Radio observations of the M8.1 solar flare of 23 June, 1988: Evidence for energy transport by thermal processes

[1]  J. Brown,et al.  Interrelation of soft and hard X-ray emissions during solar flares. II, Simulation model , 1991 .

[2]  Gordon J. Hurford,et al.  First interferometric observations of solar microwave millisecond spike bursts , 1991 .

[3]  Gordon J. Hurford,et al.  Multifrequency Observations of a Solar Microwave Burst with Two-dimensional Spatial Resolution , 1990 .

[4]  Haimin Wang,et al.  Microwave structure of the quiet sun at 8.5 GHz , 1990 .

[5]  D. Gary,et al.  The secondary spectral component of solar microwave bursts , 1990 .

[6]  L. Golub,et al.  The M8.1 flare of 23 June, 1988 , 1989 .

[7]  P. Sturrock,et al.  Classification of Solar Flares , 1989 .

[8]  G. J. Hurford,et al.  High-resolution microwave spectra of solar bursts , 1989 .

[9]  F. Fárník,et al.  Flaring arches , 1989 .

[10]  S. Martin,et al.  Flaring arches , 1988 .

[11]  D. Gary,et al.  A simple solar microwave burst observed with high spectral resolution , 1988 .

[12]  Ronald L. Moore,et al.  Evidence that magnetic energy shedding in solar filament eruptions is the drive in accompanying flares and coronal mass ejections , 1988 .

[13]  M. Aschwanden.  Theory of radio pulsations in coronal loops , 1987 .

[14]  C. Sawyer.  Visibility and rate of coronal mass ejections , 1985 .

[15]  Leon Golub,et al.  Construction Of A Multilayered X-Ray Telescope For Solar Coronal Studies From Space , 1985, Optics & Photonics.

[16]  D. Rust,et al.  Observational evidence for thermal wave fronts in solar flares , 1985 .

[17]  G. Dulk,et al.  Radio Emission from the Sun and Stars , 1985 .

[18]  K. Kai,et al.  Microwave and X-ray observations of delayed brightenings at sites remote from the primary flare locations , 1985 .

[19]  Gordon J. Hurford,et al.  A frequency-agile interferometer for solar microwave spectroscopy , 1984 .

[20]  R. Stone,et al.  Type II solar radio bursts, interplanetary shocks, and energetic particle events , 1984 .

[21]  A. Readhead,et al.  Image Formation by Self-Calibration in Radio Astronomy , 1984 .

[22]  S. Kane,et al.  Magnetic changes observed in a solar flare , 1984 .

[23]  Russell A. Howard,et al.  Associations between coronal mass ejections and solar energetic proton events , 1983 .

[24]  E. Priest,et al.  Heating of postflare loops , 1983 .

[25]  M. Kundu,et al.  Observations of H-alpha and microwave brightening caused by a distant solar flare , 1983 .

[26]  E. Priest,et al.  Numerical study of line-tied magnetic reconnection , 1982 .

[27]  S. Kahler.  Radio burst characteristics of solar proton flares , 1982 .

[28]  K. A. Marsh,et al.  Simplified expressions for the gyrosynchrotron radiation from mildly relativistic, nonthermal and thermal electrons , 1982 .

[29]  G. Pneuman.  Energetics of two-ribbon solar flares , 1982 .

[30]  R. Moore,et al.  Remote flare brightenings and type III reverse slope bursts , 1982 .

[31]  D. Melrose,et al.  Production of a collisionless conduction front by rapid coronal heating and its role in solar hard X-ray bursts. , 1979 .

[32]  R. MacQueen,et al.  The association of coronal mass ejection transients with other forms of solar activity , 1979 .

[33]  S. Kahler,et al.  Prompt solar proton events and coronal mass ejections , 1978 .

[34]  G. S. Vaiana,et al.  A survey of soft X-ray limb flare images: the relation between their structure in the corona and other physical parameters. , 1977 .

[35]  R. Kopp,et al.  Magnetic reconnection in the corona and the loop prominence phenomenon , 1976 .

[36]  J. Culhane,et al.  The solar X-ray spectrum , 1974 .

[37]  A. Böhme.  Spectral behaviour and proton effects of the type IV broad-band continua , 1972 .

[38]  H. Hudson,et al.  Soft X-ray and microwave observations of hot regions in solar flares , 1972 .