The flare of September 7, 1973: A typical example of a newly recognized class of solar transients

[1]  R. Petrasso,et al.  Study of the post-flare loops on 29 July 1973 , 1979 .

[2]  S. Martin Study of the post-flare loops on 29 July 1973 , 1979 .

[3]  S. Antiochos,et al.  The evolution of soft X-ray-emitting flare loops , 1979 .

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

[5]  D. Rust,et al.  Physical parameters in long-decay coronal enhancements , 1979 .

[6]  G. Withbroe The thermal phase of a large solar flare. [Skylab observations , 1978 .

[7]  R. Noyes,et al.  Lyman continuum observations of solar flares , 1978 .

[8]  P. Foukal Magnetic loops, downflows, and convection in the solar corona , 1978 .

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

[10]  P. Sturrock,et al.  Evaporative cooling of flare plasma , 1978 .

[11]  R. Rosner,et al.  Dynamics of the quiescent solar corona , 1978 .

[12]  E. Schmahl,et al.  Coronal mass-ejections-kinematics of the 19 December 1973 event , 1977 .

[13]  Chung-Chieh Cheng Evolution of the high-temperature plasma in the 15 June 1973 flare , 1977 .

[14]  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 .

[15]  S. Kahler The morphological and statistical properties of solar X-ray events with long decay times , 1977 .

[16]  E. M. Reeves,et al.  Extreme uv spectroheliometer on the Apollo Telescope Mount. , 1977, Applied optics.

[17]  E. Tandberg-Hanssen,et al.  Coronal plasma parameters in a long-duration X-ray event observed by Skylab , 1977 .

[18]  A. Poland,et al.  Interpretation of broad-band polarimetry of solar coronal transients - Importance of H-alpha emission , 1976 .

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

[20]  S. Kahler Determination of the energy or pressure of a solar X-ray structure using X-ray filtergrams from a single filter , 1976 .

[21]  David F. Webb,et al.  Coronal X-ray enhancements associated with Hα filament disappearances , 1976 .

[22]  P. Sturrock,et al.  Influence of magnetic field structure on the conduction cooling of flare loops , 1976 .

[23]  G. Vaiana,et al.  Spatial structure and temporal development of a solar X-ray flare observed from Skylab on June 15, 1973 , 1975 .

[24]  J. D. Bohlin,et al.  Coronal changes associated with a disappearing filament , 1975 .

[25]  K. Ohki Expansion of chromospheric matter in the gradual phase of solar flares , 1975 .

[26]  J. D. Bohlin,et al.  The sources of material comprising a mass ejection coronal transient , 1975 .

[27]  A. Poland,et al.  Direct observations of a flare related coronal and solar wind disturbance , 1975 .

[28]  K. Widing,et al.  On the Fe XXIV emission in the solar flare of 1973 June 15 , 1974 .

[29]  E. Hildner,et al.  The High Altitude Observatory White Light Coronagraph , 1974, Other Conferences.

[30]  K. Dere,et al.  The spectral dependence of solar soft X-ray flux values obtained by SOLRAD 9 , 1974 .

[31]  P. Kupferman,et al.  Spectrograph, filtergraph and magnetograph observations of the two-ribbon flare of 29 July, 1973 , 1974 .

[32]  W. M. Neupert,et al.  Spatial distribution of soft X-ray and EUV emission associated with a chromospheric flare of importance 1B on August 2, 1972 , 1973 .

[33]  J. L. Culhane,et al.  The cooling of flare produced plasmas in the solar corona , 1970 .

[34]  A. Bruzek On the Association Between Loop Prominences and Flares. , 1964 .

[35]  A. Krieger The decay of coronal loops brightened by flares and transients , 1978 .

[36]  D. Horan Electron temperature and emission measure variations during solar X-ray flares , 1971 .

[37]  A. Dupree,et al.  Calculations of ionization equilibria for oxygen, neon, silicon, and iron. , 1969 .