Determination of the microturbulence component of the solar photospheric velocity field. II. Microturbulence velocity determined from multiple lines by the method of fine analysis (in Russian)
Journal Article
·
· Astrometriya Astrofiz., v. 19, pp. 57-63
OSTI ID:4261827
- Research Organization:
- Originating Research Org. not identified
- NSA Number:
- NSA-30-022087
- OSTI ID:
- 4261827
- Journal Information:
- Astrometriya Astrofiz., v. 19, pp. 57-63, Other Information: Orig. Receipt Date: 31-DEC-74; Bib. Info. Source: IAA (International Aerospace Abstr.)
- Country of Publication:
- Country unknown/Code not available
- Language:
- Russian
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Determination of the microturbulent component of the velocity field in the solar photosphere. II. Microturbulent velocity derived by the method of fine analysis, using the multiplet lines
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Determination of the microturbulent component of the velocity field in the solar photosphere. I. Application of the method of fine analysis to the line lambda 6330 A CrI to determine microturbulent velocity
Journal Article
·
Mon Jan 01 00:00:00 EST 1973
· Astrometriya Astrofiz., v. 19, pp. 57-63
·
OSTI ID:4261827
Determination of the microturbulence component in the solar photospheric velocity field. I. Use of the fine analysis method to determine microturbulence velocity using the example of the 6330 A Crl line
Journal Article
·
Mon Jan 01 00:00:00 EST 1973
· Astrometriya Astrofiz., no. 19, pp. 51-57
·
OSTI ID:4261827
Determination of the microturbulent component of the velocity field in the solar photosphere. I. Application of the method of fine analysis to the line lambda 6330 A CrI to determine microturbulent velocity
Journal Article
·
Mon Jan 01 00:00:00 EST 1973
· Astrometriya Astrofiz., v. 19, pp. 51-57
·
OSTI ID:4261827