Astronomy:Compton telescope
A Compton telescope (also known as Compton camera or Compton imager) is a gamma-ray detector which utilizes Compton scattering to determine the origin of the observed gamma rays.[1][2]
Compton cameras are usually applied to detect gamma rays in the energy range where Compton scattering is the dominating interaction process, from a few hundred keV to several MeV. They are applied in fields such as astrophysics, nuclear medicine, and nuclear threat detection.
Principle of operation
The Compton telescope consists of two layers of Compton scattering detectors spaced apart (1.5m in the case of COMPTEL). A Compton scattering event results in an electron and a photon. Each layer detects the position of a event and the energy of an electron resulting from the Compton event. In addition, the time between events in the upper and lower layers is measured. When the time between two events matches the time it takes for the photon to travel from the upper to lower level, the events are accepted for a image. The direction of the original gamma ray is unknown but the angle of the second photon and the energies of the two electrons allow the angle between the first and second photons to be calculated. Thus each event gives a cone of possible sources for the first photon. After many events are added the overlap of their cones gives the source direction.[3]
Astrophysics missions
The COMPTEL aboard the Compton Gamma Ray Observatory observed of the gamma-ray sky in the energy range between 0.75 and 30 MeV between its launch in April 1991 and intensional deorbit in June 2000.[4][5] Among the results was a detailed study of the Crab pulsar.[6]
A successor mission, the balloon-borne Nuclear Compton Telescope, flew a successful run in 2005. It provided a gamma-ray based image of the Crab pulsar.[7]
References
- ↑ "Compton Telescope" (in en-US). 2016-03-12. https://cosi.ssl.berkeley.edu/instrument/design/.
- ↑ "Global Astronomy: Collaboration Across Cultures". https://imagine.gsfc.nasa.gov/observatories/learning/globalastro/p2373.html.
- ↑ Schoenfelder, V.; Aarts, H.; Bennett, K.; de Boer, H.; Clear, J.; Collmar, W.; Connors, A.; Deerenberg, A. et al. (June 1993). "Instrument Description and Performance of the Imaging Gamma-Ray Telescope COMPTEL aboard the Compton Gamma-Ray Observatory" (in en). The Astrophysical Journal Supplement Series 86: 657. doi:10.1086/191794. ISSN 0067-0049. https://ui.adsabs.harvard.edu/abs/1993ApJS...86..657S/abstract.
- ↑ Mrozinski, Richard B. (June 2001). "Entry Debris Field estimation methods and application to Compton Gamma Ray Observatory". 2001 Flight Mechanics Symposium (Mission Operations Directorate Nasa Johnson Space Center). https://ntrs.nasa.gov/citations/20010084992.
- ↑ "MeV Compton gamma-ray telescope (COMPTEL) [CADE"]. http://cade.irap.omp.eu/dokuwiki/doku.php?id=comptel.
- ↑ Kuiper, L.; Hermsen, W.; Cusumano, G.; Diehl, R.; Schönfelder, V.; Strong, A.; Bennett, K.; McConnell, M. L. (2001-11-01). "The Crab pulsar in the 0.75-30 MeV range as seen by CGRO COMPTEL - A coherent high-energy picture from soft X-rays up to high-energy γ-rays" (in en). Astronomy & Astrophysics 378 (3): 918–935. doi:10.1051/0004-6361:20011256. ISSN 0004-6361. Bibcode: 2001A&A...378..918K. https://www.aanda.org/articles/aa/abs/2001/42/aah2543/aah2543.html.
- ↑ Bandstra, M. S.; Bellm, E. C.; Boggs, S. E.; Perez-Becker, D.; Zoglauer, A.; Chang, H.-K.; Chiu, J.-L.; Liang, J.-S. et al. (August 9, 2011). "DETECTION AND IMAGING OF THE CRAB NEBULA WITH THE NUCLEAR COMPTON TELESCOPE". The Astrophysical Journal 738 (1): 8. doi:10.1088/0004-637x/738/1/8. ISSN 0004-637X.
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