Our Sun is the nearest star and the largest object in the solar system. The estimated age of the sun is about 4.5 billion years. It is a hot, glowing ball of hydrogen and helium gases. The distance to the sun from the earth is about 150 million kilometers and is the source of energy for our solar system. Without the solar energy, the life on earth, as we know, can not exist. The gravity of the sun holds all the objects of the solar system together. At the central region of the sun, known as ‘core’, the temperature can reach as high as 15 million degree Celsius. At this temperature, a process called nuclear fusion takes place in the core, which powers the sun. The visible surface of the sun known as photosphere is relatively cool and has temperature of about 5,500°C
The sun is the nearest star and therefore can be studied in much more detail as compared to other stars By studying the sun we can learn much more about stars in our Milky Way as well as about stars in various other galaxies The sun is a very dynamic star that extends much beyond what we see. It shows several eruptive phenomena and releases immense amount of energy in the solar system. If such explosive solar phenomena was directed towards the earth, it could cause various types of disturbances in the near earth space environment Various spacecraft and communication systems are prone to such disturbances and therefore an early warning of such events is important for taking corrective measures beforehand In addition to these, if an astronaut is directly exposed to such explosive phenomena, he/she would be in danger The various thermal and magnetic phenomena on the sun are of extreme nature Thus, the sun also provides a good natural laboratory to understand those phenomena which cannot be directly studied in the lab
The sun constantly influences the Earth with radiation, heat and constant flow of particles and magnetic fields. The constant flow of particles from the sun is known as solar wind and are mostly composed of high energy protons. The solar wind fills nearly all the space of the known solar system. Along with the solar wind, the solar magnetic field also fill the solar system. The solar wind along with other explosive/ eruptive solar events like Coronal Mass Ejection (CME) affects the nature of space. During such events, the nature of magnetic field and charge particle environment near to the planet change. In case of the Earth, the interaction of Earth magnetic field with the field carried by CME can trigger a magnetic disturbance near the Earth. Such events can affect the functioning of space assets Space weather refers to changing environmental conditions in space in the vicinity of Earth and other planets. We use more and more technology in space, as understanding space weather is very important. Also, understanding near Earth space weather sheds light on the behavior of space weather of other planets
Aditya L1 is the first space based observatory class Indian solar mission to study the Sun. The spacecraft is planned to be placed in a halo orbit around the Lagrangian point 1 (L1) of the Sun-Earth system, which is about 1.5 million km from the Earth. A satellite placed in the halo orbit around the L1 point has the major advantage of continuously viewing the Sun without any osculation/ eclipse. This will provide a greater advantage of observing the solar activities continuously. The spacecraft carries seven payloads to observe the photosphere, chromosphere, and the outermost layers of the Sun (the corona) using electromagnetic and particle detectors. Using the special vantage point of L1, four payloads directly view the Sun and the remaining three payloads carry out in-situ studies of particles and fields at the Lagrange point L1
The suit of Aditya L1 payloads are expected to provide most crucial information to understand the problems of coronal heating, Coronal Mass Ejection, pre-flare and flare activities, and their characteristics, dynamics of space weather, study of the propagation of particles, and fields in the interplanetary medium etc.
MAJOR SCIENCE OBJECTIVES
- Understanding the Coronal Heating and Solar Wind Acceleration.
- Understanding initiation of Coronal Mass Ejection, flares and near-earth space weather.
- To understand coupling and dynamics of the solar atmosphere. To understand solar wind distribution and temperature anisotropy.
UNIQUENESS OF THE MISSION
• First time spatially resolved solar disk in the near UV band CME dynamics close to the solar disk (~ from 1.05 solar radius) and thereby providing information in the acceleration regime of CME which is not observed consistently On-board intelligence to detect CME and solar flares for optimized observations and data volume Directional and energy anisotropy of solar wind using multi-direction observations
ADITYA-L1 SCIENCE PAYLOADS
The Aditya-L1 mission carries a suit of seven scientific payloads to carry out systematic study of the Sun. The Visible Emission Line Coronagraph studies the solar corona and dynamics of Coronal Mass Ejections. The Solar Ultra-violet Imaging Telescope (SUIT) payload images the Solar Photosphere and Chromosphere in near Ultra-violet (UV) and also measures the solar irradiance variations in near UV. The Aditya Solar wind Particle Experiment, (ASP EX) and Plasma Analyzer Package for Aditya (PAPA) payloads study the solar wind and energetic ions, as well as their energy distribution. The Solar Low Energy X-ray Spectrometer (Sol EXS) and The High Energy L1 Orbiting X-ray Spectrometer (HEL1OS) studies the X-ray flares from the Sun over a wide X-ray energy range. The Magnetometer payload is capable of measuring interplanetary magnetic fields at the L1 point
The science payloads of Aditya-L1 are indigenous developed by different laboratories in the country. The Visible Emission Line Coronagraph instrument is developed at the Indian Institute of Astrophysics, Bangalore; SUIT instrument at Inter University Center for Astronomy & Astrophysics, Pune Advanced Performance Experimental instrument at Physical Research Laboratory, Ahmedabad, PAPA payload at Space Physics Laboratory, Space Center, Thiruvananthapuram; Sol EXS and HEL1OS payloads at U R RO Satellite Center, Bangalore, and the Magnetometer payload at the Laboratory for Optics Systems, Bangalore. All the payloads are developed with the close collaboration of various centers of ISRO
For a two body gravitational system, the Lagrange Points are the position in space where a small object tends to stay, if put there. These points in space for two body systems such as Sun and Earth can be used by spacecraft to remain at these positions with reduced fuel consumption
Technically, at Lagrange point, the gravitational pull of the two large bodies equals the necessary centripetal force required for a small object to move with them. For two body gravitational systems, there are total five Lagrange points denoted as L1, L2, L3, L4 and L5. The Lagrange points for the Sun-Earth system are shown in the figure. The Lagrange point L1 lies between the Sun-Earth line. The distance of L1 from Earth is approximately 1% of the Earth-Sun distance
ADITYA-L1 TRAJECTORY TO L1
The Aditya-L1 mission will be launched by ISRO PSLV rocket from Space Center, Initially the spacecraft will be placed in a low earth orbit. Subsequently, the orbit will be made more elliptical and later the spacecraft will be launched towards the Lagrange point L1 by using on-board propulsion. As the spacecraft travels towards L1, it will exit the earths’ gravitational Sphere of Influence (SOI). After exit from SOI, the cruise phase will start and subsequently the spacecraft will be injected into a large halo orbit around L1. The total travel time from launch to L1 would take about four months for Aditya-L1. The trajectory of Aditya-L1 mission is shown in the figure above
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