The SOHO LASCO CME Catalog -- Version 2

Fuente: arXiv
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Main Authors: Gopalswamy, Nat, Michałek, Grzegorz, Yashiro, Seiji, Mäkelä, Pertti, Akiyama, Sachiko, Xie, Hong, Vourlidas, Angelos
Format: Preprint
Published: 2024
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author Gopalswamy, Nat
Michałek, Grzegorz
Yashiro, Seiji
Mäkelä, Pertti
Akiyama, Sachiko
Xie, Hong
Vourlidas, Angelos
author_facet Gopalswamy, Nat
Michałek, Grzegorz
Yashiro, Seiji
Mäkelä, Pertti
Akiyama, Sachiko
Xie, Hong
Vourlidas, Angelos
contents This paper provides an update on the coronal mass ejection (CME) catalog maintained at the CDAW Data Center, NASA Goddard Space Flight Center (https://cdaw.gsfc.nasa.gov/CME_list). This is version 2 (v2) of the Catalog that has been made as the default version as of May 1, 2024. The new features of the Catalog v2 are (i) online measurement tool, (ii) combination JavaScript movies from the STEREO and Solar Dynamics Observatory (SDO) missions, and (iii) insertion of newly identified CMEs for the period 1996 to 2004. The CME identification was revisited resulting in a set of $\sim$3000 new CMEs added to the Catalog. A vast majority of these CMEs are weak and narrow. The resulting statistical properties of CMEs are not significantly different from those reported using version 1.
format Preprint
id arxiv_https___arxiv_org_abs_2407_04165
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle The SOHO LASCO CME Catalog -- Version 2
Gopalswamy, Nat
Michałek, Grzegorz
Yashiro, Seiji
Mäkelä, Pertti
Akiyama, Sachiko
Xie, Hong
Vourlidas, Angelos
Solar and Stellar Astrophysics
This paper provides an update on the coronal mass ejection (CME) catalog maintained at the CDAW Data Center, NASA Goddard Space Flight Center (https://cdaw.gsfc.nasa.gov/CME_list). This is version 2 (v2) of the Catalog that has been made as the default version as of May 1, 2024. The new features of the Catalog v2 are (i) online measurement tool, (ii) combination JavaScript movies from the STEREO and Solar Dynamics Observatory (SDO) missions, and (iii) insertion of newly identified CMEs for the period 1996 to 2004. The CME identification was revisited resulting in a set of $\sim$3000 new CMEs added to the Catalog. A vast majority of these CMEs are weak and narrow. The resulting statistical properties of CMEs are not significantly different from those reported using version 1.
title The SOHO LASCO CME Catalog -- Version 2
topic Solar and Stellar Astrophysics
url https://arxiv.org/abs/2407.04165