Filigree, magnetic fields, and flows in the photosphere Zhang YiOddbjørn Engvold OriginalPaper Pages: 1 - 14
The correspondence between x-ray bright points and evolving magnetic features in the quiet sun D. F. WebbS. F. MartinJ. W. Harvey OriginalPaper Pages: 15 - 35
Microwave emission from a sunspot Jeongwoo W. LeeG. J. HurfordDale E. Gary OriginalPaper Pages: 45 - 57
Radio observations of compact solar sources located between sunspots R. A. SychA. M. UralovA. N. Korzhavin OriginalPaper Pages: 59 - 68
A comparison of theoreticalCIV emission line strengths with active region observations obtained with the Solar EUV Rocket Telescope and Spectrograph (SERTS) F. P. KeenanR. J. ThomasV. M. Burke OriginalPaper Pages: 69 - 74
Correction to the field of view for the high altitude observatory mark III K-coronameter D. G. SimeR. R. Fisher OriginalPaper Pages: 75 - 87
Image analysis of the solar corona from the July 11, 1991 eclipse O. T. MatsuuraE. PicazzioR. P. Campos OriginalPaper Pages: 89 - 99
Numerical simulations of fast MHD waves in a coronal plasma K. MurawskiB. Roberts OriginalPaper Pages: 101 - 112
Interactive flare sites within an active region complex G. PolettoG. A. GaryM. E. Machado OriginalPaper Pages: 113 - 140
Magnetic field changes associated with a sub-flare and surge M. J. HagyardE. A. WestJ. E. Smith OriginalPaper Pages: 141 - 153
Alfvén turbulence and the time dependence of non-thermal line broadening in flares David AlexanderAlexander L. MacKinnon OriginalPaper Pages: 155 - 168
Physical properties of white-light flares derived from their center-to-limb distribution Donald F. NeidigPhilip H. WiborgLou B. Gilliam OriginalPaper Pages: 169 - 194
Ground-level energetic solar particle event on 24 May 1990: Possibility of direct solar neutron detection G. A. KovaltsovYu. E. EfimovL. G. Kocharov OriginalPaper Pages: 195 - 198
On the possible physical conditions which result in appearance of low brightness temperature microwave regions on the sun R. Brajša OriginalPaper Pages: 199 - 202