The spectral lines emitted due to the transition of an electron from the higher energy state to a particular lower energy state form a spectral series.
Various spectral series are
- Lyman Series: The spectral lines emitted due to the transition of an electron from any higher orbit to the first orbit form a spectral series known as the Lyman series.
- Balmer Series: The spectral lines emitted due to the transition of an electron from any higher orbit to the second orbit form a spectral series known as the Balmer series.
- Paschen Series: The spectral lines emitted due to the transition of an electron from any higher orbit to the third orbit form a spectral series known as the Paschen series.
- Brackett Series: The spectral lines emitted due to the transition of an electron from any higher orbit to the fourth orbit form a spectral series known as the Brackett series.
- Pfund Series: The spectral lines emitted due to the transition of an electron from any higher orbit to the fifth orbit form a spectral series known as the Pfund series.
The longest wavelength and shortest wavelength of these spectral series can be calculated by using the Rydberg formula