Book contents
- Frontmatter
- Contents
- List of contributors
- Preface
- 1 X-ray polarimetry: historical remarks and other considerations
- Part I Polarimetry techniques
- 2 Scattering polarimetry in high-energy astronomy
- 3 Photoelectric polarimeters
- 4 Bragg crystal polarimeters
- 5 X-ray polarimetry with the photon-counting pixel detector Timepix
- 6 High-energy polarized photon interactions with matter: simulations with Geant4
- 7 The GPD as a polarimeter: theory and facts
- 8 Ideal gas electron multipliers (GEMs) for X-ray polarimeters
- 9 Broad-band soft X-ray polarimetry
- 10 Feasibility of X-ray photoelectric polarimeters with large field of view
- 11 Angular resolution of a photoelectric polarimeter
- 12 Development of a Thomson X-ray polarimeter
- 13 Hard X-ray / soft gamma-ray polarimetry using a Laue lens
- Part II Polarized emission in X-ray sources
- Part III Future missions
- Author index
- Subject index
8 - Ideal gas electron multipliers (GEMs) for X-ray polarimeters
from Part I - Polarimetry techniques
Published online by Cambridge University Press: 06 July 2010
- Frontmatter
- Contents
- List of contributors
- Preface
- 1 X-ray polarimetry: historical remarks and other considerations
- Part I Polarimetry techniques
- 2 Scattering polarimetry in high-energy astronomy
- 3 Photoelectric polarimeters
- 4 Bragg crystal polarimeters
- 5 X-ray polarimetry with the photon-counting pixel detector Timepix
- 6 High-energy polarized photon interactions with matter: simulations with Geant4
- 7 The GPD as a polarimeter: theory and facts
- 8 Ideal gas electron multipliers (GEMs) for X-ray polarimeters
- 9 Broad-band soft X-ray polarimetry
- 10 Feasibility of X-ray photoelectric polarimeters with large field of view
- 11 Angular resolution of a photoelectric polarimeter
- 12 Development of a Thomson X-ray polarimeter
- 13 Hard X-ray / soft gamma-ray polarimetry using a Laue lens
- Part II Polarized emission in X-ray sources
- Part III Future missions
- Author index
- Subject index
Summary
We have developed gas electron multipliers (GEMs) for space science applications, in particular for X-ray polarimeters. We have employed a laser etching technique instead of the standard wet etching for the GEM production. Our GEMs showed no gain increase after applying high voltage and kept the gain for more than two weeks at a level of 2% (RMS). We show the gain properties and the results of some acceleration tests to mimic a two-years low-Earth-orbit operation in this paper.
Introduction
The GEM is one of the recently developed micro-pattern gas detectors. A dense pattern of through-holes is drilled in an insulator substrate, which is typically polyimide, sandwiched by thin copper foils. The surface and cross-section micrographs of a GEM are shown in Figure 8.1. When high voltage is applied to the copper electrodes in an appropriate gas, the GEM works as an electron multiplier. GEMs are used in many fields such as high energy and nuclear physics, X-ray imaging, etc. In astrophysics, photoelectric X-ray polarimeters, in which the GEM is a key device to multiply an electron cloud whilst retaining its shape, are the most interesting application.
We have produced GEMs since 2002 for X-ray polarimeters. The standard method to produce GEMs is a wet etching technique, while our method is laser etching, which has many advantages. Cylindrical holes are easily formed with the laser etching. The capability to drill cylindrical holes helps in forming finer-pitch holes on a thicker substrate.
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- Information
- X-ray PolarimetryA New Window in Astrophysics, pp. 60 - 65Publisher: Cambridge University PressPrint publication year: 2010