Abstract
This paper reviews the development status of GRAPE (the Gamma-Ray Polarimeter Experiment), a hard X-ray Compton Polarimeter. The purpose of GRAPE is to measure the polarization of hard X-rays in the 50-300 keV energy range. We are particularly interested in X-rays that are emitted from solar flares and gamma-ray bursts (GRBs), although GRAPE could also be employed in the study of other astrophysical sources. Accurately measuring the polarization of the emitted radiation will lead to a better understating of both emission mechanisms and source geometries. The GRAPE design consists of an array of plastic scintillators surrounding a central high-z crystal scintillator. The azimuthal distribution of photon scatters from the plastic array into the central calorimeter provides a measure of the polarization fraction and polarization angle of the incident radiation. The design of the detector provides sensitivity over a large field-of-view (> π steradian). The design facilitates the fabrication of large area arrays with minimal deadspace. This paper presents the latest design concept and the most recent results from laboratory tests of a GRAPE science model.
Author supplied keywords
Cite
CITATION STYLE
Bloser, P. F., Legere, J. S., Macri, J. R., McConnell, M. L., Narita, T., & Ryan, J. M. (2006). GRAPE - A balloon-borne gamma-ray polarimeter experiment. In Chinese Journal of Astronomy and Astrophysics (Vol. 6, pp. 393–397). Institute of Physics Publishing. https://doi.org/10.1088/1009-9271/6/S1/54
Register to see more suggestions
Mendeley helps you to discover research relevant for your work.