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ZENODO
Dataset . 2021
Data sources: Datacite
image/svg+xml art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos Open Access logo, converted into svg, designed by PLoS. This version with transparent background. http://commons.wikimedia.org/wiki/File:Open_Access_logo_PLoS_white.svg art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos http://www.plos.org/
ZENODO
Dataset . 2021
Data sources: ZENODO
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PDBM-project-for-ICMEs: Earth-directed Interplanetary Coronal Mass Ejections between 1996 and 2018

Authors: Gianluca Napoletano; Raffaello Foldes; Dario Del Moro; Giancarlo De Gasperis; Ajay Kumar Tiwari; Jannis Teunissen;

PDBM-project-for-ICMEs: Earth-directed Interplanetary Coronal Mass Ejections between 1996 and 2018

Abstract

Dataset Description '''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''''' CME data from Richardson & Cane catalog (http://www.srl.caltech.edu/ACE/ASC/DATA/level3/icmetable2.htm) + LASCO CDAW CME List (https://cdaw.gsfc.nasa.gov/CME_list/) Version 3.0 12/04/2021 ICME_complete_dataset_v3.csv column details: CME_num: (int) progressive no. of CME LASCO_Start: (datetime) Date of first appearance of CME in LASCO/C2 coronograph Start_Date: (datetime) Date of CME transit at 20 solar radii Arrival_Date: (datetime) Date of Plasma arrival at L1 (ACE) PE_duration: (hrs) duration of plasma disturbance at L1 Arrival_v: (km/s) CME arrival speed at L1 Transit_time: (hrs) date difference in hours between 'Start_Date' and 'Arrival_Date' Transit_time_err: (hrs) error on the CME transit time between 20 solar radii and 1AU LASCO_Date: (datetime) CME start date as reported in the LASCO/CDAW catalog LASC0_v: (km/s) linear speed of CMEs fastest component LASCO_pa: (deg) CME principal angle, counterclockwise from North LASCO_da: (deg) CME angular width LASCO_halo: (string) 'FH' if LASCO_da>270, 'HH' if LASCO_da>180, 'PH' if LASC_da>90, 'N' otherwise v_r: (km/s) radially de-projected CME speed v_r_err: (km/s) uncertainty of the de-projected speed Theta_source: (arcsec) longitude of the most probable source of the CME Phi_source: (arcsec) co-latitude of the most probable source of the CME source_err: (arcsec) uncertainty of the CME source on the solar disk POS_source_angle: (deg) plane-of-sky angle of the source region of the CME rel_wid: (rad) CME width relative to its lift-off speed and position Mass: (g) Mass estimation of the CME SW_type: Solar wind expected during the ICME propagation, Fast (F) or Slow (S) Bz: (nT) z-component of the magnetic field at L1 DST: (signed int) minimum DST during CME duration at L1 v_r_stat: (km/s) statistical de-projection of the CME linear speed, i.e. v_r_stat=LASCO_v*1.027+41.5 (from Pauris et al. 2020, Space Weather) Accel.: (m/s^2) CME acceleration between the lift-off and 20 solar radii Analityc_w: (km/s) solar wind value obtained via analytic inversion of the Drag-Based Model equations Analityc_gamma: (km^-1) value of the drag parameter obtained via analytic inversion of the Drag-Based Model equations filename: (string) name of the file containing PDBM information from the statistical inversion procedure

Keywords

Database, Probabilistic Drag-Based Model, ICMEs, Space Weather

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selected citations
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popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
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influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
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impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
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