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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

The Dynamics of Stellar Coronae Harboring Hot-jupiters II. A Space Weather Event on A Hot-jupiter

TL;DR: In this paper, the effects of a coronal mass ejection (CME) event on a close-in giant planet in an extrasolar system were modeled in a similar manner as in simulations of space weather events on Earth.
Journal ArticleDOI

How is open solar magnetic flux lost over the solar cycle

TL;DR: In this paper, the authors reconstruct open solar flux over the last three solar cycles and demonstrate that the loss term may be related to the degree to which the heliospheric current sheet is warped, i.e., locally tilted from the solar rotation direction.
Journal ArticleDOI

The height evolution of the `true' CME mass derived from STEREO COR1 and COR2 observations

TL;DR: In this article, the authors derived deprojected CME kinematics and CME ''true'' mass evolutions for a sample of 25 events that occurred during December 2007 to April 2011.
Journal ArticleDOI

The Solar Connection of Enhanced Heavy Ion Charge States in the Interplanetary Medium: Implications for the Flux-Rope Structure of CMEs

TL;DR: In this paper, the authors investigated a set of 54 interplanetary coronal mass ejection (ICME) events whose solar sources are very close to the disk center (within ± 15∘ from the central meridian).
Journal ArticleDOI

Temperature of the Source Plasma in Gradual Solar Energetic Particle Events

TL;DR: In this article, the power-law dependence of element abundance enhancements vs suppressions in solar energetic particle (SEP) events has been investigated and a new method to determine the most probable value of $T$676 for these events in the energy region was proposed.
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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