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The Aditya-L1 mission, aimed at studying the Sun from an orbit around the L1, would carry seven payloads to observe the photosphere, chromosphere and the outermost layers of the Sun, the corona, in different wavebands. Aditya-L1 is a fully indigenous effort with the participation of national institutions, an ISRO official said.
The Bengaluru-based Indian Institute of Astrophysics (IIA) is the lead institute for the development of Visible Emission Line Coronagraph payload. While Inter-University Centre for Astronomy and Astrophysics, Pune, has developed the Solar Ultraviolet Imager payload for the mission. Aditya-L1 can provide observations on the corona, and on the solar Chromosphere using the UV payload and on the flares using the X-ray payloads. The particle detectors and the magnetometer payload can provide information on charged particles and the magnetic field reaching the halo orbit around L1. The satellite, realised at U R Rao Satellite Centre here, arrived at the ISRO’s spaceport of Sriharikota in Andhra Pradesh, two weeks ago. ”Most likely the launch will take place on September 2 ”, an ISRO official said.
The spacecraft is planned to be placed in a halo orbit around the L1 of the Sun-Earth system. A satellite placed in the halo orbit around the L1 point has the major advantage of continuously viewing the Sun without any occultation/eclipses, ISRO noted. ”This will provide a greater advantage of observing the solar activities and its effect on space weather in real time,” it said. Using the special vantage point L1, four payloads directly view the Sun and the remaining three payloads carry out in-situ studies of particles and fields at the L1, thus providing important scientific studies of the propagatory effect of solar dynamics in the interplanetary medium.
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They also include Physics of solar corona and its heating mechanism; Diagnostics of the coronal and coronal loops plasma: Temperature, velocity and density; Development, dynamics and origin of CMEs; Identify the sequence of processes that occur at multiple layers (chromosphere, base and extended corona) which eventually leads to solar eruptive events; Magnetic field topology and magnetic field measurements in the solar corona; Drivers for space weather (origin, composition and dynamics of solar wind.
The instruments of Aditya-L1 are tuned to observe the solar atmosphere, mainly the chromosphere and corona. In-situ instruments will observe the local environment at L1.