FORMATION DEPTHS OF ABSORPTION LINES IN THE SOLAR ATMOSPHERE,

Abstract

Effective formation depths are determined for absorption lines in the solar atmosphere used for recording the magnetic field with the double magnetograph of the Crimean Astrophysical Observatory: wavelengths 4808, 5250, 5302, (FeI, 6103 (CaI) and 4554A (BaII). (Author)

Document Details

Document Type
Technical Report
Publication Date
Mar 01, 1970
Accession Number
AD0705044

Entities

People

  • V. G. Buslavskii

Organizations

  • Air Force Cambridge Research Laboratories

Tags

DTIC Thesaurus Topics

  • Absorption
  • Atmospheres
  • Magnetic Fields
  • Observatories
  • Solar Atmosphere
  • Stellar Atmospheres

Fields of Study

  • Physics

Readers

  • Solar Physics

Technology Areas

  • Space