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In 1888, Rydberg put forward an empirical relation to calculate the wavelengths of spectral emission...
The Rydberg formula helps to determine the wavenumber or wavelengths of hydrogen spectral lines obta...
The Rydberg-Ritz combination principle states that the wavenumber of the unknown spectral lines of a...
The hydrogen atomic spectrum consists of a sequence of spectral lines arranged in the decreasing ord...
The splitting of the main spectral line into two or more components with a slight variation in wavel...
Balmer is well renowned for his research on the hydrogen spectral series. The part of the hydrogen e...
Gives an idea about what fine structure is and the origin of fine structure in hydrogen-like atoms. ...
This series of spectral lines were observed during electron transition from higher stationary orbits...
The electron transitions from n ≥6 to n=5 result in the emergence of a sequence of spectral lines ...
The hydrogen spectrum has six series. They are Lyman series, Balmer series, Paschen series, Brackett...
In 1916, Sommerfeld extended Bohr's atomic model with the assumption of elliptical electron path...
atomic spectra
Consider a sample of hydrogen gas in the glass discharge tube. The electric current is passed throug...
Basic Astrophysics
Zeeman effect
An important topic in Astrophysics.. checkout and make use of it friends!!
This power point explains about resolving power of a plane diffraction grating
This is a presentation on "STARK EFFECT".
This PPT explains about the Comparison of prism and grating spectra
Many electronic (as opposed to photographic) remote sensors acquire data using scanning systems, whi...
