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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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Citations
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Journal ArticleDOI

A Semi-empirical Approach to the Dynamic Coupling of CMEs and Solar Wind

TL;DR: In this paper , the authors deduce expressions to approximate the main forces that affect the dynamic coupling between CMEs and the surrounding solar wind from a magnetohydrodynamic perspective, combined with a few reasonable assumptions, allowing them to obtain expressions for the thermal and magnetic pressure forces, viscous and dynamic drag, and gravity.
Journal ArticleDOI

Solar Energetic Particle Forecasting Algorithms and Associated False Alarms

TL;DR: A new forecasting algorithm is defined which uses a combination of CME and flare parameters, and it is shown that the false-alarm ratio is similar to that for the algorithm based upon fast CMEs, but the percentage of SEP events not forecast is reduced to 32.4%.
Journal ArticleDOI

An Insight into the Coupling of CME Kinematics in Inner and Outer Corona and the Imprint of Source Regions

TL;DR: In this article, a follow-up statistical study of several 3D kinematic parameters of 59 CMEs studied by Majumdar et al. was conducted, where the source regions were identified and classified as Active Regions (ARs), Active Prominences (APs), and Prominence Eruptions (PEs).
Journal ArticleDOI

Magnetic helicity and free magnetic energy as tools for probing eruptions in two differently evolving solar active regions

TL;DR: In this paper , the instantaneous relative magnetic helicity and free magnetic energy budgets for several days in two solar active regions (ARs), AR11890 and AR11618, were calculated using vector magnetograms from the HMI/SDO and a magnetic connectivity-based method.
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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