Abstract
Using polarimetry as a tool to study processes and objects emitting high-energy photons was until now rather uncommon. Recent satellite measurements have proved the high power of polarization observables and initiated a rapid development of new instruments. We describe the physical mechanisms leading to photon polarization, and discuss the processes used for its detection at energies from few kiloelectronvolts X-rays up to megaelectronvolts gamma-rays. Past instrumentation and pioneer attempts of polarization measurements are summarized and reviewed with respect to experimental difficulties and scientific achievements. We also present current and planned polarimeters and the utilization of novel, energy-specific detection technologies. Finally, we discuss the importance of proper modelling and calibration of the polarimeter, and describe several methods used to characterize it.
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Hajdas, W., Suarez-Garcia, E. (2013). Polarimetry at high energies. In: Huber, M.C.E., Pauluhn, A., Culhane, J.L., Timothy, J.G., Wilhelm, K., Zehnder, A. (eds) Observing Photons in Space. ISSI Scientific Report Series, vol 9. Springer, New York, NY. https://doi.org/10.1007/978-1-4614-7804-1_34
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DOI: https://doi.org/10.1007/978-1-4614-7804-1_34
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