PaschenSerien

Paschen series, named after the German physicist Friedrich Paschen, is a series of spectral lines in the emission spectrum of hydrogen and other hydrogen-like atoms. These lines are observed when an electron transitions from a higher energy level to the third energy level (n=3) in the atom. The Paschen series is part of the Balmer series, which is a subset of the hydrogen spectrum, and it falls within the infrared region of the electromagnetic spectrum.

The Paschen series is characterized by the transition of an electron from a higher principal quantum number n to n=3. The wavelengths of the spectral lines in the Paschen series can be calculated using the Rydberg formula, which is given by:

1/λ = R(1/3² - 1/n²)

where λ is the wavelength of the emitted photon, R is the Rydberg constant (1.0973731534 × 10⁷ m⁻¹), and n is the principal quantum number of the higher energy level. The Paschen series includes transitions from n=4 to n=3, n=5 to n=3, and so on, with each transition corresponding to a specific wavelength of light.

The Paschen series is significant in astrophysics and atomic physics as it provides valuable information about the energy levels and transitions within hydrogen and hydrogen-like atoms. It is also used in various applications, such as spectroscopy, where the analysis of spectral lines helps in identifying the composition and properties of different materials. Additionally, the Paschen series is relevant in the study of plasma physics and the behavior of ionized gases, as it can provide insights into the energy distribution and dynamics of electrons in such systems.