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Cloud Formation From a Localized Water Release in the Upper Mesosphere: Indication of Rapid Cooling

Polar mesospheric clouds (PMCs) occur in the summer near 82 ‐85km altitude due to seasonal changes of temperature and humidity. However, water vapor and associated PMCs have also been observed associated with rocket exhaust. The effects of this rocket exhaust on the temperature of the upper mesosphe...

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Autores principales: Collins, Richard L., Stevens, Michael H., Azeem, Irfan, Taylor, Michael J., Larsen, Miguel F., Williams, Bifford P., Li, Jintai, Alspach, Jennifer H., Pautet, Pierre‐Dominique, Zhao, Yucheng, Zhu, Xun
Formato: Online Artículo Texto
Lenguaje:English
Publicado: John Wiley and Sons Inc. 2021
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7988588/
https://www.ncbi.nlm.nih.gov/pubmed/33777609
http://dx.doi.org/10.1029/2019JA027285
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author Collins, Richard L.
Stevens, Michael H.
Azeem, Irfan
Taylor, Michael J.
Larsen, Miguel F.
Williams, Bifford P.
Li, Jintai
Alspach, Jennifer H.
Pautet, Pierre‐Dominique
Zhao, Yucheng
Zhu, Xun
author_facet Collins, Richard L.
Stevens, Michael H.
Azeem, Irfan
Taylor, Michael J.
Larsen, Miguel F.
Williams, Bifford P.
Li, Jintai
Alspach, Jennifer H.
Pautet, Pierre‐Dominique
Zhao, Yucheng
Zhu, Xun
author_sort Collins, Richard L.
collection PubMed
description Polar mesospheric clouds (PMCs) occur in the summer near 82 ‐85km altitude due to seasonal changes of temperature and humidity. However, water vapor and associated PMCs have also been observed associated with rocket exhaust. The effects of this rocket exhaust on the temperature of the upper mesosphere are not well understood. To investigate these effects, 220 kg of pure water was explosively released at 85 km as part of the Super Soaker sounding rocket experiment on the night of January 25–26, 2018 at Poker Flat Research Range (65°N, 147°W). A cloud formed within 18 s and was measured by a ground‐based Rayleigh lidar. The peak altitude of the cloud appeared to descend from 92 to 78 km over 3 min. Temperatures leading up to the release were between 197 and 232 K, about 50 K above the summertime water frost point when PMCs typically occur. The apparent motion of the cloud is interpreted in terms of the expansion of the explosive release. Analysis using a water vapor radiative cooling code coupled to a microphysical model indicates that the cloud formed due to the combined effects of rapid radiative cooling (∼25 K) by meter‐scale filaments of nearly pure water vapor (∼1 ppv) and an increase in the frost point temperature (from 150 to 200 K) due to the high concentration of water vapor. These results indicate that water exhaust not only acts as a reservoir for mesospheric cloud production but also actively cools the mesosphere to induce cloud formation.
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spelling pubmed-79885882021-03-25 Cloud Formation From a Localized Water Release in the Upper Mesosphere: Indication of Rapid Cooling Collins, Richard L. Stevens, Michael H. Azeem, Irfan Taylor, Michael J. Larsen, Miguel F. Williams, Bifford P. Li, Jintai Alspach, Jennifer H. Pautet, Pierre‐Dominique Zhao, Yucheng Zhu, Xun J Geophys Res Space Phys Research Article Polar mesospheric clouds (PMCs) occur in the summer near 82 ‐85km altitude due to seasonal changes of temperature and humidity. However, water vapor and associated PMCs have also been observed associated with rocket exhaust. The effects of this rocket exhaust on the temperature of the upper mesosphere are not well understood. To investigate these effects, 220 kg of pure water was explosively released at 85 km as part of the Super Soaker sounding rocket experiment on the night of January 25–26, 2018 at Poker Flat Research Range (65°N, 147°W). A cloud formed within 18 s and was measured by a ground‐based Rayleigh lidar. The peak altitude of the cloud appeared to descend from 92 to 78 km over 3 min. Temperatures leading up to the release were between 197 and 232 K, about 50 K above the summertime water frost point when PMCs typically occur. The apparent motion of the cloud is interpreted in terms of the expansion of the explosive release. Analysis using a water vapor radiative cooling code coupled to a microphysical model indicates that the cloud formed due to the combined effects of rapid radiative cooling (∼25 K) by meter‐scale filaments of nearly pure water vapor (∼1 ppv) and an increase in the frost point temperature (from 150 to 200 K) due to the high concentration of water vapor. These results indicate that water exhaust not only acts as a reservoir for mesospheric cloud production but also actively cools the mesosphere to induce cloud formation. John Wiley and Sons Inc. 2021-02-22 2021-02 /pmc/articles/PMC7988588/ /pubmed/33777609 http://dx.doi.org/10.1029/2019JA027285 Text en © 2021. The Authors. This is an open access article under the terms of the http://creativecommons.org/licenses/by-nc/4.0/ License, which permits use, distribution and reproduction in any medium, provided the original work is properly cited and is not used for commercial purposes.
spellingShingle Research Article
Collins, Richard L.
Stevens, Michael H.
Azeem, Irfan
Taylor, Michael J.
Larsen, Miguel F.
Williams, Bifford P.
Li, Jintai
Alspach, Jennifer H.
Pautet, Pierre‐Dominique
Zhao, Yucheng
Zhu, Xun
Cloud Formation From a Localized Water Release in the Upper Mesosphere: Indication of Rapid Cooling
title Cloud Formation From a Localized Water Release in the Upper Mesosphere: Indication of Rapid Cooling
title_full Cloud Formation From a Localized Water Release in the Upper Mesosphere: Indication of Rapid Cooling
title_fullStr Cloud Formation From a Localized Water Release in the Upper Mesosphere: Indication of Rapid Cooling
title_full_unstemmed Cloud Formation From a Localized Water Release in the Upper Mesosphere: Indication of Rapid Cooling
title_short Cloud Formation From a Localized Water Release in the Upper Mesosphere: Indication of Rapid Cooling
title_sort cloud formation from a localized water release in the upper mesosphere: indication of rapid cooling
topic Research Article
url https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7988588/
https://www.ncbi.nlm.nih.gov/pubmed/33777609
http://dx.doi.org/10.1029/2019JA027285
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