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Distribution of sunspot umbral areas: 1917-1982
Hypercharge, solar structure, and stellar evolution
The magnetic and velocity structure adjacent to solar active regions
Depth and latitude dependence of solar rotation
Oscillations in solar models with weakly interacting massive particles
Energetic particle acceleration in spherically symmetrical accretion flows and shocks
Rotation and expansion within sunspot groups
Meridional motions of sunspots and sunspot groups
Nonspherical expansion of radiation-driven winds
Stokes profile analysis and vector magnetic fields. III. Extended temperature minima of sunspot umbrae as inferred from Stokes profiles of Mg I λ4571
Statistical mechanics of partially ionized stellar plasmas: The Planck-Larkin partition function, polarization shifts, and simulations of optical spectra
Simultaneous measurements of sunspot umbral oscillations in the photosphere, chromosphere, and transition region
The polarization properties of model sunspots: The broad-band polarization signature of the Schluter-Temesvary representation
The ejection of helical field structures through the outer corona
Electric current sheet formation in a magnetic field induced by continuous magnetic footpoint displacements
Numerical solution of the magnetostatic equations for thick flux tubes, with application to sunspots, pores, and related structures
Photoelectric observations of chromospheric sunspot oscillations. IV. The Ca II H line and He I λ10830
Relation of chromospheric activity to convection, rotation, and pre-main-sequence evolution
The magnetohydrodynamic stability of coronal arcades. III. Sheared equilibrium fields
Radiative transfer diagnostics - Understanding multilevel transfer calculations. I. Analysis of the full statistical equilibrium equations

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