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Dive into the research topics where S. R. Das Gupta is active.

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Featured researches published by S. R. Das Gupta.


Astrophysics and Space Science | 1977

A new representation of theH-functions of radiative transfer

S. R. Das Gupta

We obtain a new representation of ChandrasekharsH-functionsH(z) corresponding to the dispersion functionT(z) = |δrs−frs(z)|, [frs(z)] is of rank one.H(z) is obtained in the formAbstractWe obtain a new representation of ChandrasekharsH-functionsH(z) corresponding to the dispersion functionT(z) = |δrs−frs(z)|, [frs(z)] is of rank one.H(z) is obtained in the form


Astrophysics and Space Science | 1974

OnH-functions of radiative transfer

S. R. Das Gupta


Astrophysics and Space Science | 1978

A note on theH-functions of transfer problems in multiplying media

S. R. Das Gupta

H\left( z \right) = \left( {A_0 + A_1 z} \right)/\left( {K + z} \right) - \sum\limits_1^n {\int\limits_{E_r } {P_r (x) dx/(x + z),} }


Astrophysics and Space Science | 1978

An exact solution of transfer equations for interlocked multiplets

S. R. Das Gupta


Astrophysics and Space Science | 1978

A new technique for exact and unique solution of transfer equations in finite media

S. R. Das Gupta

WherePrx(=ør(x)/H(x)) is continuous onErwhich are subsets of [0, 1].Ao,A1are determinable constants andK is the positive root ofT(z),ør(x) are known functions. From this formH(z) is then obtained in terms of a Fredholm type integral equation. This new form ofH(z) has proved to be very useful in solving coupled integral equations involvingX-,Y-functions of transport problems.Pr(x) can be replaced by approximating polynomials whose coefficients can be determined as functions of the moments of known functions; a closed form approximation ofH(z) to a sufficiently high degree of accuracy is then readily available by term integrations.


Astrophysics and Space Science | 1980

On transfer equation in a semi-infinite atmosphere with albedo ω>1

S. R. Das Gupta; Z. Islam; S. K. Bishnu

ChandrasekharsH-functionH(z) corresponding to the dispersion functionT(z)=|δ rs −frs(z)|, where [f rs (z)] is of rank 1, is obtained in terms of a Cauchy integral whose density functionQ(x,ω 1,ω 2,...) can be approximated by approximating polynomials (uniformly converging toQ(x)) having their coefficients expressed as known functions of the parametersω r s. A closed form approximation ofH(z) to a sufficiently high degree of accuracy is then readily available by term by term integration.


Astrophysics and Space Science | 1987

An exact solution of time-dependent equation of transfer of trapped radiation in a finite absorbing medium

S. K. Bishnu; S. R. Das Gupta

Some useful results and remodelled representations ofH-functions corresponding to the dispersion function


Astrophysics and Space Science | 1987

Decomposition of product of certain functions relevant to the solution of transfer equations by Wiener-Hopf technique

Santanu Das Gupta; S. R. Das Gupta


Astrophysics and Space Science | 1991

Laser radiation in active amplifying media treated as a transport problem : transfer equation derived and exactly solved

Santanu Das Gupta; S. R. Das Gupta

T\left( z \right) = 1 - 2z^2 \sum\limits_1^n {\int_0^{\lambda r} {Y_r } \left( x \right){\text{d}}x/\left( {z^2 - x^2 } \right)}


Astrophysics and Space Science | 1991

Exact solution of the transport equation in finite media with a plane and uniform point source and flux normally incident at the faces from outside

S. K. Bishnu; S. R. Das Gupta

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S. K. Bishnu

University of North Bengal

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B. Majee

University of North Bengal

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Z. Islam

University of North Bengal

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Zahurul Islam

Bangladesh University of Engineering and Technology

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Chitta R. Nayak

University of North Bengal

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