Well, the different series represent different electronic transitions. But there is an important equation, the Rydberg formula which describes all of them.. I think you've learned of it since you mention the n values. This lead to the Bohr model of the hydrogen atom, which explained _why_ you had these levels.
Or, almost. See, it turned out that those lines were not actually single lines, but several lines very close together.. And so they had to add more variables to describe how these levels-within-levels fit together.. and the answer to that eventually came from quantum mechanics.
A spectral line that appears at a wavelength of 321 nm in the laboratory appears at a wavelength of 328 nm in the spectrum of a distant object. We say that the object's spectrum is red shifted.
The second longest wavelength in the absorption spectrum of hydrogen corresponds to the transition from the n=2 to n=4 energy levels. This transition produces a spectral line known as the H-alpha line, which falls in the red part of the visible spectrum at a wavelength of 656.3 nm.
The range of spectral lines produced during electron transition is determined by the energy difference between the initial and final electronic states. This energy difference corresponds to the photon energy of the emitted light, which dictates the wavelength or frequency of the spectral lines observed in the spectrum. Additionally, the atomic structure and electron configuration of the atom also play a role in determining the specific transitions and resulting spectral lines.
The detector in a spectrograph that records spectral lines photographically is a photographic plate or film. This photographic medium captures the light from the spectral lines dispersed by the spectrograph, allowing them to be recorded for analysis and interpretation.
The spectral properties of a flame refer to the visible light emitted when a hydrocarbon fuel burns. The color of the flame can indicate the temperature and the presence of certain elements in the fuel. Spectral analysis of the light emitted from a flame can be used to identify the chemical composition of the burning material.
The relationship between the wavelength of a spectral line and its energy is inverse. This means that as the wavelength decreases, the energy of the spectral line increases, and vice versa.
Germanium has a maximum spectral response at around 1.8 µm wavelength, while silicon's maximum spectral response is at around 1.1 µm wavelength.
To find the wavelength of a spectral line using a diffraction grating, you can use the formula: dsin(θ) = mλ, where d is the spacing of the grating lines, θ is the angle of diffraction, m is the order of the spectral line, and λ is the wavelength of the light. By measuring the angle of diffraction of the spectral line and knowing the grating spacing, you can calculate the wavelength of the light.
Green.
what is spectral evidence Spectrum (spectral) refers to different frequencies of light associated with a substance.
what is spectral evidence Spectrum (spectral) refers to different frequencies of light associated with a substance.
As the frequencies of pure spectral colors increase, the wavelengths of the colors will decrease. This is because frequency and wavelength are inversely proportional in electromagnetic waves, according to the equation λν = c, where λ is the wavelength, ν is the frequency, and c is the speed of light.
The colors not found in the light spectrum are magenta, pink, and purple. These colors are called "non-spectral colors" or "extra-spectral colors" because they are perceived by our brains through a combination of wavelengths rather than being associated with a single wavelength of light.
The wavelength of yellow sodium light in water is approximately 589 nanometers. This specific wavelength is characteristic of the spectral emission line of sodium when it is viewed through water.
A spectral line
The shortest wavelength present in the Brackett series of spectral lines is in the infrared region around 1.46 micrometers. This series represents transitions in hydrogen atoms from higher energy levels to the n=4 energy level.
Barium has an atomic spectra of lines, not only one line (with one wavelength); I reccomend to consult a catalog of spectral lines. See the link below.