4.1.1.5 Perform imaging spectroscopy of solar flares with 2.3
arcsec spatial resolution,
extending down to soft X-ray
(3 keV) energies.
4.1.1.6 Perform imaging spectroscopy of hard X-ray micro flares
with high sensitivity down to low
energies (3 keV).
4.1.1.7 Image hard X-rays of the Crab Nebula with 2.3 arcsec
resolution.
4.1.1.8 Obtain high spectral resolution observations of
transient hard
X-ray and gammaray sources,
including accreting black holes,
cosmic gamma-ray bursts, and
terrestrial bursts from trapped
energetic electron precipitation,
aurora, and lightning.
4.1.1.9 Perform imaging spectroscopy (> 3 keV) of high
temperature
components of solar active
regions.
4.1.1.10 Search for polarization of > 20 keV X-rays in solar
flares.
4.1.1.11 Perform spectroscopy of steady cosmic hard X-ray and
gamma-ray sources using Earth
occultation methods.