National Institute of Technology Rourkela

राष्ट्रीय प्रौद्योगिकी संस्थान राउरकेला

ଜାତୀୟ ପ୍ରଯୁକ୍ତି ପ୍ରତିଷ୍ଠାନ ରାଉରକେଲା

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Syllabus

Course Details

Subject {L-T-P / C} : PH5112 : Stellar and Planetary Atmosphere { 3-0-0 / 3}

Subject Nature : Theory

Coordinator : Suryanarayan Dash

Syllabus

Module 1 :

(6 hrs): Composition and structure of the atmosphere, stellar and planetary atmosphere, Hydrostatic equilibrium and pressure stratification, Optical depth and radiative transfer basics.

Module 2 :

(8 hrs): The equation of radiative transfer, Emission, absorption, and scattering processes, Opacity sources: bound-bound, bound-free, free-free transitions, Thomson scattering, Line formation and broadening mechanisms, Doppler, natural, collisional, and Stark broadening.

Module 3 :

(8 hrs): Change in atmospheric pressure, temperature, and density with altitude, Basic radiative transfer in the atmosphere, Concept of local thermodynamic equilibrium (LTE) and Non-local thermodynamic equilibrium (NLTE).

Module 4 :

(6 hrs): Equation of motion and fundamental forces, circulation of the atmosphere, Atmospheric waves and turbulence, Weather systems: cyclones, anticyclones, monsoons.

Module 5 :

(8 hrs): Observational techniques to characterize explanatory atmosphere: photometry, spectroscopy, and polarimetry, The role of magnetic fields in stellar & planetary atmospheres, effect of stellar winds on planetary atmosphere.

Course Objective

1 .

To understand the structure of the stellar and planetary atmosphere

2 .

To analyze the atmospheric dynamics and circulation patterns

3 .

To apply the radiative transfer principles in stellar atmospheres

4 .

To understand the planetary weather systems

5 .

To characterize the exoplanet and their atmosphere

Course Outcome

1 .

At the end of course, students will be able to:
CO1: understand the properties of stellar and planetary atmosphere.

2 .

CO2: learn to apply radiative transfer processes.

3 .

CO3: acquire the knowledge of line formation and broadening mechanism.

4 .

CO4: understand the concept of LTE and NLTE.

5 .

CO5: characterize stellar and planetary atmospheres.

Essential Reading

1 .

Salby, M.L., , Physics of the Atmosphere and Climate, Cambridge University Press

2 .

Pierrehumbert, R.T., Principles of Planetary Climate, Cambridge University Press.

3 .

Gray, D.F., The Observation and Analysis of Stellar Photospheres, Cambridge University Press.

4 .

Seinfeld, J.H., & Pandis, S.N., Atmospheric Chemistry and Physics: From Air Pollution to Climate Change, Wiley.

Supplementary Reading

1 .

J. A. Bittencourt, Fundamentals of Plasma Physics, Springer

2 .

Lamers, H.J.G.L.M., & Cassinelli, J.P. , Introduction to Stellar Winds, Cambridge University Press. . (1999).

3 .

Hubeny, I., & Mihalas, D.,, Theory of Stellar Atmospheres: An Introduction to Astrophysical Non-equilibrium Quantitative Spectroscopic Analysis, Princeton University Press.

Journal and Conferences

1 .