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Model solar chromosphere with prescribed heating

The Astrophysical journal, 1989-11, Vol.346 (2), p.1010-1018

1989

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Chromospheric and coronal heating

The Astrophysical journal, 1989-01, Vol.336 (2), p.1089-1091

1989

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A model of the solar chromosphere-corona transition region based on classical thermal conduction

The Astrophysical journal, 1990-10, Vol.362 (1), p.364-369

ATHAY, R. G

1990

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Temperature and center-limb variations of transition region velocities

The Astrophysical journal, 1989-11, Vol.346 (1), p.514-522

1989

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Chromosphere-corona transition region models with magnetic field and fluid flow

The Astrophysical journal, 1981-10, Vol.249, p.340

Athay, R. G.

1981

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The role of spicules in heating the solar atmosphere

The Astrophysical journal, 1982-04, Vol.255, p.743

1982

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Bifurcation in the low chromosphere

The Astrophysical journal, 1990-08, Vol.358 (2), p.710-717

1990

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Responses of transition region models to magnetic field geometry and downflow velocities

The Astrophysical journal, 1982-12, Vol.263, p.982

Athay, R. G.

1982

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Chromospheric and coronal heating by sound waves

The Astrophysical journal, 1978-12, Vol.226, p.1135

1978

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Velocity effects on the profiles of H? and two FeI lines

Solar physics, 1970-05, Vol.12 (2)

Athay, R.G.

1970

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Stellar chromospheres and coronae

The Astrophysical journal, 1981-11, Vol.250, p.709

Athay, R. G.

1981

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Analysis of the prominence associated with the coronal mass ejection of August 18, 1980

Journal of Geophysical Research, 1986-10, Vol.91 (A10), p.10961-10973

1986

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The magnetic and velocity structure adjacent to solar active regions

The Astrophysical journal, 1987-07, Vol.318 (1), p.437-444

1987

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Magnetic shear. III - Hale region 17255

The Astrophysical journal, 1986-04, Vol.303 (2), p.877-883

1986

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Theoretical Line Intensities. VIII. Comment on the Effectively Thin Approximation

The Astrophysical journal, 1969-07, Vol.157, p.281

Athay, R. Grant

1969

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Characteristics of the expansion associated with eruptive prominences

Solar physics, 1987-01, Vol.110 (2), p.359-379

1987

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Steady flows in the solar transition region observed with SMM

The Astrophysical journal, 1981-12, Vol.251, p.L115

1981

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A Non-Lte Line-Blanketed Solar Model

The Astrophysical journal, 1970-01, Vol.161, p.713

Athay, R. Grant

1970

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Probabilistic radiative transfer - an integral-equation approach

The Astrophysical journal, 1976-02, Vol.204, p.160

Athay, R. G.

1976

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Excitation of Chromospheric he I

The Astrophysical journal, 1963-04, Vol.137, p.931

Athay, R. Grant

1963

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Magnetic shear. IV - Hale regions 16740, 16815, and 16850

The Astrophysical journal, 1986-04, Vol.303 (2), p.884-891

1986

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Temporal and Spatial Fluctuations in Widths of solar Euv Lines

International Astronomical Union Colloquium, 1980, Vol.51, p.53-53

1980

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A Probabilistic Formulation of the Noncoherent-Scattering Problem

The Astrophysical journal, 1972-01, Vol.176, p.659

Athay, R. Grant

1972

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Chromospheric oscillations observed with OSO 8. IV - Power and phase spectra for C IV

The Astrophysical journal, 1979-05, Vol.229, p.1147

1979

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Phase Differences Between Intensity and Doppler Shift and Between Two EUV Emission Lines of Sill For 300 Second and 95 Second Chromospheric Oscillations

International Astronomical Union Colloquium, 1977-07, Vol.43, p.13-13

1977

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Model solar chromosphere with prescribed heating

Chromospheric and coronal heating

A model of the solar chromosphere-corona transition region based on classical thermal conduction

Temperature and center-limb variations of transition region velocities

Chromosphere-corona transition region models with magnetic field and fluid flow

The role of spicules in heating the solar atmosphere

Bifurcation in the low chromosphere

Responses of transition region models to magnetic field geometry and downflow velocities

Chromospheric and coronal heating by sound waves

Velocity effects on the profiles of H? and two FeI lines

Stellar chromospheres and coronae

Analysis of the prominence associated with the coronal mass ejection of August 18, 1980

The magnetic and velocity structure adjacent to solar active regions

Magnetic shear. III - Hale region 17255

Theoretical Line Intensities. VIII. Comment on the Effectively Thin Approximation

Characteristics of the expansion associated with eruptive prominences

Steady flows in the solar transition region observed with SMM

A Non-Lte Line-Blanketed Solar Model

Probabilistic radiative transfer - an integral-equation approach

Excitation of Chromospheric he I

Magnetic shear. IV - Hale regions 16740, 16815, and 16850

Temporal and Spatial Fluctuations in Widths of solar Euv Lines

A Probabilistic Formulation of the Noncoherent-Scattering Problem

Chromospheric oscillations observed with OSO 8. IV - Power and phase spectra for C IV

Phase Differences Between Intensity and Doppler Shift and Between Two EUV Emission Lines of Sill For 300 Second and 95 Second Chromospheric Oscillations

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