/
Gamma-ray imager/ Gamma-ray imager/

Gamma-ray imager/ - PowerPoint Presentation

lindy-dunigan
lindy-dunigan . @lindy-dunigan
Follow
389 views
Uploaded On 2016-04-30

Gamma-ray imager/ - PPT Presentation

polarimeter concept based on GRIPS Albert Y Shih NASAGSFC on behalf of the GRIPS team Measurements and science objectives Angular resolution of 5 arcsec up to 22 MeV Spatial separation between ionassociated and electronassociated emission ID: 299844

instrument resolution minimum imaging resolution instrument imaging minimum angular mev kev grips detectable 511 polarimetry line pitch function response

Share:

Link:

Embed:

Download Presentation from below link

Download Presentation The PPT/PDF document "Gamma-ray imager/" is the property of its rightful owner. Permission is granted to download and print the materials on this web site for personal, non-commercial use only, and to display it on your personal computer provided you do not modify the materials and that you retain all copyright notices contained in the materials. By downloading content from our website, you accept the terms of this agreement.


Presentation Transcript

Slide1

Gamma-ray imager/polarimeter concept based on GRIPS

Albert Y.

Shih (NASA/GSFC)

on behalf of the

GRIPS

teamSlide2

Measurements and science objectives

Angular resolution of ~5

arcsec

up to 2.2

MeV

Spatial separation between ion-associated and electron-associated emission

Clean point-response function

Source sizes and shapes

Multiple sources needing high dynamic range

Minimum

detectable polarization of ~1% in

a large flare

, also imaging

polarimetry

Pitch-angle distribution of relativistic electrons

Albedo

Spectral resolution of <~0.5% FWHM

Accelerated abundances and ion angular distributions

Atmospheric conditions from 511

keV

lineSlide3

Instrument technologies3D position-sensitive germanium detectors (3D-GeDs) developed by LBNL

Locate to within <0.1 mm

3

Compton-scatter track reconstruction

Multi-pitch rotating modulator (MPRM)

2-cm thick tungsten

Functions like RMC or coded-mask imaging

Photo of two

NCT

detectors(7.5 cm × 7.5 cm × 1.5 cm)

Illustration of the MPRMSlide4

Instrument concept

Compact arrangement of 3D-GeDs in one or more cryostats

16 in a 2×2×4 configuration

(same as

GRIPS

balloon instrument)

64 in a 4×4×4 configurationRegular annealing to preserve resolution and line shape?

Individual photon tagging, >5 GB/dayScintillator-based anti-coincidence shieldIn addition to background

rejection via Compton imaging20-meter boom with loose requirements on pointing/stability

Or formation flying?Illustration of a 20-meter boomSlide5

Instrument capabilities

5” minimum angular resolution (compared to 35” with

RHESSI

)

Point-response function virtually free of

sidelobes

~1% minimum detectable polarization at 150–650 keV3 keV to >~10

MeV, resolution of 1.8 keV at 662 keVSimultaneous imaging,

polarimetry, and spectroscopy

Energy (MeV)Effective area, spectroscopy (cm2)

Effective area, imaging (cm

2

)

GRIPS

RHESSI

GRIPS

RHESSI

0.511~15039~966.02.223~5222~253.34.4~2711~51.7

4×4×4 configuration