Formation of large NAT particles and denitrification in polar stratosphere: possible role of cosmic rays and effect of solar activity

The formation of large nitric acid trihydrate (NAT) particles has important implications for denitrification and ozone depletion. Existing theories have difficulty in explaining the formation of large NAT particles at temperatures above the ice frost point, which has been observed recently over wide...

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Published in:Atmospheric Chemistry and Physics
Main Author: Yu, F.
Format: Text
Language:English
Published: 2018
Subjects:
Online Access:https://doi.org/10.5194/acp-4-2273-2004
https://www.atmos-chem-phys.net/4/2273/2004/
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spelling ftcopernicus:oai:publications.copernicus.org:acp3645 2023-05-15T15:11:09+02:00 Formation of large NAT particles and denitrification in polar stratosphere: possible role of cosmic rays and effect of solar activity Yu, F. 2018-06-28 application/pdf https://doi.org/10.5194/acp-4-2273-2004 https://www.atmos-chem-phys.net/4/2273/2004/ eng eng doi:10.5194/acp-4-2273-2004 https://www.atmos-chem-phys.net/4/2273/2004/ eISSN: 1680-7324 Text 2018 ftcopernicus https://doi.org/10.5194/acp-4-2273-2004 2019-12-24T09:59:15Z The formation of large nitric acid trihydrate (NAT) particles has important implications for denitrification and ozone depletion. Existing theories have difficulty in explaining the formation of large NAT particles at temperatures above the ice frost point, which has been observed recently over wide Arctic regions. Our analyses reveal that high-energy comic ray particles might induce the freezing of supercooled HNO 3 -H 2 O-H 2 SO 4 droplets when they penetrate these thermodynamically unstable droplets. The cosmic ray-induced freezing (CRIF) appears to be consistent with the observed, highly selective formation of NAT particles. We suggest a possible physical process behind the CRIF mechanism: the reorientation of polar solution molecules into the crystalline configuration in the strong electrical fields of moving secondary ions generated by passing cosmic rays. A simple formula connecting the CRIF rate to cosmic ray flux is derived with an undefined parameter constrained by observed NAT formation rates. Our simulations indicate that strong solar proton events (SPEs) may significantly enhance the formation of large NAT particles and denitrification. The CRIF mechanism offers a possible explanation for the observed high correlations between the thin nitrate-rich layers in polar ice cores and major SPEs, and the observed enhancement in the aerosol backscattering ratio at PSC layers shortly after an SPE and the significant precipitation velocity of the enhanced PSC layers. The key uncertainty in the CRIF mechanism is the probability ( P ) of freezing when a CR particle hits a thermodynamically, unstable STS droplet. Further studies are needed to either confirm or reject the CRIF hypothesis. Text Arctic Copernicus Publications: E-Journals Arctic Atmospheric Chemistry and Physics 4 9/10 2273 2283
institution Open Polar
collection Copernicus Publications: E-Journals
op_collection_id ftcopernicus
language English
description The formation of large nitric acid trihydrate (NAT) particles has important implications for denitrification and ozone depletion. Existing theories have difficulty in explaining the formation of large NAT particles at temperatures above the ice frost point, which has been observed recently over wide Arctic regions. Our analyses reveal that high-energy comic ray particles might induce the freezing of supercooled HNO 3 -H 2 O-H 2 SO 4 droplets when they penetrate these thermodynamically unstable droplets. The cosmic ray-induced freezing (CRIF) appears to be consistent with the observed, highly selective formation of NAT particles. We suggest a possible physical process behind the CRIF mechanism: the reorientation of polar solution molecules into the crystalline configuration in the strong electrical fields of moving secondary ions generated by passing cosmic rays. A simple formula connecting the CRIF rate to cosmic ray flux is derived with an undefined parameter constrained by observed NAT formation rates. Our simulations indicate that strong solar proton events (SPEs) may significantly enhance the formation of large NAT particles and denitrification. The CRIF mechanism offers a possible explanation for the observed high correlations between the thin nitrate-rich layers in polar ice cores and major SPEs, and the observed enhancement in the aerosol backscattering ratio at PSC layers shortly after an SPE and the significant precipitation velocity of the enhanced PSC layers. The key uncertainty in the CRIF mechanism is the probability ( P ) of freezing when a CR particle hits a thermodynamically, unstable STS droplet. Further studies are needed to either confirm or reject the CRIF hypothesis.
format Text
author Yu, F.
spellingShingle Yu, F.
Formation of large NAT particles and denitrification in polar stratosphere: possible role of cosmic rays and effect of solar activity
author_facet Yu, F.
author_sort Yu, F.
title Formation of large NAT particles and denitrification in polar stratosphere: possible role of cosmic rays and effect of solar activity
title_short Formation of large NAT particles and denitrification in polar stratosphere: possible role of cosmic rays and effect of solar activity
title_full Formation of large NAT particles and denitrification in polar stratosphere: possible role of cosmic rays and effect of solar activity
title_fullStr Formation of large NAT particles and denitrification in polar stratosphere: possible role of cosmic rays and effect of solar activity
title_full_unstemmed Formation of large NAT particles and denitrification in polar stratosphere: possible role of cosmic rays and effect of solar activity
title_sort formation of large nat particles and denitrification in polar stratosphere: possible role of cosmic rays and effect of solar activity
publishDate 2018
url https://doi.org/10.5194/acp-4-2273-2004
https://www.atmos-chem-phys.net/4/2273/2004/
geographic Arctic
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genre Arctic
genre_facet Arctic
op_source eISSN: 1680-7324
op_relation doi:10.5194/acp-4-2273-2004
https://www.atmos-chem-phys.net/4/2273/2004/
op_doi https://doi.org/10.5194/acp-4-2273-2004
container_title Atmospheric Chemistry and Physics
container_volume 4
container_issue 9/10
container_start_page 2273
op_container_end_page 2283
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