Syllabus: GS 3 / Space
In News
- Researchers investigated the magnetic field at different layers of the solar atmosphere using data from the Kodaikanal Tower Tunnel Telescope.
About the study
- The IIA’s approach involves probing the solar magnetic field at various atmospheric heights, an essential endeavor for understanding fundamental solar processes.
- The solar atmosphere is composed of various layers connected through magnetic fields.
- These magnetic fields are responsible for transferring energy and mass from the inner layers to the outer layers.
- The magnetic field is the prime driver of the solar wind.
- Data Collection: Researchers use Hydrogen-alpha and Calcium II 8662 Å spectral lines to analyze the magnetic field at different solar atmosphere heights.
- Findings: The Hα line is less sensitive to local temperature fluctuations, making it effective for probing the chromospheric magnetic field, especially in active regions with sudden temperature changes.
Impact
- The findings from IIA’s research have the potential to transform our understanding of solar physics.
- By addressing the complexities of solar magnetic fields, the institute contributes to broader efforts to solve long standing questions about solar energy transfer and solar wind dynamics.
- This research is crucial for tackling the coronal heating problem and understanding the mechanisms driving solar wind.
Future outlook
- The Indian Institute of Astrophysics continues to lead the way in solar research, with its innovative techniques and cutting-edge technology paving the way for groundbreaking discoveries in astrophysics.
- Future studies will likely build on these advancements, offering deeper insights into the sun’s behavior and its effects on space weather.
Do you know ? – The Kodaikanal Solar Observatory (KoSO) is known for the discovery of the Evershed Effect in 1909. – It is operated by the Indian Institute of Astrophysics (IA), and it is located in Kodaikanal, Tamil Nadu. – The Kodaikanal Tower Tunnel Telescope features a sophisticated 3-mirror Coelostat system. – This setup includes a primary mirror (M1) that tracks the sun, a secondary mirror (M2) that redirects sunlight downward, and a tertiary mirror (M3) that aligns the beam horizontally. |
Source : PIB
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