MLchartDataset catalogue

Helioseismology

Term · Meteorology and atmospheric science · MLC-T-MET-006217

The study of the Sun's interior structure and dynamics by observing the oscillations on its surface. These oscillations, caused by sound waves resonating within the Sun, provide information about temperature, density, composition, and rotation beneath the photosphere. Understanding the solar dynamo through helioseismology is relevant to forecasting solar cycles and their influence on Earth's climate and space weather.

Table 1. Record
IdentifierMLC-T-MET-006217
FieldMeteorology and atmospheric science
Record as JSON
{
  "id": "MLC-T-MET-006217",
  "term": "Helioseismology",
  "field": "Meteorology and atmospheric science",
  "definition": "The study of the Sun's interior structure and dynamics by observing the oscillations on its surface. These oscillations, caused by sound waves resonating within the Sun, provide information about temperature, density, composition, and rotation beneath the photosphere. Understanding the solar dynamo through helioseismology is relevant to forecasting solar cycles and their influence on Earth's climate and space weather.",
  "url": "https://mlchart.com/terminology/meteorology/helioseismology/"
}

Record 4,502 of 10,816 in Meteorology and atmospheric science terminology (MLC-0110). Request the full dataset.