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Data · dataset · 2026

Mesospheric dynamical changes induced by the solar proton events in October-November 2003

Listed in National Center for Atmospheric Research

The Thermosphere Ionosphere Mesosphere Electrodynamic General Circulation Model (TIME-GCM) was used to study the atmospheric dynamical influence of the solar protons that occurred in Oct-Nov 2003, the fourth largest period of solar proton events (SPEs) measured in the past 40 years.

Description

The highly energetic solar protons produced odd hydrogen (HO x ) and odd nitrogen (NO y ). Significant short-lived ozone decreases (10-70%) followed these enhancements of HO x and NO y and led to a cooling of most of the lower mesosphere.

Temperature changes up to ±2.6 K were computed as well as wind (zonal, meridional, vertical) perturbations up to 20-25% of the background winds as a result of the solar protons. The solar proton-induced mesospheric temperature and wind perturbations diminished over a period of 4-6 weeks after the SPEs. The Joule heating in the mesosphere, induced by the solar protons, was computed to be relatively insignificant for these solar storms.

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National Center for Atmospheric Researchff8f923f-9501-4cd7-9e06-5e7eb311e06310 d agoJSON v1
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concepts[field].local:field:earth-environmentalmapping · data ucar educonnector:data_ucar_edu@1.0.0
concepts[field].local:field:ocean-atmosphericmapping · data ucar educonnector:data_ucar_edu@1.0.0
created_datesource · data ucar educonnector:data_ucar_edu@1.0.0
descriptionsource · data ucar educonnector:data_ucar_edu@1.0.0/notes
publication_datesource · data ucar educonnector:data_ucar_edu@1.0.0
titlesource · data ucar educonnector:data_ucar_edu@1.0.0/title
updated_datesource · data ucar educonnector:data_ucar_edu@1.0.0