Journal of Geophysical Research: Space Physics

We report the properties of all the 841 coronal mass ejections (CMEs) observed by the Solar and Heliospheric Observatory (SOHO) Large Angle Spectroscopic Coronagraph (LASCO) C2 and C3 white‐light coronagraphs from January 1996 through June 1998, and we compare those properties to previous observations by other similar instruments. Both the CME rate and the distribution of apparent locations of CMEs varied during this period as expected based on previous solar cycles. The distribution of apparent speeds and the fraction of CMEs showing acceleration were also in agreement with earlier reports. The pointing stability provided by an L‐1 orbit and the use of CCD detectors have resulted in superior brightness sensitivity for LASCO over earlier coronagraphs; however, we have not detected a significant population of fainter (i.e., low mass) CMEs. The general shape of the distribution of apparent sizes for LASCO CMEs is similar to those of earlier reports, but the average (median) apparent size of 72° (50°) is significantly larger. The larger average apparent size is predominantly the result of the detection of a population of partial and complete halo CMEs, at least some of which appear to be events with a significant longitudinal component directed along the Sun‐Earth line, either toward or away from the Earth. Using full disk solar images obtained by the Extreme ultraviolet Imaging Telescope (EIT) on SOHO, we found that 40 out of 92 of these events might have been directed toward the Earth, and we compared the timing of those with the Kp geomagnetic storm index in the days following the CME. Although the “false alarm” rate was high, we found that 15 out of 21 (71%) of the Kp ≥ 6 storms could be accounted for as SOHO LASCO/EIT frontside halo CMEs. If we eliminate three Kp storms that occurred following LASCO/EIT data gaps, then the possible association rate was 15 out of 18 (83%).

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Ana Cristina Chaves

(2011)

10.1190/SBGf2011

Alisson Dal Lago, Walter D. Gonzalez, Carlos R. Braga, Aline de Lucas, Lucas R. Vieira and Tardelli R. C. Stekel

CME dynamics using coronagraph and interplanetary ejecta observations

(2011)

(2014)

10.1190/sbgf2011-427

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T. A. Kuchar, A. Buffington, C. N. Arge, P. P. Hick, T. A. Howard, B. V. Jackson, J. C. Johnston, D. R. Mizuno, S. J. Tappin and D. F. Webb, Observations of a comet tail disruption induced by the passage of a CME, Journal of Geophysical Research: Space Physics, 113, A4, (2008).
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J. M. Schmidt and N. Gopalswamy, Synthetic radio maps of CME‐driven shocks below 4 solar radii heliocentric distance, Journal of Geophysical Research: Space Physics, 113, A8, (2008).
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Maxim L. Khodachenko, Ignasi Ribas, Helmut Lammer, Jean-Mathias Grießmeier, Martin Leitner, Franck Selsis, Carlos Eiroa, Arnold Hanslmeier, Helfried K. Biernat, Charles J. Farrugia and Helmut O. Rucker, Coronal Mass Ejection (CME) Activity of Low Mass M Stars as An Important Factor for The Habitability of Terrestrial Exoplanets. I. CME Impact on Expected Magnetospheres of Earth-Like Exoplanets in Close-In Habitable Zones, Astrobiology, 10.1089/ast.2006.0127, 7, 1, (167-184), (2007).
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Paulo de Tarso

(2007)

10.1190/SBGf2007

A. Dal Lago, W. D. Gonzalez and R. Schwenn

Coronal mass ejection geometry using single coronagraph observations

(2007)

(2014)

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G. Michalek, N. Gopalswamy and S. Yashiro, Prediction of Space Weather Using an Asymmetric Cone Model for Halo CMEs, Solar Physics, 10.1007/s11207-007-9081-8, 246, 2, (399-408), (2007).
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M. L. Mays, O. C. St. Cyr, E. Quémerais, S. Ferron, J.-L. Bertaux, S. Yashiro and R. Howard, An Attempt to Detect Coronal Mass Ejections in Lyman-α Using SOHO Swan, Solar Physics, 10.1007/s11207-007-0196-8, 241, 1, (113-125), (2007).
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T. S. Bastian, Synchrotron Radio Emission from a Fast Halo Coronal Mass Ejection, The Astrophysical Journal, 10.1086/519246, 665, 1, (805-812), (2007).
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Yingna Su, Adriaan Van Ballegooijen, James McCaughey, Edward Deluca, Katharine K. Reeves and Leon Golub, What Determines the Intensity of Solar Flare/CME Events?, The Astrophysical Journal, 10.1086/519679, 665, 2, (1448-1459), (2007).
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Paulo de Tarso

