Found: 5
Select item for more details and to access through your institution.
The fraunhofer lines classifications by asymmetry changes inside the profiles in the spectrum of the Sun.
- Published in:
- Astrophysical Bulletin, 2017, v. 72, n. 3, p. 337, doi. 10.1134/S1990341317030221
- By:
- Publication type:
- Article
On the fine structure of the Fe I λ532.4185-nm line profile in the spectrum of the solar disk center.
- Published in:
- Kinematics & Physics of Celestial Bodies, 2008, v. 24, n. 6, p. 296, doi. 10.3103/S0884591308060056
- By:
- Publication type:
- Article
On the Doppler Width of Spectral Lines.
- Published in:
- Kinematics & Physics of Celestial Bodies, 2018, v. 34, n. 2, p. 102, doi. 10.3103/S0884591318020058
- By:
- Publication type:
- Article
The total number of spicules on the solar surface and their role in heating and mass balanace in the solar corona.
- Published in:
- Astronomy Reports, 2016, v. 60, n. 9, p. 848, doi. 10.1134/S1063772916080060
- By:
- Publication type:
- Article
Intensity Dependence of the Asymmetry of Fraunhofer Line Profiles.
- Published in:
- Astronomy Reports, 2001, v. 45, n. 1, p. 75, doi. 10.1134/1.1336604
- By:
- Publication type:
- Article