3-D GCM modelling of thermospheric nitric oxide during the 2003 Halloween storm

Numerical modelling of thermospheric temperature changes associated with periods of high geomagnetic activity are often inaccurate due to unrealistic representation of nitric oxide (NO) densities and associated 5.3-mu m radiative cooling. In previous modelling studies, simplistic parameterisations o...

Full description

Bibliographic Details
Main Authors: Dobbin, AL, Griffin, EM, Aylward, AD, Millward, GH
Format: Report
Language:unknown
Published: EUROPEAN GEOSCIENCES UNION 2006
Subjects:
Online Access:http://discovery.ucl.ac.uk/142984/
id ftucl:oai:eprints.ucl.ac.uk.OAI2:142984
record_format openpolar
spelling ftucl:oai:eprints.ucl.ac.uk.OAI2:142984 2023-05-15T17:04:17+02:00 3-D GCM modelling of thermospheric nitric oxide during the 2003 Halloween storm Dobbin, AL Griffin, EM Aylward, AD Millward, GH 2006 http://discovery.ucl.ac.uk/142984/ unknown EUROPEAN GEOSCIENCES UNION open In: ANNALES GEOPHYSICAE. (pp. 2403 - 2412). EUROPEAN GEOSCIENCES UNION (2006) atmospheric composition and structure thermosphere-composition and chemistry pressure density and temperature airglow and aurora GEOMAGNETIC STORMS IONOSPHERE SATELLITE OXYGEN Proceedings paper 2006 ftucl 2016-01-15T03:27:24Z Numerical modelling of thermospheric temperature changes associated with periods of high geomagnetic activity are often inaccurate due to unrealistic representation of nitric oxide (NO) densities and associated 5.3-mu m radiative cooling. In previous modelling studies, simplistic parameterisations of NO density and variability have often been implemented in order to constrain thermospheric temperature predictions and post storm recovery timescales during and following periods of high aurora] activity. In this paper we use the University College London (UCL) 3-D Coupled Thermosphere and Middle Atmosphere (CMAT) General Circulation Model to simulate the 11-day period from 23 October to 3 November 2003, during which the Earth experienced some of the largest geomagnetic activity ever recorded; the so called "Halloween storm". This model has recently been updated to include a detailed self consistent calculation of NO production and transport. Temperatures predicted by the model compare well with those observed by the UCL Fabry Perot Interferometer at Kiruna, northern Sweden, when changes in solar and auroral activity are taken into account in the calculation of NO densities. The spatial distribution of predicted temperatures at approximately 250-km altitude is also discussed. Simulated NO densities at approximately 110km are presented. Large quantities of NO are found to be present at to the equator, one to two days after the most intense period of geomagnetic activity. This is the first 3-D GCM simulation of NO production and transport over the 2003 Halloween storm period. Report Kiruna Northern Sweden University College London: UCL Discovery Kiruna
institution Open Polar
collection University College London: UCL Discovery
op_collection_id ftucl
language unknown
topic atmospheric composition and structure
thermosphere-composition and chemistry
pressure
density
and temperature
airglow and aurora
GEOMAGNETIC STORMS
IONOSPHERE
SATELLITE
OXYGEN
spellingShingle atmospheric composition and structure
thermosphere-composition and chemistry
pressure
density
and temperature
airglow and aurora
GEOMAGNETIC STORMS
IONOSPHERE
SATELLITE
OXYGEN
Dobbin, AL
Griffin, EM
Aylward, AD
Millward, GH
3-D GCM modelling of thermospheric nitric oxide during the 2003 Halloween storm
topic_facet atmospheric composition and structure
thermosphere-composition and chemistry
pressure
density
and temperature
airglow and aurora
GEOMAGNETIC STORMS
IONOSPHERE
SATELLITE
OXYGEN
description Numerical modelling of thermospheric temperature changes associated with periods of high geomagnetic activity are often inaccurate due to unrealistic representation of nitric oxide (NO) densities and associated 5.3-mu m radiative cooling. In previous modelling studies, simplistic parameterisations of NO density and variability have often been implemented in order to constrain thermospheric temperature predictions and post storm recovery timescales during and following periods of high aurora] activity. In this paper we use the University College London (UCL) 3-D Coupled Thermosphere and Middle Atmosphere (CMAT) General Circulation Model to simulate the 11-day period from 23 October to 3 November 2003, during which the Earth experienced some of the largest geomagnetic activity ever recorded; the so called "Halloween storm". This model has recently been updated to include a detailed self consistent calculation of NO production and transport. Temperatures predicted by the model compare well with those observed by the UCL Fabry Perot Interferometer at Kiruna, northern Sweden, when changes in solar and auroral activity are taken into account in the calculation of NO densities. The spatial distribution of predicted temperatures at approximately 250-km altitude is also discussed. Simulated NO densities at approximately 110km are presented. Large quantities of NO are found to be present at to the equator, one to two days after the most intense period of geomagnetic activity. This is the first 3-D GCM simulation of NO production and transport over the 2003 Halloween storm period.
format Report
author Dobbin, AL
Griffin, EM
Aylward, AD
Millward, GH
author_facet Dobbin, AL
Griffin, EM
Aylward, AD
Millward, GH
author_sort Dobbin, AL
title 3-D GCM modelling of thermospheric nitric oxide during the 2003 Halloween storm
title_short 3-D GCM modelling of thermospheric nitric oxide during the 2003 Halloween storm
title_full 3-D GCM modelling of thermospheric nitric oxide during the 2003 Halloween storm
title_fullStr 3-D GCM modelling of thermospheric nitric oxide during the 2003 Halloween storm
title_full_unstemmed 3-D GCM modelling of thermospheric nitric oxide during the 2003 Halloween storm
title_sort 3-d gcm modelling of thermospheric nitric oxide during the 2003 halloween storm
publisher EUROPEAN GEOSCIENCES UNION
publishDate 2006
url http://discovery.ucl.ac.uk/142984/
geographic Kiruna
geographic_facet Kiruna
genre Kiruna
Northern Sweden
genre_facet Kiruna
Northern Sweden
op_source In: ANNALES GEOPHYSICAE. (pp. 2403 - 2412). EUROPEAN GEOSCIENCES UNION (2006)
op_rights open
_version_ 1766058354116919296