,
L. Prech2, Z. Nemecek2, F. Lefeuvre3
1 CESR-U. Of Toulouse-CNRS
2 Charles University, Prague
3 LPCE, CNRS, Orléans
Workshop on Coupling of Thunderstorms and Lightning Discharges to Near-Earth Space 23-27 June 2008, Corte, France
Charged particle
W= 3.5 eV/e--hole pair
The spectrometer uses semi-conductors as particle detectorsThe spectrometer uses semi-conductors as particle detectors(an electron crossing a semi-conductor generate pairs of e-holes. A pair is (an electron crossing a semi-conductor generate pairs of e-holes. A pair is produced for each 3.5 eV lost. The energy lost is measured) produced for each 3.5 eV lost. The energy lost is measured)
PARTICLE ENVIRONMENT AT 700 KM ALTITUDEPARTICLE ENVIRONMENT AT 700 KM ALTITUDE(200 keV)(200 keV)
DEMETER DATA
IDEE conceptionIDEE conception
3 objectives:3 objectives:
-Pitch-angle Distribution of Radiation Belt Electrons
-Relativistic Runaway Electrons (RRE)
-Lightning-induced Electron Precipitation (LEP)
Can IDP (DEMETER) do that?Can IDP (DEMETER) do that?
Relativistic Runaway Electrons (RRE) Not enough Geometrical Factor
Lightning-induced Electron Precipitation (LEP) Energy range and time resolution not adequate
Pitch-angle Distribution of Radiation Belt Electrons No angular channels
Two spectrometers, 735 cmTwo spectrometers, 735 cm33 each eachOne looking upward, the other downwardOne looking upward, the other downward
IDEE TARANISIDEE TARANIS
Silicon matrix Energy range : 70 keV – 350 keV
CdTe matrix Energy range : 350 keV – 4 MeV
Objectif - Runaway Relativistic Objectif - Runaway Relativistic ElectronsElectrons
Possible RRE spectrum (Red)
Where we can distinguish a RRE spectrum from the bkg electrons.
(After DEMETER data)
Runaway Relativistic ElectronsRunaway Relativistic Electrons
Possible RRE spectrum (Red)Detection of RRE8 horizontal bands, 8 CdTe cells in eachthickness 6mm to stop electrons up to 4 Mev
Runaway Relativistic ElectronsRunaway Relativistic Electrons
Possible RRE spectrum (Red)An Al foil (0.65mm width) protects thesensor from low energy particles
Runaway Relativistic ElectronsRunaway Relativistic Electrons
CdTe detector Geometrical FactorGEANT-4 simulation with real design
An Al foil (0.65mm) protects the sensor From low energy particles
Objectif - Lightning induced electron precipitation Objectif - Lightning induced electron precipitation (DEMETER - above Europe: weak energy, critical time resolution of electron data )(DEMETER - above Europe: weak energy, critical time resolution of electron data )
DEMETERDEMETER
Lightning-induced Electron PrecipitationLightning-induced Electron Precipitation
Example of LEP measurements E = 30 - 200keV
A Si detector is located ahead of the CdTeto measure moderate fluxes and (weak) energies of precipitated electrons. Expected flux: 8 104 s-1 in 200 ms bursts
Radiation belt detector: Si central cellRadiation belt detector: Si central cell
For strong fluxes of radiation belt electrons, the only central part of the silicium is used.
Can we provide measurements at high latitudes?Can we provide measurements at high latitudes?
Demeter electron flux
Geant-4 simulations
Can we provide measurements in high latitude regions?Can we provide measurements in high latitude regions?
Yes, we can
Spectrometersimulation
Spectra providedby the Si centralcell and by thecentral cell in Coincidence withCdTe are not saturated
Response to RRE eventResponse to RRE event
Geant-4 simulation20 counts/event
Measurable signalfor CdTe only
Expected response to RRE eventExpected response to RRE event
Geant-4 simulation20 counts/event
Time profile ofmodeled fluxduring an event ,Noise below 1 count/5ms ( < 200)
CdTe
Response to associated Gamma raysResponse to associated Gamma rays
Geant-4 simulation
when gamma onlyare received, the measured signal isvery weak.
Gammas will notdisturbed electronmeasurements.