Impact of January 2005 Solar Proton Events on Chlorine Species
Sudden changes in stratospheric chlorine species in the polar northern atmosphere, caused by the Solar Proton Events (SPEs) of 17 and 20 January 2005, have been investigated and compared with version 4 of the Whole Atmosphere Community Climate Model (WACCM4). We used Aura Microwave Limb Sounder (MLS...
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ftnasantrs:oai:casi.ntrs.nasa.gov:20120008733 2023-05-15T18:02:17+02:00 Impact of January 2005 Solar Proton Events on Chlorine Species Funke, B. Damiani, A. Santee, M. L. Jackman, C. H. Cordero, R. R. Marsh, D. R. Wang, S. Lopez-Puertas, M. Froidevaux, L. von Clarmann, T. Gardini, A. Storini, M. Unclassified, Unlimited, Publicly available October 24, 2011 application/pdf http://hdl.handle.net/2060/20120008733 unknown Document ID: 20120008733 http://hdl.handle.net/2060/20120008733 Copyright, Distribution as joint owner in the copyright CASI Meteorology and Climatology GSFC.JA.5993.2012 2011 ftnasantrs 2019-07-21T06:21:53Z Sudden changes in stratospheric chlorine species in the polar northern atmosphere, caused by the Solar Proton Events (SPEs) of 17 and 20 January 2005, have been investigated and compared with version 4 of the Whole Atmosphere Community Climate Model (WACCM4). We used Aura Microwave Limb Sounder (MLS) measurements to monitor the variability of ClO, HCl, HOCl and Michelson Interferometer for Passive Atmospheric Sounder (MIPAS) on ENVISAT to retrieve ClONO2. SPE-induced chlorine activation has been identified. HCl decrease occurred at nearly all the investigated altitudes with the lowest values (of less than 0.25 ppbv) on 21 January. HOCl was found to be the main active chlorine species under nighttime conditions (with increases of more than 0.2 ppbv) whereas both HOCL and CLO enhancements (about 0.1 ppbv) have been observed at the polar night terminator. Further, small ClO decreases (of less than 0.1 ppbv) and ClONO2 enhancements (~0.2 ppbv) have been observed at higher latitudes (i.e., at nighttime) roughly above 2hPa. While WACCM4 reproduces most of the SPE-induced variability in the chlorine species fairly well, in some particular regions discrepancies between the modeled and measured temporal evolution of the abundances of chlorine species were found. HOCl changes are modelled very well with respect to both magnitude and geographic distribution. ClO decreases are reproduced at high latitudes, whereas ClO enhancements in the terminator region are underestimated and attributed to background variations. WACCM4 also reproduces the HCl depletion in the mesosphere but it does not show the observed decrease below about 2 hPa. Finally, WACCM4 simulations indicate that the observed ClONO2 increase is dominated by background variability, although SPE-induced production might contribute by 0.1 ppbv. Other/Unknown Material polar night NASA Technical Reports Server (NTRS) |
institution |
Open Polar |
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NASA Technical Reports Server (NTRS) |
op_collection_id |
ftnasantrs |
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unknown |
topic |
Meteorology and Climatology |
spellingShingle |
Meteorology and Climatology Funke, B. Damiani, A. Santee, M. L. Jackman, C. H. Cordero, R. R. Marsh, D. R. Wang, S. Lopez-Puertas, M. Froidevaux, L. von Clarmann, T. Gardini, A. Storini, M. Impact of January 2005 Solar Proton Events on Chlorine Species |
topic_facet |
Meteorology and Climatology |
description |
Sudden changes in stratospheric chlorine species in the polar northern atmosphere, caused by the Solar Proton Events (SPEs) of 17 and 20 January 2005, have been investigated and compared with version 4 of the Whole Atmosphere Community Climate Model (WACCM4). We used Aura Microwave Limb Sounder (MLS) measurements to monitor the variability of ClO, HCl, HOCl and Michelson Interferometer for Passive Atmospheric Sounder (MIPAS) on ENVISAT to retrieve ClONO2. SPE-induced chlorine activation has been identified. HCl decrease occurred at nearly all the investigated altitudes with the lowest values (of less than 0.25 ppbv) on 21 January. HOCl was found to be the main active chlorine species under nighttime conditions (with increases of more than 0.2 ppbv) whereas both HOCL and CLO enhancements (about 0.1 ppbv) have been observed at the polar night terminator. Further, small ClO decreases (of less than 0.1 ppbv) and ClONO2 enhancements (~0.2 ppbv) have been observed at higher latitudes (i.e., at nighttime) roughly above 2hPa. While WACCM4 reproduces most of the SPE-induced variability in the chlorine species fairly well, in some particular regions discrepancies between the modeled and measured temporal evolution of the abundances of chlorine species were found. HOCl changes are modelled very well with respect to both magnitude and geographic distribution. ClO decreases are reproduced at high latitudes, whereas ClO enhancements in the terminator region are underestimated and attributed to background variations. WACCM4 also reproduces the HCl depletion in the mesosphere but it does not show the observed decrease below about 2 hPa. Finally, WACCM4 simulations indicate that the observed ClONO2 increase is dominated by background variability, although SPE-induced production might contribute by 0.1 ppbv. |
format |
Other/Unknown Material |
author |
Funke, B. Damiani, A. Santee, M. L. Jackman, C. H. Cordero, R. R. Marsh, D. R. Wang, S. Lopez-Puertas, M. Froidevaux, L. von Clarmann, T. Gardini, A. Storini, M. |
author_facet |
Funke, B. Damiani, A. Santee, M. L. Jackman, C. H. Cordero, R. R. Marsh, D. R. Wang, S. Lopez-Puertas, M. Froidevaux, L. von Clarmann, T. Gardini, A. Storini, M. |
author_sort |
Funke, B. |
title |
Impact of January 2005 Solar Proton Events on Chlorine Species |
title_short |
Impact of January 2005 Solar Proton Events on Chlorine Species |
title_full |
Impact of January 2005 Solar Proton Events on Chlorine Species |
title_fullStr |
Impact of January 2005 Solar Proton Events on Chlorine Species |
title_full_unstemmed |
Impact of January 2005 Solar Proton Events on Chlorine Species |
title_sort |
impact of january 2005 solar proton events on chlorine species |
publishDate |
2011 |
url |
http://hdl.handle.net/2060/20120008733 |
op_coverage |
Unclassified, Unlimited, Publicly available |
genre |
polar night |
genre_facet |
polar night |
op_source |
CASI |
op_relation |
Document ID: 20120008733 http://hdl.handle.net/2060/20120008733 |
op_rights |
Copyright, Distribution as joint owner in the copyright |
_version_ |
1766172098511765504 |