Unlocking the Mysteries of the Sun: Aditya-L1’s Observations of a Coronal Mass Ejection
By R Anil Kumar
Bengaluru, December 10. Indian researchers using the Visible Emission Line Coronagraph (VELC) onboard the Aditya-L1 mission have unveiled fascinating details about a solar event that has a profound impact on space weather. Aditya-L1, India’s first space-based solar mission, observed a Coronal Mass Ejection (CME)— a massive burst of solar plasma and magnetic fields ejected from the Sun’s outer atmosphere.
Launched on September 2, 2023, the mission was successfully placed on January 6, 2024 in a halo orbit around the first Sun-Earth Lagrange Point L1, which is about 1.5 million km away from the Earth.
What Is the Sun’s Corona and Why Is It Important?
The corona is the Sun’s outermost layer, extending millions of kilometers into space. It is an extremely hot and glowing region of the Sun, with temperatures around million degrees Celsius—much hotter than the Sun’s surface which is around 5,600 degrees Celsius. Why Corona is so hot is one of the biggest mysteries in solar science.
Normally, the corona is difficult to see because the Sun’s bright light overwhelms it, but during a solar eclipse, the corona becomes visible as a glowing halo around the Sun. Understanding the corona is crucial because it holds key insights into the Sun’s activity and how it affects space weather.
What is a Coronal Mass Ejection (CME) and Why Does It Happen?
A Coronal Mass Ejection (CME) is a massive release of solar wind and magnetic fields from the Sun’s corona. During a CME, large amounts of charged particles (such as electrons and protons) and plasma are ejected into space at extremely high speeds, often reaching millions of kilometers per hour. When a CME reaches Earth, it can interact with our magnetic field, leading to disturbances that can disrupt satellite communications, GPS systems, and power grids.
CMEs are caused by magnetic activity in the Sun’s corona. The Sun’s magnetic field is highly dynamic, constantly changing and shifting. These changes can cause the magnetic field lines to become twisted and stretched. When these magnetic fields suddenly realign or reconnect, they release a tremendous amount of energy, which pushes solar material outward into space, resulting in a CME. This explosive release of energy is often associated with solar flares, but CMEs may occur independently of them as well. The accurate connection between CME and solar flares are still a scientific puzzle. Understanding the causes and behavior of CMEs is crucial for predicting their effects on Earth and protecting our technology from space weather hazards.
What Did researchers Discover from VELC onboard Aditya-L1?
The researchers from Indian Institute of Astrophysics reported the following important observations in a paper titled ‘New Results on the Onset of a Coronal Mass Ejection from 5303 Å Emission Line Observations with VELC/ADITYA-L1’ published in peer reviewed International journal ‘The Astrophysical Journal Letter’.
The following key observations about July 16, 2024 CME are reported:
Coronal Dimming (Light Decrease):
During the Coronal Mass Ejection (CME), the Sun’s outer atmosphere, or corona, became much dimmer in a specific region. The brightness in that area dropped by about 50%, a decrease caused by the ejection of solar material. This reduction in brightness lasted for about 6 hours. This is also known as Coronal dimming.
Increase in Temperature and Turbulence:
The temperature around the region of CME is enhanced by about 30% and this region become more turbulent during the event. Both these effects are also reflected in the measurement of non-thermal velocity (or chaotic motion) of the plasma which was measured to be around 24.87 km/s. The Sun’s dynamic magnetic field gets more active during such eruptions and is the cause for observed enhanced turbulence.
Plasma Movement and Deflection:
The Doppler velocity measurements of the ejected plasma during CME is found to be redshifted with a speed of about 10 kilometers per second. It means that plasma is found to be moving away from the observer during the CME event. This also indicates a deflection of CME by the dynamic magnetic field of the Sun. This finding shows that solar magnetic forces can influence the direction of propagation of the ejected plasma as it moves in the inter-planetary space. The understanding of such deflections of the ejected plasma is important for the prediction of how CME evolves upon leaving the Sun and travelling through the solar system.
Upper panel: Shows the variation of the brightness (or intensity) of the emission line as it changes with time. The observed dip in the brightness of emission line around 13:18 UT indicates the onset of coronal dimming. The coronal dimming occurs because a large amount of solar material is ejected during the CME. This dimming, lasting for about more than 6 hours indicates that the CME has removed significant plasma from the Sun’s corona, causing a temporary reduction in brightness in the observed region.
Middle panel: Displays the width of the emission line over time. After the CME, the width increased, indicating enhanced turbulence. This may be due to restructuring of coronal magnetic field at the source region of CME after its launch.
Lower panel: Shows the Doppler velocity measurements, which measures the speed at which the solar material is moving toward or away from the observer. The Doppler velocity increased to about +10 km per second after coronal dimming which indicates the plasma is moving away from observer with this speed after CME.
The Aditya-L1 mission continues to provide invaluable insights into the Sun’s behavior, laying the groundwork for future research and helping us better understand our nearest star. Aditya-L1 is not just a scientific achievement but also an inspiration for students and young scientists across the country. It shows the power of space research and the potential for India to contribute in solving scientific challenges through space based research.
(With inputs and Image source ISRO)
