Abstract | AdityaL1 is India’s first space solar mission with a suite of seven payloads to study the solar
dynamics. Visible Emission Line Coronagraph (VELC) on Aditya(L1) is an internally occulted solar
coronagraph with simultaneous imaging, spectroscopy and spectro-polarimetry channels close to the
solar limb. The primary science goals of this mission are (1) Diagnostics of the coronal and coronal
loops plasma (Temperature, Velocity, & Density), (2) Heating of the corona, (3) Development,
dynamics & origin of CME's, (4) Studies on the drivers for space weather and (5) Measurement of
coronal magnetic fields in the corona (not planned by any mission so far). VELC is designed to
image solar corona and multi-slit spectroscopic channels at three emission lines namely 530.3nm,
789.2nm and 1074.7nm. It has dual-beam spectro-polarimetry at 1074.7nm for magnetic field
measurements. The stringent demands on design, realization of subsystems, integration and finally
the calibration challenges will be discussed in this talk. |