MLchartDataset catalogue

Bishop's ring

Term · Meteorology and atmospheric science · MLC-T-MET-003931

A large, whitish or bluish-white halo observed around the sun or moon, often with a brownish-red outer border. This optical phenomenon is caused by the diffraction of light by very fine dust particles in the upper atmosphere. It was first widely observed after the 1883 eruption of Krakatoa.

Table 1. Record
IdentifierMLC-T-MET-003931
FieldMeteorology and atmospheric science
Record as JSON
{
  "id": "MLC-T-MET-003931",
  "term": "Bishop's ring",
  "field": "Meteorology and atmospheric science",
  "definition": "A large, whitish or bluish-white halo observed around the sun or moon, often with a brownish-red outer border. This optical phenomenon is caused by the diffraction of light by very fine dust particles in the upper atmosphere. It was first widely observed after the 1883 eruption of Krakatoa.",
  "url": "https://mlchart.com/terminology/meteorology/bishop-s-ring/"
}

Record 1,149 of 10,816 in Meteorology and atmospheric science terminology (MLC-0110). Request the full dataset.