Imaging TGFs and GRBs from the earth rim mounting of the ASIM/MXGS imager-spectrometer on the ISS
- University of Valencia, Image Processing Laboratory, Astronomy and Space Physics, Valencia, Spain (paul.connell@uv.es)
On January 10th 2022 the ASIM mission to the ISS was moved to the SDN mount point on the Columbus module for observations towards the earth rim and the cosmos. This enabled the ASIM/MXGS imager spectrometer to observe TGFs in a small ISS nadir FOV covering 35-65 degrees off-axis, and GRBs in the cosmos which covers most of its FOV. We present here initial results of imaging locations for off-axis TGFs with a low spectral hardness ratio and a much larger event count due to the reduction in the "flux cosine effect", and how this might facilitate estimates of mean TGF altitude. We also present the first MXGS location images of second long GRBs and their associated lightcurves and spectra.
How to cite: Connell, P., Reglero, V., Navarro, J., and Eyles, C.: Imaging TGFs and GRBs from the earth rim mounting of the ASIM/MXGS imager-spectrometer on the ISS, EGU General Assembly 2022, Vienna, Austria, 23–27 May 2022, EGU22-3037, https://doi.org/10.5194/egusphere-egu22-3037, 2022.
