By Kameshwar C Wali
S Chandrasekhar, popularly referred to as Chandra, was once one of many preferable scientists of the 20 th century. The yr 2010 marks the start centenary of Chandra. His specified form of examine, inward sure, looking a private point of view to grasp a specific box, after which go directly to one other used to be so designated that it'll draw huge curiosity and a spotlight between students.
As Chandra elucidates within the preface, ''The quite a few installments describe intimately the evolution of my clinical paintings up to now 40 years and documents each one research, describing the doubts and the successes, the pains and the tribulations. And the components my a variety of affiliates and assistants performed within the final touch of the various investigations are detailed''. it really is certainly a notable and infrequent record, interesting to learn and adventure the fun, frustrations and struggles of an artistic brain
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S Chandrasekhar, popularly often called Chandra, was once one of many prime scientists of the twentieth century. The yr 2010 marks the start centenary of Chandra. His distinct type of learn, inward sure, looking a private point of view to grasp a selected box, after which move directly to one other was once so specified that it'll draw enormous curiosity and a spotlight between students.
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Extra info for A Scientific Autobiography: S. Chandrasekhar
However, scientificbio January 5, 2011 11:30 Turbulence; Hydromagnetism (1948–1960) Summer 1956 scientificbio Reprint volume: A Scientific Autobiography ... 39 on the whole, this period was about the most frustrating in my entire experience to date. During the winter and spring months, I lectured on quantum mechanics. I had an enthusiastic class: the class applauded at the end of the courses. Apparently this was the second time it had happened in the Physics Department. Fermi’s class in Nuclear Physics had similarly been applauded in an earlier year.
I was surprised that the matrix was reducible. At about this time, I began to think of the general laws of scattering and, having corresponded with Hamilton off and on during 1946, I decided to see him when I was due East in February. Paper XVI was, of course, simple. It was a tabulation of H-functions. I realized at this stage that the main problems of semi-infinite atmospheres had been solved. It remained to go into finite atmospheres. For this purpose, functional equations similar to Ambarzumian’s had to be formulated for the case of finite atmospheres.
The paper by Rayleigh on the character of the equilibrium of an incompressible fluid of varying density seemed a good paper to discuss. The idea of extending it to include viscosity was immediately apparent. But I made a number of errors. I ‘knew’ something was incorrect in my treatment because in the case when the heavier liquid was overlying the lighter one, I found that the arrangement was predicted to be stable for wave numbers exceeding a certain value. I consulted Wentzel regarding this. He was very generous and checked my analysis.