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What is the primary function of the Visible Emission Line Coronagraph (VELC) as part of the ADITYA-L1 Mission?
  • a)
    To study the Earth's atmosphere
  • b)
    To observe the solar corona from a distance of 1.5 million kilometers
  • c)
    To monitor satellite communications
  • d)
    To analyze terrestrial weather patterns
Correct answer is option 'B'. Can you explain this answer?
Verified Answer
What is the primary function of the Visible Emission Line Coronagraph ...
The VELC is designed to observe the solar corona, which is the outermost layer of the Sun's atmosphere, from a unique vantage point approximately 1.5 million kilometers away from Earth. This distance allows it to conduct detailed imaging and spectroscopy of the corona, focusing on characteristics such as temperature and plasma velocity. The capability to analyze the solar corona is critical for understanding solar phenomena that can impact space weather and communications on Earth.
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What is the primary function of the Visible Emission Line Coronagraph ...
Primary Function of VELC
The Visible Emission Line Coronagraph (VELC) is an integral component of the ADITYA-L1 Mission, primarily designed to study the solar corona.
Key Objectives of VELC
  • Observation of the Solar Corona: VELC aims to observe the solar corona, the outer atmosphere of the Sun, which is crucial for understanding solar dynamics and its influence on space weather.
  • Distance from Earth: Positioned approximately 1.5 million kilometers away from Earth at the L1 Lagrange point, VELC provides an unobstructed view of the Sun, allowing for continuous monitoring of solar activities.
  • Study of Solar Phenomena: The coronagraph enables the observation of solar events such as solar flares, coronal mass ejections (CMEs), and other transient phenomena that can impact space weather and, consequently, satellite operations and communication systems on Earth.
  • Understanding Solar Influence: By analyzing the solar corona, VELC helps in understanding the mechanisms driving solar wind and its interaction with the Earth's magnetosphere, which can affect satellite communications and terrestrial technology.

Conclusion
In summary, the primary function of the Visible Emission Line Coronagraph (VELC) is to observe the solar corona from a distance of 1.5 million kilometers, facilitating vital research in solar physics and its implications for space weather phenomena. This role is crucial for enhancing our understanding of the Sun and its effects on the Earth and its technological systems.
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Passage - 6The Aditya mission was conceived as a 400kg class satellite carrying one payload, the Visible Emission Line Coronagraph (VELC) and was planned to launch in a 400 km low earth orbit. A Satellite placed in the halo orbit around the [1] of the Sun -Earth system has the major advantage of continuously viewing the Sun without any occultation/ eclipses.Therefore, the Aditya mission has now been revised to "[1] mission" and will be inserted in a halo orbit around the [2], which is 1.5 million km from the Earth. The satellite carries additional six payloads with enhanced science scope and objectives. The project is approved and the satellite will be launched during 2019 - 2020 timeframe by PSLV-XL from [3].The Aditya mission was meant to observe only the solar corona. The outer layers of the Sun, extending to thousands of km above the disc (photospher e) is termed as the corona. It has a temperature of more than a million degree Kelvin which is much higher than the solar disc temperature of around 6000K. How the corona gets heated to such high temperatures is still an unanswered question in solar physics.In addition, particle payloads will study the particle flux emanating from the Sun and reaching the [2] orbit, and the magnetometer payload will measure the variation in magnetic field strength at the halo orbit around [2]. These payloads have to be placed outside the interference from the Earths magnetic field and could not have been useful in the low earth orbit.Q.The first spacecraft in the world launched to study the Sun is

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What is the primary function of the Visible Emission Line Coronagraph (VELC) as part of the ADITYA-L1 Mission?a) To study the Earth's atmosphereb) To observe the solar corona from a distance of 1.5 million kilometersc) To monitor satellite communicationsd) To analyze terrestrial weather patternsCorrect answer is option 'B'. Can you explain this answer? for CLAT 2025 is part of CLAT preparation. The Question and answers have been prepared according to the CLAT exam syllabus. Information about What is the primary function of the Visible Emission Line Coronagraph (VELC) as part of the ADITYA-L1 Mission?a) To study the Earth's atmosphereb) To observe the solar corona from a distance of 1.5 million kilometersc) To monitor satellite communicationsd) To analyze terrestrial weather patternsCorrect answer is option 'B'. Can you explain this answer? covers all topics & solutions for CLAT 2025 Exam. Find important definitions, questions, meanings, examples, exercises and tests below for What is the primary function of the Visible Emission Line Coronagraph (VELC) as part of the ADITYA-L1 Mission?a) To study the Earth's atmosphereb) To observe the solar corona from a distance of 1.5 million kilometersc) To monitor satellite communicationsd) To analyze terrestrial weather patternsCorrect answer is option 'B'. Can you explain this answer?.
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