Centre d'Etude Spatiale
des Rayonnements
Département
Hautes-Energies
SIGMA detection
===============
Cosmic gamma radiation
~~~~~~~~~~~~~~~~~~~~~~
image:images/electro.spectrum.gif[width="600"]
* The cosmic gamma rays constitute the highest-energy domain of electromagnetic
spectrum. Gamma-ray photons emitted by celestial bodies are ten of thousand times
more energetic than photons of visible light.
* Visible light radiation has wavelength range from about 4000 angstroms
to 7000 angstroms. This corresponds to an energy of two or three electron
volts comparing to gamma-ray photons energy domain which starts at about 100 keV.
* The earth's atmosphere absorbs cosmic gamma radiation. So they can be studied
only in space.
Gamma-ray photons detection
~~~~~~~~~~~~~~~~~~~~~~~~~~~
* Because the wavelenths of gamma photons are smaller than the distances between
the atom matter, it is not possible to reflect and concentrate a beam of gamma
photons in lenses and mirrors as it can be done with visible light in traditional
optical telescopes.
* Gamma-ray photons can be detected by collecting electrons they create when
striking with detectors which are high density materials as sodium
iodide. Three major types of interaction play an important role in
radiation measurements and all these processes lead to the partial
or complete transfer of the gamma-ray photon energy to electron.
* The atomic number of the interaction medium and the energy of the gamma photon
have a strong influence on the relative probabilities of these three interactions :
** Photoelectric absorption predominates for low-energy gamma rays
(up to several tens keV) for the heaviest elements.
** Pair production predominates for high-energy gamma rays (above 5-10 MeV).
** Compton scattering is the most probable process over the range of energies between
these extremes.
SIGMA gamma-ray detectors
~~~~~~~~~~~~~~~~~~~~~~~~~
* The observational domain of the SIGMA telescope extends from high-energy X-rays
to low-energy gamma rays, in the energy range 35 keV to 1.3 MeV
* When a gamma photon enters the sodium iodide gamma-ray detector, it excites the
molecules and induces them to emit a flash of visible light.
* Sensitive light-detecting photomultiplier tubes detect that light and convert
it in an electric pulse. The height of the electric pulse is
proportional to the gamma photon energy in the sodium iodide
crystal.