About: Understanding large SEP events with the PATH code: Modeling of the 13 December 2006 SEP event

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scholarly article

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rdf:type	Item
description	wetenschappelijk artikel (nl) գիտական հոդված (hy) scholarly article (en) наукова стаття, опублікована в грудні 2010 (uk) im Dezember 2010 veröffentlichter wissenschaftlicher Artikel (de)
publication date	wds:Q58473248-DB2BC8F0-9B1C-402F-B25B-CF4166F6D1D7
publication date	2010-12-01 00:00:00Z (xsd:dateTime)
language of work or name	wds:Q58473248-6ADEBF81-8420-4E11-928E-44162033D79E
language of work or name	English
cites work	wds:Q58473248-177C8681-2DCA-4943-ADA2-7FF78FE0B387 wds:Q58473248-2AB0E8E0-19BA-48A4-AE9B-734859E6801E wds:Q58473248-2D3A2B22-485E-4B1E-8674-88A2AA5A5802 wds:Q58473248-2D97BD66-E3C3-4B38-A5A1-B9547A4E4FF7 wds:Q58473248-2E52D25E-649C-48BB-B210-1B4DDBF023D4 wds:Q58473248-3EC2B3C6-E21F-44CC-B8D4-D2E54E2396BC wds:Q58473248-486B5812-C77A-47BB-91F5-8754794CC711 wds:Q58473248-497064F4-43B6-4AF9-B255-4CBB4EB6BDB7 wds:Q58473248-4E6BBF3C-0555-477B-A574-E49A8867B757 wds:Q58473248-53D8FF5A-03AC-45FD-897E-4D95C7B7C9A2 wds:Q58473248-56E94993-B2E3-419F-8C41-733D4D7132F3 wds:Q58473248-630D2BAC-ACC8-4BD6-A99D-82C11B80D1CA wds:Q58473248-6432470F-A803-473D-959D-C0471116DFC6 wds:Q58473248-759F43F0-E047-496C-9227-8AF7A590C0E4 wds:Q58473248-97E53E3E-3822-4F61-8A93-D05D81F2B277 wds:Q58473248-9AE44798-B987-420A-8712-9BAA6E61F5F1 wds:Q58473248-B58AABF6-1ECD-4DA9-8CF8-F5E22FDDEC47 wds:Q58473248-C2190FCC-A966-419D-AF19-22552346CBD9 wds:Q58473248-C6C353C0-862A-4669-94BE-61C507EB1FDC wds:Q58473248-E3DF2706-51BE-4E26-AF4C-A66BA9A101EB wds:Q58473248-F0DC3040-6D9F-4C94-B4D3-876628DC0AC7 wds:Q58473248-F19B3925-867F-49AB-A874-3D83DA6C4B20 wds:Q58473248-FC6AD118-F3FB-4B7D-ADB4-BF615B9A0647 wds:Q58473248-FEEE4868-1EAD-44E5-A0F6-A7C70305DF19
cites work	Fast and optimal solution to the “Rankine-Hugoniot problem” Shock geometry, seed populations, and the origin of variable elemental composition at high energies in large gradual solar particle events A brief review of “solar flare effects” on the ionosphere Particle acceleration and coronal mass ejection driven shocks: A theoretical model The Solar Isotope Spectrometer for the Advanced Composition Explorer Particle Acceleration at Interplanetary Shocks Acceleration and transport of heavy ions at coronal mass ejection-driven shocks Particle acceleration and coronal mass ejection driven shocks: Shocks of arbitrary strength Energetic particle acceleration and transport at coronal mass ejection-driven shocks Using the path code for modeling gradual SEP events in the inner heliosphere A model for spectral and compositional variability at high energies in large, gradual solar particle events Heavy-ion elemental abundances in large solar energetic particle events and their implications for the seed population A comprehensive view of the 2006 December 13 CME: from the Sun to interplanetary space Particle acceleration at perpendicular shock waves: Model and observations Perpendicular diffusion coefficient for charged particles of arbitrary energy Nonlinear collisionless perpendicular diffusion of charged particles Shock geometry and spectral breaks in large SEP events Simulation results for heavy ion spectral variability in large gradual solar energetic particle events The Ultra-Low-Energy Isotope Spectrometer (ULEIS) for the ACE spacecraft The role of interplanetary scattering in western hemisphere large solar energetic particle events Coronal Mass Ejection Shock and Sheath Structures Relevant to Particle Acceleration Modeling a mixed SEP event with the PATH model: December 13, 2006 The Solar Energetic Particle Event of 14 December 2006 Coronal Mass Ejection (CME)-induced shock formation, propagation and some temporally and spatially developing shock parameters relevant to particle energization
author name string	wds:Q58473248-24AA1AB7-934F-4478-AC66-D8AD99441EC8 wds:Q58473248-334E5CDC-6D6F-407C-9DD7-9947AF3FA7C2 wds:Q58473248-3F47FFD7-4A65-41DB-90D3-0358BC39B36D wds:Q58473248-56F21D7C-0536-4414-9C4D-9BDB1124A94F wds:Q58473248-7A4FC64C-43CF-4D2D-BE0D-0F719A636C9D wds:Q58473248-7DFC817B-CC0D-4389-AFE5-0488E0BAE84B wds:Q58473248-958A754A-F382-4F34-8561-7AB51946E463 wds:Q58473248-CC1C2FC9-AE9A-4C95-A3F4-0C84ADD925DC wds:Q58473248-CF0DF193-C624-41E2-B1E3-173BB1CD334B
author name string	G. Li Q. Hu C. M. S. Cohen R. A. Mewaldt T. T. von Rosenvinge O. P. Verkhoglyadova G. M. Mason M. D. Looper D. K. Haggerty
rdfs:label	Understanding large SEP events with the PATH code: Modeling of the 13 December 2006 SEP event (en) Understanding large SEP events with the PATH code: Modeling of the 13 December 2006 SEP event (nl)
skos:prefLabel	Understanding large SEP events with the PATH code: Modeling of the 13 December 2006 SEP event (en) Understanding large SEP events with the PATH code: Modeling of the 13 December 2006 SEP event (nl)
name	Understanding large SEP events with the PATH code: Modeling of the 13 December 2006 SEP event (en) Understanding large SEP events with the PATH code: Modeling of the 13 December 2006 SEP event (nl)
author	wds:Q58473248-D779020C-739F-45F3-9525-315D0026588A
author	Gary P. Zank
title	wds:Q58473248-4CD43FAB-5CFA-40C8-B479-AA005FB2C3D7
title	Understanding large SEP events with the PATH code: Modeling of the 13 December 2006 SEP event (en)
instance of	wds:Q58473248-77825B84-97D6-4FC4-A4CA-B0F07F7CCE25
instance of	scholarly article
published in	wds:Q58473248-42FBFD4F-C0A0-46CF-AC55-8DAB56B34149
published in	Journal of Geophysical Research
issue	wds:Q58473248-FB62D469-0418-4BC0-BD05-18506A802251
volume	wds:Q58473248-77E44154-63D9-4679-A812-C0651DAE6021
issue	A12
volume	115
DOI	wds:Q58473248-E89BC08F-31FD-457F-9A01-12E55720B87A
DOI	http://dx.doi.org/10.1029/2010JA015615
DOI	10.1029/2010JA015615
ADS bibcode	wds:Q58473248-AD9F05FA-5A30-4C5A-8C40-4E6815C3870A
ADS bibcode	2010JGRA..11512103V
is owl:sameAs of	Understanding large SEP events with the PATH code: Modeling of the 13 December 2006 SEP event

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