GRAPE: a balloon-borne gamma-ray polarimeter

The Gamma-RAy Polarimeter Experiment (GRAPE) is a concept for an astronomical hard X-ray Compton polarimeter operating in the 50 - 500 keV energy band. The instrument has been optimized for wide-field polarization measurements of transient outbursts from energetic astrophysical objects such as gamma-ray bursts and solar flares. The GRAPE instrument is composed of identical modules, each of which consists of an array of scintillator elements read out by a multi-anode photomultiplier tube (MAPMT). Incident photons Compton scatter in plastic scintillator elements and are subsequently absorbed in inorganic scintillator elements; a net polarization signal is revealed by a characteristic asymmetry in the azimuthal scattering angles. We have constructed a prototype GRAPE module that has been calibrated at a polarized hard X-ray beam and flown on an engineering balloon test flight. A full-scale scientific balloon payload, consisting of up to 36 modules, is currently under development. The first flight, a one-day flight scheduled for 2011, will verify the expected scientific performance with a pointed observation of the Crab Nebula. We will then propose long-duration balloon flights to observe gamma-ray bursts and solar flares.

[1]  Huang Yong-feng,et al.  2008 Nanjing Gamma-Ray Burst Conference , 2008 .

[2]  Prospects for GRB Polarimetry with GRAPE , 2006 .

[3]  T. Sakamoto,et al.  POET: POlarimeters for Energetic Transients , 2008, 0810.2499.

[4]  James M. Ryan,et al.  Development of a hard X-ray polarimeter for astrophysics , 1998, 1998 IEEE Nuclear Science Symposium Conference Record. 1998 IEEE Nuclear Science Symposium and Medical Imaging Conference (Cat. No.98CH36255).

[5]  James M. Ryan,et al.  A Modular Hard X-Ray Polarimeter for Solar Flares , 2000 .

[6]  F. Lei,et al.  Compton Polarimetry in Gamma-Ray Astronomy , 1997 .

[7]  Nicolas Produit,et al.  GRB polarimetry with POET , 2008 .

[8]  James M. Ryan,et al.  A Polarimeter for Studying Hard X-Rays from Solar Flares , 1999 .

[9]  A. Stepanov,et al.  Hard X-ray Radiation from Solar Flares in the Second Half of 2001: Preliminary Results of the SPR-N Experiment Onboard the Coronas-F Satellite , 2003 .

[10]  James M. Ryan,et al.  A Balloon‐Borne Gamma‐Ray Polarimeter for Gamma‐Ray Bursts , 2009 .

[11]  J. Stephen,et al.  Polarized Gamma-Ray Emission from the Crab , 2008, Science.

[12]  Mark L. McConnell,et al.  Developing a Compton polarimeter to measure polarization of hard x-rays in the 50-300 keV energy range , 2005, SPIE Optics + Photonics.

[13]  Robert Novick,et al.  Stellar and solar X-ray polarimetry , 1981 .

[14]  James M. Ryan,et al.  Development of a hard x-ray polarimeter for gamma-ray bursts , 1998 .

[15]  James M. Ryan,et al.  The Development of GRAPE, a Gamma Ray Polarimeter Experiment , 2003 .

[16]  Reuven Ramaty,et al.  Backscatter, anisotropy, and polarization of solar hard X-rays , 1978 .

[17]  K. C. Chandler,et al.  Calculations of neutron flux spectra induced in the Earth's atmosphere by galactic cosmic rays , 1973 .

[18]  Mark L. McConnell,et al.  Dedicated polarimeter design for hard x-ray and soft gamma-ray astronomy , 2004, SPIE Optics + Photonics.

[19]  P. F. Bloser,et al.  Calibration of the Gamma-RAy Polarimeter Experiment (GRAPE) at a polarized hard X-ray beam , 2009 .

[20]  Bing Zhang Gamma-Ray Bursts in the Swift Era , 2007, astro-ph/0701520.

[21]  Chris R. Shrader,et al.  MGEANT—A GEANT-based multi-purpose simulation package for gamma-ray astronomy missions , 2000 .

[22]  Mark L. McConnell,et al.  Hard x-ray polarimeter for gamma-ray bursts and solar flares , 2003, SPIE Astronomical Telescopes + Instrumentation.

[23]  W. H. McMaster,et al.  MATRIX REPRESENTATION OF POLARIZATION , 1961 .

[24]  Gordon D. Holman,et al.  Electron Bremsstrahlung Hard X-Ray Spectra, Electron Distributions, and Energetics in the 2002 July 23 Solar Flare , 2003 .

[25]  T. Narita,et al.  A hard X-ray polarimeter designed for transient astrophysical sources , 2005, IEEE Nuclear Science Symposium Conference Record, 2005.

[26]  J. Leach,et al.  The impulsive phase of solar flares. II - Characteristics of the hard X-rays , 1983 .

[27]  James M. Ryan,et al.  Development of a hard X-ray polarimeter for solar flares and gamma-ray bursts , 1997 .

[28]  S. Boggs,et al.  Polarization of the prompt γ-ray emission from the γ-ray burst of 6 December 2002 , 2003, Nature.

[29]  Neil Gehrels,et al.  GAMMA-RAY BURST: Sixth Huntsville Symposium , 2009 .

[30]  C. Wunderer,et al.  Testing Lorentz Invariance with GRB 021206 , 2003, astro-ph/0310307.

[31]  N. Gehrels,et al.  Instrumental background in balloon-borne gamma-ray spectrometers and techniques for its reduction , 1985 .

[32]  I. Grenier,et al.  Polarization of the Crab Pulsar and Nebula as Observed by the INTEGRAL/IBIS Telescope , 2008, 0809.1292.

[33]  M. McConnell,et al.  RHESSI as a Hard X-Ray Polarimeter , 2002, astro-ph/0209384.

[34]  P. F. Bloser,et al.  GRAPE - A Balloon-Borne Gamma-Ray Polarimeter Experiment , 2006 .

[35]  A. Hanslmeier,et al.  Does solar flare activity lag behind sunspot activity? , 2003 .

[36]  Mark L. McConnell,et al.  Recent laboratory tests of a hard x-ray solar flare polarimeter , 1999, Optics & Photonics.

[37]  Martin H. Israel,et al.  FiberGLAST: a scintillating fiber approach to the GLAST mission , 1999, Optics & Photonics.

[38]  Ralf S. Klessen,et al.  American Institute of Physics Conference Series , 2010 .