A Brief History of CME Science

[1]  Bruce T. Tsurutani,et al.  The extreme magnetic storm of 1–2 September 1859 , 2003 .

[2]  D. Alexander,et al.  The active Sun , 2001 .

[3]  O. S. St. Cyr,et al.  Coronal mass ejections, interplanetary ejecta and geomagnetic storms , 2000 .

[4]  Barbara June Thompson,et al.  Relationship of halo coronal mass ejections, magnetic clouds, and magnetic storms , 2000 .

[5]  Christopher T. Russell,et al.  Relationships between coronal mass ejection speeds from coronagraph images and interplanetary characteristics of associated interplanetary coronal mass ejections , 1999 .

[6]  J. Schmelz,et al.  The Many Faces of the Sun , 1999 .

[7]  B. Thompson,et al.  Observations of a Propagating Disturbance in TRACE , 1999 .

[8]  J. B. Gurman,et al.  SOHO/EIT observations of an Earth‐directed coronal mass ejection on May 12, 1997 , 1998 .

[9]  E. Cliver.  Solar activity and geomagnetic storms: From M regions and flares to coronal holes and CMEs , 1995 .

[10]  E. Cliver.  Solar activity and geomagnetic storms: The corpuscular hypothesis , 1994 .

[11]  E. Cliver.  Solar activity and geomagnetic storms: The first 40 years , 1994 .

[12]  E. Cliver.  Was the eclipse comet of 1893 a disconnected coronal mass ejection? , 1989 .

[13]  T. T. von Rosenvinge,et al.  The role of interplanetary shocks in the longitude distribution of solar energetic particles , 1988 .

[14]  H. Rosenbauer,et al.  Coronal mass ejections and interplanetary shocks , 1985 .

[15]  R. Schwenn.  Direct correlation between coronal transients and interplanetary disturbances , 1983 .

[16]  R. Schwenn.  Direct correlations between coronal transients and interplanetary disturbances , 1983 .

[17]  P. McIntosh,et al.  Disappearing solar filaments: A useful predictor of geomagnetic activity , 1981 .

[18]  J. Eddy,et al.  A new sun : the solar results from Skylab , 1979 .

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

[20]  E. Hildner,et al.  The speeds of coronal mass ejection events , 1976 .

[21]  R. MacQueen,et al.  Mass ejections from the Sun: A view from Skylab , 1974 .

[22]  J. Eddy.  Nineteenth-century coronal transient , 1974 .

[23]  T. Hirayama.  Theoretical model of flares and prominences , 1974 .

[24]  A. Hundhausen,et al.  Coronal Expansion and Solar Wind , 1972 .

[25]  A. Hundhausen,et al.  Observation of a solar flare induced interplanetary shock and helium-enriched driver gas , 1970 .

[26]  B. Coppi,et al.  A New Model of Solar Flares , 1964, Nature.

[27]  E. Smith,et al.  EVIDENCE FOR A COLLISION-FREE MAGNETOHYDRODYNAMIC SHOCK IN INTERPLANETARY SPACE , 1964 .

[28]  H. Carmichael,et al.  A process for flares , 1964 .

[29]  T. L. Cline,et al.  Explorer 12 observations of solar cosmic rays and energetic storm particles after the solar flare of September 28, 1961 , 1962 .

[30]  E. Parker.  Sudden Expansion of the Corona Following a Large Solar Flare and the Attendant Magnetic Field and Cosmic-Ray Effects. , 1961 .

[31]  J. H. Piddington.  INTERPLANETARY MAGNETIC FIELD AND ITS CONTROL OF COSMIC-RAY VARIATIONS , 1958 .

[32]  T. Gold,et al.  The cosmic ray flare effect , 1958 .

[33]  E. Parker,et al.  Solar Cosmic Rays of February, 1956 and Their Propagation through Interplanetary Space , 1956 .

[34]  P. Morrison,et al.  Solar Origin of Cosmic-Ray Time Variations , 1956 .

[35]  S. Forbush,et al.  Three Unusual Cosmic-Ray Increases Possibly Due to Charged Particles from the Sun , 1946 .

[36]  H. Newton.  Solar Flares and Magnetic Storms , 1943 .

[37]  M. A. Ellison.  Line-Width Measures and the Observation of a Red-Shift in the Eruptive Hα Line , 1943 .

[38]  S. Forbush.  On the Effects in Cosmic-Ray Intensity Observed During the Recent Magnetic Storm , 1937 .

[39]  H. Newton.  Eruptive dark flocculi and their possible relation to magnetic disturbances , 1936 .

[40]  G. Hale.  The Spectrohelioscope and its Work. Part III. Solar Eruptions and Their Apparent Terrestrial Effects , 1931 .

[41]  G. Hale.  The Spectrohelioscope and its Work , 1929 .

[42]  V. Ferraro,et al.  The Electrical State of Solar Streams of Corpuscles , 1929 .

[43]  S. Chapman.  Solar Streams of Corpuscles: Their Geometry, Absorption of Light, and Penetration , 1929 .

[44]  H. Newton,et al.  Magnetic Storms and Solar Activity, 1874 to 1927 , 1928 .

[45]  F. A. Lindemann.  LXX. Note on the theory of magnetic storms , 1919 .

[46]  George E. Hale,et al.  On the probable existence of a magnetic field in sun‐spots , 1908 .

[47]  George E. Hale,et al.  On the Probable Existence of a Magnetic Field in Sun-Spots , 1908 .

[48]  F. H. Bigelow.  Further study of the solar corona , 1890, American Journal of Science.

[49]  R. C. Carrington.  Description of a Singular Appearance seen in the Sun on September 1, 1859 , 1859 .

[50]  E. Sabine.  On periodical laws discoverable in the mean effects of the larger magnetic disturbances.―No. III , 1857, Proceedings of the Royal Society of London.