- Visible Emission Line Coronagraph (VELC): It can peek as close as 1.05 solar radii, a region never imaged by any solar telescope. It can thus give us more information about CMEs.
- Solar Ultraviolet Imaging Telescope (SUIT): It will observe UV radiations from different zones of the solar atmosphere. It will help us to better understand the climate variation on earth.
- Solar Low Energy X-Ray Spectrometer (SoLEXS)
- High Energy L1 Orbiting X-Ray Spectrometer (HEL1OS)
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- Aditya Solar Particle Experiment (ASPEX): In-situ measurements of solar particles & ions.
- Plasma Analyzer Package for Aditya (PAPA)
- Advanced Tri-axial High Resolution Digital Magnetometers
- With ASPEX, PAPA, and ATHRDM scientists can predict probable geomagnetic storms and better understand space weather dynamics.
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