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    More solar storms brewing after last week’s aurorae as Sun ‘wakes up’

    • May 15, 2024
    • Posted by: OptimizeIAS Team
    • Category: DPN Topics
    No Comments

     

     

    More solar storms brewing after last week’s aurorae as Sun ‘wakes up’

    Sub: Science and tech

    Sec: Space sector

    Tags: aurorae, Solar storms

    Context:

    • On the night of May 10, 2023, a vivid display of aurorae was visible globally, including in atypical locations such as Hanle, Ladakh.

    Details of the event:

    • The aurorae were caused by a geomagnetic storm triggered by coronal mass ejections (CMEs) from the Sun, which interacted with Earth’s magnetic field and upper atmosphere.
    • The event coincided with the Sun approaching the peak of its 11-year solar cycle, marked by increased sunspot activity and magnetic field reversals.
      • The solar cycle is the cycle that the Sun’s magnetic field goes through approximately every 11 years.
      • The solar cycle affects activity on the surface of the Sun, such as sunspots which are caused by the Sun’s magnetic fields.
    • The specific sunspot AR 3664 was noted to be exceptionally active, growing 16 times as wide as Earth by May 7 and releasing three CMEs that impacted Earth on May 10.
    • The last similar intensity geomagnetic storm occurred in 2003. The most severe historical geomagnetic storm recorded occurred in 1859, known for causing widespread telegraph disruptions.

    Potential Hazards:

    • Such solar events can cause significant disruptions, including blackouts, satellite malfunctions, and dangers to astronauts due to intensified solar radiation and charged particles.

    Auroras:

    • Auroras are natural light displays that occur when charged particles from solar winds interact with the Earth’s magnetosphere.
      • The magnetosphere is the region surrounding the Earth where the dominant magnetic field is the Earth’s, rather than the magnetic field of interplanetary Space.
      • It protects the Earth against solar winds and is strongest at the poles.
    • These particles travel along the Earth’s magnetic field and upon colliding with atmospheric molecules and atoms, cause emissions of light seen as auroras.
      • In North Pole- Aurora Borealis
      • In South Pole- Aurora Australis

    Role of Aditya- L1:

    • ISRO’s spacecraft Aditya-L1, positioned at the L1 Lagrange point, is equipped to monitor solar activities and played a role in observing recent solar events.
      • Instruments like ISRO’s Visible Emission Line Coronagraph (VELC) on Aditya-L1 are critical for advancing the understanding and prediction of solar storms.
      • ASPEX payload had captured the enhancement of the alpha particle and proton flux of the solar wind as signatures of the solar storm.
      • SoLEXS and HEL1OS payloads had detected “the multiple X- and M-class flares during the last few days”.
    • The Chandrayaan-2 orbiter around the moon also reportedly detected “signatures” of the emissions from the Sun.

    About Aditya-L1 Mission:

    • Aditya-L1 is the first space based observatory class Indian solar mission to study the Sun from a substantial distance of 1.5 million kilometers.
    • Aditya-L1 is also ISRO’s second astronomy observatory-class mission after AstroSat (2015).
    • The spacecraft is placed in a halo orbit around the Lagrangian point 1 (L1) of the Sun-Earth system.

    Objective:

    • The mission aims to provide valuable insights into the solar corona, photosphere, chromosphere, and solar wind.
    • The primary objective of Aditya-L1 is to gain a deeper understanding of the Sun’s behavior, including its radiation, heat, particle flow, and magnetic fields, and how they impact Earth.

    Payloads of Aditya-L1 solar observatory:

    Payloads of Aditya L-1Description
    Visible Emission Line Coronagraph (VELC)
    • The VELC payload on-board Aditya-L1 is an internally occulted solar coronagraph with simultaneous imaging, spectroscopy and spectro-polarimetry channels close to the solar limb.
    • Both imaging and spectroscopic observations obtained by VELC payload are key to study the diagnostic parameters of solar corona and dynamics as well as origin of the coronal mass ejections and magnetic field measurements of the solar corona.
    Aditya Solar wind Particle Experiment (ASPEX) payload
    • Studies solar wind and energetic ions.
    • Analyze their energy distribution.
    • ASPEX comprises two cutting-edge instruments – the Solar wind Ion Spectrometer (SWIS) and STEPS (SupraThermal and Energetic Particle Spectrometer).
    • SWIS instrument has successfully measured solar wind ions, primarily protons and alpha particles.
    Solar Ultra-violet Imaging Telescope (SUIT)
    • Captures images of the Solar Photosphere and Chromosphere in near Ultraviolet (UV).
    • Measures solar irradiance variations in near UV.
    Solar Low Energy X-ray Spectrometer (SoLEXS)
    • Functions as a Soft X-ray spectrometer.
    • Studies X-ray flares from the Sun across a wide X-ray energy range.
    High Energy L1 Orbiting X-ray Spectrometer (HEL1OS)
    • Acts as a Hard X-ray spectrometer.
    • Investigates X-ray flares from the Sun across a wide X-ray energy range.
    Plasma Analyser Package for Aditya (PAPA)
    • Gather data on plasma characteristics and composition in the interplanetary space.
    • Provides insights into solar wind interactions with the environment.
    Advanced Tri-axial High-Resolution Digital Magnetometers (MAG)
    • To measure the low-intensity interplanetary magnetic field in space.
    • It has two sets of Magnetic Sensors.
    aurorae More solar storms brewing after last week’s aurorae as Sun ‘wakes up’ Science and tech SOLAR STORMS
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