Exploring the Capabilities of the Anti-Coincidence Shield of the International Gamma-Ray Astrophysics Laboratory (INTEGRAL) Spectrometer to Study Solar Flares

@article{RodrguezGasn2014ExploringTC,
  title={Exploring the Capabilities of the Anti-Coincidence Shield of the International Gamma-Ray Astrophysics Laboratory (INTEGRAL) Spectrometer to Study Solar Flares},
  author={R. Rodr{\'i}guez-Gas{\'e}n and J. Kiener and V. Tatischeff and N. Vilmer and C. Hamadache and K. Klein},
  journal={Solar Physics},
  year={2014},
  volume={289},
  pages={1625-1641}
}
The International Gamma-Ray Astrophysics Laboratory (INTEGRAL) is a European Space Agency hard X-ray/γ-ray observatory for astrophysics, covering photon energies from 15 keV to 10 MeV. It was launched in 2002, and since then the Bismuth Germanate (BGO) detectors of the Anti-Coincidence Shield (ACS) of the Spectrometer on INTEGRAL (SPI) have detected many hard X-ray (HXR) bursts from the Sun, producing light curves at photon energies above ≈ 100 keV. The spacecraft has a highly elliptical orbit… Expand

References

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The INTEGRAL mission
SPI: The spectrometer aboard INTEGRAL
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