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 (in Russian)
Journal Article
·
· Astrometriya Astrofiz., v. 19, pp. 57-63
OSTI ID:4308921
- Research Organization:
- Originating Research Org. not identified
- NSA Number:
- NSA-30-013508
- OSTI ID:
- 4308921
- Journal Information:
- Astrometriya Astrofiz., v. 19, pp. 57-63, Other Information: Orig. Receipt Date: 31-DEC-74
- Country of Publication:
- Country unknown/Code not available
- Language:
- Russian
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Determination of the microturbulence component of the solar photospheric velocity field. II. Microturbulence velocity determined from multiple lines by the method of fine analysis
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
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:4308921
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:4308921
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:4308921