MLchartDataset catalogue

Fraunhofer lines

Term · Meteorology and atmospheric science · MLC-T-MET-005750

Dark absorption lines observed in the spectrum of the sun and other stars, caused by the absorption of specific wavelengths of light by cooler gases in their outer atmospheres. These lines correspond to particular chemical elements, providing information about the composition of stellar atmospheres. The strongest Fraunhofer lines are designated by letters, such as the D-lines for sodium.

Table 1. Record
IdentifierMLC-T-MET-005750
FieldMeteorology and atmospheric science
Record as JSON
{
  "id": "MLC-T-MET-005750",
  "term": "Fraunhofer lines",
  "field": "Meteorology and atmospheric science",
  "definition": "Dark absorption lines observed in the spectrum of the sun and other stars, caused by the absorption of specific wavelengths of light by cooler gases in their outer atmospheres. These lines correspond to particular chemical elements, providing information about the composition of stellar atmospheres. The strongest Fraunhofer lines are designated by letters, such as the D-lines for sodium.",
  "url": "https://mlchart.com/terminology/meteorology/fraunhofer-lines/"
}

Record 3,755 of 10,702 in Meteorology and atmospheric science terminology (MLC-0110). Request the full dataset.