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10.1190/SBGf2007

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Nat Gopalswamy, Coronal mass ejections of solar cycle 23, Journal of Astrophysics and Astronomy, 10.1007/BF02702527, 27, 2-3, (243-254), (2006).
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M. J. Owens, V. G. Merkin and P. Riley, A kinematically distorted flux rope model for magnetic clouds, Journal of Geophysical Research: Space Physics, 111, A3, (2006).
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Alejandro Lara, Nat Gopalswamy, Hong Xie, Eduardo Mendoza‐Torres, Román Pérez‐Eríquez and Gregory Michalek, Are halo coronal mass ejections special events?, Journal of Geophysical Research: Space Physics, 111, A6, (2006).
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T. A. Howard, D. F. Webb, S. J. Tappin, D. R. Mizuno and J. C. Johnston, Tracking halo coronal mass ejections from 0–1 AU and space weather forecasting using the Solar Mass Ejection Imager (SMEI), Journal of Geophysical Research: Space Physics, 111, A4, (2006).
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Y. Liu, J. D. Richardson, J. W. Belcher, C. Wang, Q. Hu and J. C. Kasper, Constraints on the global structure of magnetic clouds: Transverse size and curvature, Journal of Geophysical Research: Space Physics, 111, A12, (2006).
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M. J. Owens, Magnetic cloud distortion resulting from propagation through a structured solar wind: Models and observations, Journal of Geophysical Research: Space Physics, 111, A12, (2006).
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Hans Gleisner and Jürgen Watermann, Concepts of medium-range (1–3 days) geomagnetic forecasting, Advances in Space Research, 10.1016/j.asr.2005.10.010, 37, 6, (1116-1123), (2006).
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H. S. Hudson, J.-L Bougeret and J. Burkepile, Coronal Mass Ejections: Overview of Observations, Space Science Reviews, 10.1007/s11214-006-9009-x, 123, 1-3, (13-30), (2006).
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Yun-Chun Jiang, Le-Ping Li and Li-Heng Yang, The Filament Eruption of 1999 March 21 and Its Associated Coronal Dimmings and CME, Chinese Journal of Astronomy and Astrophysics, 10.1088/1009-9271/6/3/10, 6, 3, (345-353), (2006).
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C. Marque, A. Posner and K.‐L. Klein, Solar Energetic Particles and Radio‐silent Fast Coronal Mass Ejections, The Astrophysical Journal, 10.1086/501157, 642, 2, (1222-1235), (2006).
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Curt A. de Koning, John T. Steinberg, J. T. Gosling, Daniel B. Reisenfeld, Ruth M. Skoug, O. C. St. Cyr, M. L. Malayeri, André Balogh, Adam Rees and D. J. McComas, An unusually fast interplanetary coronal mass ejection observed by Ulysses at 5 AU on 15 November 2003, Journal of Geophysical Research: Space Physics, 110, A1, (2005).
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R.‐S. Kim, K.‐S. Cho, Y.‐J. Moon, Y.‐H. Kim, Y. Yi, M. Dryer, Su‐Chan Bong and Y.‐D. Park, Forecast evaluation of the coronal mass ejection (CME) geoeffectiveness using halo CMEs from 1997 to 2003, Journal of Geophysical Research: Space Physics, 110, A11, (2005).
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Volume105, IssueA8

1 August 2000

Pages 18169-18185

Journal of Geophysical Research: Space Physics

Properties of coronal mass ejections: SOHO LASCO observations from January 1996 to June 1998

Abstract

Number of times cited: 305

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Journal of Geophysical Research: Space Physics

Properties of coronal mass ejections: SOHO LASCO observations from January 1996 to June 1998

Abstract

Number of times cited: 305

RESOURCES

PUBLICATION INFO

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