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Journal ArticleDOI

The SOHO/LASCO CME Catalog

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TLDR
The SOHO/LASCO CME catalog as mentioned in this paper is a data base for the analysis of coronal mass ejections (CMEs) in the solar corona.
Abstract
Coronal mass ejections (CMEs) are routinely identified in the images of the solar corona obtained by the Solar and Heliospheric Observatory (SOHO) mission’s Large Angle and Spectrometric Coronagraph (LASCO) since 1996. The identified CMEs are measured and their basic attributes are cataloged in a data base known as the SOHO/LASCO CME Catalog. The Catalog also contains digital data, movies, and plots for each CME, so detailed scientific investigations can be performed on CMEs and the related phenomena such as flares, radio bursts, solar energetic particle events, and geomagnetic storms. This paper provides a brief description of the Catalog and summarizes the statistical properties of CMEs obtained using the Catalog. Data products relevant to space weather research and some CME issues that can be addressed using the Catalog are discussed. The URL of the Catalog is: http://cdaw.gsfc.nasa.gov/CME_list.

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Journal ArticleDOI

Solar Cycle in the Heliosphere and Cosmic Rays

TL;DR: In this article, the cyclic variability of such heliospheric parameters as solar wind speed and density and heliosphere magnetic field, open magnetic flux and latitude variations of the heliope current sheet are reviewed.
Journal ArticleDOI

Statistical Study of Magnetic Nonpotential Measures in Confined and Eruptive Flares

TL;DR: In this article, the authors studied the relation of degree of magnetic nonpotentiality with the observed flare/CME in active regions and found a general relation that degree of non potentiality is positively correlated with the flare strength and the associated CME speeds.
Journal ArticleDOI

Identification of Super- and Sub-critical Regions in Shocks driven by Coronal Mass Ejections

TL;DR: In this paper, white-light coronagraphic images were used to estimate the compression ratio X = rho_d/rho_u all along the front of CME-driven shocks.
Journal ArticleDOI

The Effects of Uncertainty in Initial CME Input Parameters on Deflection, Rotation, Bz, and Arrival Time Predictions

TL;DR: In this article, the authors explore the effects of different background magnetic field models and find that the changes in deflection and rotation resulting from the uncertainty in the initial parameters tend to exceed the changes from dierent magnetic backgrounds.
References
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Journal ArticleDOI

The Large Angle Spectroscopic Coronagraph (LASCO): Visible light coronal imaging and spectroscopy

TL;DR: The Large Angle Spectroscopic Coronagraph (LASCO) is a triple coronagraph being jointly developed for the Solar and Heliospheric Observatory (SOHO) mission as discussed by the authors.
Book ChapterDOI

The Large Angle Spectroscopic Coronagraph (LASCO)

TL;DR: The Large Angle Spectroscopic Coronagraph (LASCO) is a three coronagraph package which has been jointly developed for the Solar and Heliospheric Observatory (SOHO) mission by the Naval Research Laboratory (USA), the Laboratoire d'Astronomie Spatiale (France), the Max-Planck-Institut fur Aeronomie (Germany), and the University of Birmingham (UK) as discussed by the authors.
Journal ArticleDOI

Waves: The Radio and Plasma Wave Investigation on the Wind Spacecraft

TL;DR: The WAVES investigation on the WIND spacecraft will provide comprehensive measurements of the radio and plasma wave phenomena which occur in Geospace as mentioned in this paper, in coordination with the other onboard plasma, energetic particles, and field measurements will help us understand the kinetic processes that are important in the solar wind and in key boundary regions of the Geospace.
Journal ArticleDOI

Interplanetary acceleration of coronal mass ejections

TL;DR: In this article, an empirical model was proposed to predict the arrival of CMEs at 1 AU, based on the relation between the acceleration and initial speed of the CME.
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