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Solar Faculae and Flocculent Flows: Spectropolarimetric and Filter Observations in the Fe I, Ba II, and Ca II Lines

Kinematics and physics of celestial bodies, 2024-02, Vol.40 (1), p.40-46

Kostik, R. I.

2024

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Observations of a bright plume in solar granulation

Astronomy and astrophysics (Berlin), 2007-12, Vol.476 (1), p.341-347

2007

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Results of Observations of Wave Motions in the Solar Facula

Kinematics and physics of celestial bodies, 2022, Vol.38 (1), p.49-60

2022

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Five-minute oscillations above granules and intergranular lanes

Astronomy and astrophysics (Berlin), 2001-04, Vol.369 (2), p.660-671

2001

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Influence of magnetic field on propagation of five-minute oscillations in the sun’s atmosphere: Phase shifts

Kinematics and physics of celestial bodies, 2014-02, Vol.30 (1), p.40-45

2014

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Kyiv monitoring program of Fraunhofer lines variation with 11-year cycle of solar activity

Journal of physical studies, 2017, Vol.21 (1/2), Article 1901

2017

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Is the problem of solar iron abundance solved?

Advances in space research, 1995-01, Vol.15 (7), p.69-72

1995

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THE SCANNER FOR PRECISE SPECTROPHOTOMETRY OF THE SUN AS A STAR

Solar physics, 1997-05, Vol.172 (1-2), p.361-370

1997

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Damping constant and turbulence in the solar atmosphere

Solar physics, 1982-05, Vol.78 (1), p.39-57

Kostik, R. I.

1982

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Helioseismology space and ground based studies

Proceedings of the International Astronomical Union, 2004-06, Vol.2004 (IAUS223), p.273-274

2004

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Oscillations in solar atmospheric structures

Journal of physical studies, 2004, Vol.8 (3), p.279-295

2004

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On the asymmetry of selected Fraunhofer lines

Solar physics, 1977-08, Vol.53 (2), p.353-358

1977

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Solar Oscillator Strengths as a Diagnostic Tool

Symposium - International Astronomical Union, 1990, Vol.138, p.35-40

1990

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On the microturbulence in the solar photosphere

Solar physics, 1979-05, Vol.62 (1), p.89-92

1979

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On the possible mechanism of formation of emission rim in hydrogen filaments

Solar physics, 1975-11, Vol.45 (1), p.119-124

1975

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The interpretation of absorption-line shifts in the solar spectrum

Solar physics, 1972-09, Vol.26 (1), p.42-51

1972

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Formation of the profiles of absorption lines in the inhomogeneous medium

Stellar Turbulence, 2005, p.53-54

2005

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The NLTE Formation of Iron Lines Used in Solar Polarimetry

Solar physics, 1997-05, Vol.172 (1-2), p.117-124

1997

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On the establishment of internally consistent abundance-oscillator strength scales

Stellar Turbulence, 2005, p.296-296

2005

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Matrix equations for radiation diffusion. II

Astrophysics, 1969, Vol.3 (1), p.6-16

Kostik, R. I.

1969

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Matrix equations of radiation diffusion. III

Astrophysics, 1968, Vol.3 (2), p.76-83

Kostik, R. I.

1968

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On the microstructure in the solar photosphere

Solar physics, 1979-01, Vol.62 (1), p.89-92

1979

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On the asymmetry of selected fraunhofer lines, II

Solar physics, 1974-06, Vol.36 (2), p.279-285

1974

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Matrix equations for radiation diffusion. I

Astrophysics, 1968, Vol.2 (4), p.197-220

1968

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Comparative Analysis of Physical Conditions in the Solar and Procyon Atmospheres

Symposium - International Astronomical Union, 1990, Vol.138, p.421-425

1990

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Solar Faculae and Flocculent Flows: Spectropolarimetric and Filter Observations in the Fe I, Ba II, and Ca II Lines

Observations of a bright plume in solar granulation

Results of Observations of Wave Motions in the Solar Facula

Five-minute oscillations above granules and intergranular lanes

Influence of magnetic field on propagation of five-minute oscillations in the sun’s atmosphere: Phase shifts

Kyiv monitoring program of Fraunhofer lines variation with 11-year cycle of solar activity

Is the problem of solar iron abundance solved?

THE SCANNER FOR PRECISE SPECTROPHOTOMETRY OF THE SUN AS A STAR

Damping constant and turbulence in the solar atmosphere

Helioseismology space and ground based studies

Oscillations in solar atmospheric structures

On the asymmetry of selected Fraunhofer lines

Solar Oscillator Strengths as a Diagnostic Tool

On the microturbulence in the solar photosphere

On the possible mechanism of formation of emission rim in hydrogen filaments

The interpretation of absorption-line shifts in the solar spectrum

Formation of the profiles of absorption lines in the inhomogeneous medium

The NLTE Formation of Iron Lines Used in Solar Polarimetry

On the establishment of internally consistent abundance-oscillator strength scales

Matrix equations for radiation diffusion. II

Matrix equations of radiation diffusion. III

On the microstructure in the solar photosphere

On the asymmetry of selected fraunhofer lines, II

Matrix equations for radiation diffusion. I

Comparative Analysis of Physical Conditions in the Solar and Procyon Atmospheres

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