KODAIKANAL SOLAR OBSERVATORY - SCI & TECH

News: 125 years of Kodaikanal Solar Observatory: How the Great Drought of 1876 led to its establishment

 

What's in the news?

       The Madras Observatory was merged with the KoSO following the reorganisation of all Indian observatories on April 1, 1899.

 

Key takeaways:

       The hilltop observatory helped in making some key scientific discoveries over the years.

 

Kodaikanal Solar Observatory (KoSO):

       It is a solar observatory owned and operated by the Indian Institute of Astrophysics.

 

Backdrop:

       The concept of an Indian solar observatory began in the late 19th century, and the government approved the establishment of the Solar Physics Observatory in Kodaikanal in August 1893.

 

Location:

       Kodaikanal in the Palani hills of Tamil Nadu was picked for the observatory because of its good atmospheric conditions, based on surveys by Charles Michie Smith (a Professor of Physics at the Madras Christian College).

 

Foundation:

       Lord Wenlock, the Governor of Madras at the time, laid the foundation stone for KoSO in 1895.

       Systematic observations at KoSO commenced on March 14, 1901.

 

Instruments at KoSO:

       Initially, KoSO had telescopes to study sunspots, prominences, and solar radiation.

       Now, it has advanced instruments like the H-alpha telescope and the White Light Active Region Monitor (WARM) for high solar imaging.

 

Need for Observatory:

1. Great Drought of 1875-1877:

       The event, caused by low rainfall, highlighted the need for thorough solar studies to understand its effects on weather patterns.

 

2. India’s Geographical Significance:

       India’s drought was part of a broader global issue, impacting multiple countries and resulting in widespread famine.

 

Significance of KoSo:

       Archives: KSO has one of the world’s most comprehensive solar data archives, with daily images of the sun dating back over a century.

 

       Digitization Project: An ongoing project aims to digitize and preserve the observatory’s vast collection of solar observations, ensuring their availability for future research.