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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

Simulation of the Solar Energetic Particle Event on 2020 May 29 Observed by Parker Solar Probe

TL;DR: In this article , a stochastic three-dimensional focused transport simulation of solar energetic particles (SEPs) produced by a data-driven coronal mass ejection (CME) shock propagating through a datadriven model of coronal and heliospheric magnetic fields is presented.
Journal ArticleDOI

Automatic Detection of Limb Prominences in 304 A EUV Images

TL;DR: In this article, a new algorithm for automatic detection of prominences on the solar limb in 304 A EUV images is presented, and results of its application to SOHO/EIT data discussed.
Journal ArticleDOI

Ensemble Learning for CME Arrival Time Prediction

TL;DR: In this article , an ensemble learning approach, named CMETNet, was proposed for predicting the arrival time of CMEs from the Sun to the Earth, with a Pearson product-moment correlation coefficient of 0.83 and a mean absolute error of 9.75 hours.
Journal ArticleDOI

Interaction of a coronal mass ejection and a stream interaction region: A case study

TL;DR: In this article , the authors investigated the interaction of a coronal mass ejection (CME) and coronal hole (CH) in its vicinity using remote-sensing and 1 AU in situ data.
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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