About: Composition changes after the "Halloween" solar proton event: the High Energy Particle Precipitation in the Atmosphere (HEPPA) model versus MIPAS data intercomparison study

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About: Composition changes after the "Halloween" solar proton event: the High Energy Particle Precipitation in the Atmosphere (HEPPA) model versus MIPAS data intercomparison study Goto Sponge NotDistinct Permalink

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scholarly article

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rdf:type	Item
description	wetenschappelijk artikel (nl) scholarly article (en) наукова стаття, опублікована у вересні 2011 (uk) article scientifique publié en 2011 (fr) im September 2011 veröffentlichter wissenschaftlicher Artikel (de)
publication date	wds:Q58093235-771CD0F9-E48A-4C8B-9B2A-2F9A6E1FB07F
publication date	2011-09-05 00:00:00Z (xsd:dateTime)
language of work or name	wds:Q58093235-733B8E05-8BDD-4E65-BED6-6A8BC0362CC3
language of work or name	English
author name string	wds:Q58093235-100E62E5-E3B1-48F5-B133-C1EFE54D2A63 wds:Q58093235-577618DB-AC9B-423D-B817-6DEDE4181835 wds:Q58093235-7E8BBDDA-F259-4A1D-B101-D99BB8F5EFDE wds:Q58093235-9997FA7B-56A7-440B-9D8A-50AEF70E09A5 wds:Q58093235-BAC369EB-E215-4014-82CC-110F4D470F14 wds:Q58093235-BCDD292F-64DC-4D86-A190-F9A533C7B72E wds:Q58093235-CCF158AE-6BF7-45ED-9DD7-5C17D154E831 wds:Q58093235-D349E4B6-A179-4CDC-84E9-F4465A21DB18 wds:Q58093235-D3522747-51B0-4CD7-A7A8-D4A8B7B3D6B2 wds:Q58093235-EE73C2C6-4955-4D36-A8C3-583A85D6FA6C wds:Q58093235-F14EEFDF-C3C1-401D-A82A-3ACA6956722A wds:Q58093235-F804B99D-9535-4F4C-861D-5E9698EC8356
author name string	D. R. Marsh C. H. Jackman A. Baumgaertner T. Egorova A. Krivolutsky J. Kieser J. M. Wissing M. Calisto S. Versick S.-M. Salmi T. Reddmann T. Y. Vyushkova
rdfs:label	Composition changes after the "Halloween" solar proton event: the High Energy Particle Precipitation in the Atmosphere (HEPPA) model versus MIPAS data intercomparison study (en) Composition changes after the "Halloween" solar proton event: the High Energy Particle Precipitation in the Atmosphere (nl)
skos:prefLabel	Composition changes after the "Halloween" solar proton event: the High Energy Particle Precipitation in the Atmosphere (HEPPA) model versus MIPAS data intercomparison study (en) Composition changes after the "Halloween" solar proton event: the High Energy Particle Precipitation in the Atmosphere (nl)
name	Composition changes after the "Halloween" solar proton event: the High Energy Particle Precipitation in the Atmosphere (HEPPA) model versus MIPAS data intercomparison study (en) Composition changes after the "Halloween" solar proton event: the High Energy Particle Precipitation in the Atmosphere (nl)
author	wds:Q58093235-0277B65C-006C-47D7-B44F-7BBE589AD2D9 wds:Q58093235-0BEE1040-4C15-48A5-AE2B-B7E78D7F4A64 wds:Q58093235-44703162-16A3-411B-AFE2-EBBF786A7BE5 wds:Q58093235-7C7CA4C4-7762-422D-84C3-52697D71DE6A wds:Q58093235-7F4FCD8B-9136-4E92-96DF-055FB6663C59 wds:Q58093235-84EE747E-DF7E-45E6-98DC-11319EF04499 wds:Q58093235-AEE1FC5C-0B57-469F-BFD5-5F0D8CB3E8D5 wds:Q58093235-FBAD2CDD-238A-4214-AB6A-E2FC24AD98FA
author	Bernd Funke Manuel López-Puertas Thomas von Clarmann Miriam Sinnhuber Nadine Wieters Gabriele Stiller Eugene Rozanov P. T. Verronen
title	wds:Q58093235-8CDBBE4C-0366-4C16-8AD3-26F262215F9C
title	Composition changes after the "Halloween" solar proton event: the High Energy Particle Precipitation in the Atmosphere (HEPPA) model versus MIPAS data intercomparison study (en)
page(s)	wds:Q58093235-BF9E0BE4-1C26-4632-865A-8EBE7D1DBD0A
page(s)	9089-9139
instance of	wds:Q58093235-E9C64F4E-B4F5-4D9A-89B4-BD6AF41CAF19
instance of	scholarly article
main subject	wds:Q58093235-03ACC295-D394-42B6-A9D8-6C9B3230F21A wds:Q58093235-39694D7C-E83A-42EB-B365-A14468E63CE3
main subject	atmospheric sciences atmosphere
published in	wds:Q58093235-9B220FD6-09EF-4A43-8E41-D4A979A22005
published in	Atmospheric Chemistry and Physics
issue	wds:Q58093235-45B78B34-E434-4669-8E48-BA14DC49D393
volume	wds:Q58093235-61C23F87-15B9-4709-9751-0955B4769A1E
issue	17
volume	11
DOI	wds:Q58093235-D760B9A4-D4A5-44DB-BA0D-BB57BEA7EB4E
DOI	http://dx.doi.org/10.5194/ACP-11-9089-2011
DOI	10.5194/ACP-11-9089-2011
copyright license	wds:Q58093235-5582d224-6093-4933-80ea-e0e6573473b2
copyright status	wds:Q58093235-b57dc593-8399-47f7-aaa4-2fd750712ed5
copyright license	Creative Commons Attribution 3.0 Unported
copyright status	copyrighted
ADS bibcode	wds:Q58093235-86451F7A-8C4B-4450-A875-4E1F61639B4E
ADS bibcode	2011ACP....11.9089F
is about of	https://www.wikidata.org/wiki/Special:EntityData/Q58093235
is cites work of	Energetic Particle Influence on the Earth’s Atmosphere Ionization of the Polar Atmosphere by Energetic Electron Precipitation Retrieved From Balloon Measurements Solar signals in CMIP-5 simulations: the stratospheric pathway Nitric oxide response to the April 2010 electron precipitation event - using WACCM and WACCM-D with and without medium energy electrons WACCM-D-Whole Atmosphere Community Climate Model with D-region ion chemistry Missing driver in the Sun-Earth connection from energetic electron precipitation impacts mesospheric ozone Polar Ozone Response to Energetic Particle Precipitation Over Decadal Time Scales: The Role of Medium-Energy Electrons What is the solar influence on climate? Overview of activities during CAWSES-II The strength of the meridional overturning circulation of the stratosphere. Toward a comprehensive global electric circuit model: Atmospheric conductivity and its variability in CESM1(WACCM) model simulations Effects of solar proton events on dayglow observed by the TIMED/SABER satellite Reconciling differences in stratospheric ozone composites Transport versus energetic particle precipitation: Northern polar stratospheric NO x and ozone in January-March 2012 Observed effects of solar proton events and sudden stratospheric warmings on odd nitrogen and ozone in the polar middle atmosphere Hemispheric distributions and interannual variability of NOyproduced by energetic particle precipitation in 2002-2012 Simulation of energetic particle precipitation effects during the 2003-2004 Arctic winter The response of mesospheric NO to geomagnetic forcing in 2002-2012 as seen by SCIAMACHY WACCM-D-Improved modeling of nitric acid and active chlorine during energetic particle precipitation

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