New stratospheric dust belt due to the Chelyabinsk bolide
The Ozone Mapping Profiler Suite (OMPS) Limb Profiler (LP) on the recently launched NASA/NOAA NPP/Suomi satellite detected aerosol excess in the mid‐stratosphere (25–45 km altitude) between 50°N and 70°N latitudes. OMPS/LP observations trace this aerosol plume to the meteor that struck near Chelyabi...
Gespeichert in:
| Veröffentlicht in: | Geophysical research letters 2013-09, Vol.40 (17), p.4728-4733 |
|---|---|
| Hauptverfasser: | , , , , |
| Format: | Artikel |
| Sprache: | eng |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
| container_end_page | 4733 |
|---|---|
| container_issue | 17 |
| container_start_page | 4728 |
| container_title | Geophysical research letters |
| container_volume | 40 |
| creator | Gorkavyi, Nick Rault, D. F. Newman, P. A. da Silva, A. M. Dudorov, A. E. |
| description | The Ozone Mapping Profiler Suite (OMPS) Limb Profiler (LP) on the recently launched NASA/NOAA NPP/Suomi satellite detected aerosol excess in the mid‐stratosphere (25–45 km altitude) between 50°N and 70°N latitudes. OMPS/LP observations trace this aerosol plume to the meteor that struck near Chelyabinsk, Russia on 15 February 2013. This new dust layer, located above the Junge aerosol layer, has persisted over at least a 3 month period. Material collected on the ground following the bolide explosion showed that the meteor was mostly composed of olivine and pyroxenes. Simulations using Lagrangian and Eulerian atmospheric models trace the plume back to Chelyabinsk and confirm that the plume altitude was at altitudes between 25 and 45 km. The models also confirm the plume circumpolar longitudinal spreading observed by OMPS/LP, with propagation speeds up to 85 m/s.
Key Points
Simulations using atmospheric models confirm that the belt related to bolide
Limb profiler has proven to be a valuable tool to track the meteor plume |
| doi_str_mv | 10.1002/grl.50788 |
| format | Article |
| fullrecord | <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_miscellaneous_1529952562</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>1529952562</sourcerecordid><originalsourceid>FETCH-LOGICAL-a4928-14a1e4dc6f1703f36362a6f0d99dac34604f6203af9a7b9cfc4cf5556e99016b3</originalsourceid><addsrcrecordid>eNp1kD1PwzAQhi0EEqUw8A8iscCQ9hx_JB5RBSlSBaICMVqOY9O0aVNsR6X_nkCAAYnp3uF57k4vQucYRhggGb-6esQgzbIDNMCC0jgDSA_RAEB0OUn5MTrxfgkABAgeIHFvdpEPToXGbxfGVToqWx-iwtShSyYKTRQWJposTL1XRbXxq6ho6qo0p-jIqtqbs-85RM-3N0-TaTx7yO8m17NYUZFkMaYKG1pqbnEKxBJOeKK4hVKIUmlCOVDLEyDKCpUWQltNtWWMcSMEYF6QIbrs925d89YaH-S68trUtdqYpvUSs0QIljCedOjFH3TZtG7TfScxp92RjDLRUVc9pV3jvTNWbl21Vm4vMcjPEmVXovwqsWPHPburarP_H5T5fPZjxL1R-WDefw3lVpKnJGXy5T6X4nGa42xOZU4-AAUigII</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>1642038459</pqid></control><display><type>article</type><title>New stratospheric dust belt due to the Chelyabinsk bolide</title><source>Wiley Online Library Journals Frontfile Complete</source><source>Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals</source><source>Wiley Free Content</source><source>Wiley-Blackwell AGU Digital Library</source><creator>Gorkavyi, Nick ; Rault, D. F. ; Newman, P. A. ; da Silva, A. M. ; Dudorov, A. E.</creator><creatorcontrib>Gorkavyi, Nick ; Rault, D. F. ; Newman, P. A. ; da Silva, A. M. ; Dudorov, A. E.</creatorcontrib><description>The Ozone Mapping Profiler Suite (OMPS) Limb Profiler (LP) on the recently launched NASA/NOAA NPP/Suomi satellite detected aerosol excess in the mid‐stratosphere (25–45 km altitude) between 50°N and 70°N latitudes. OMPS/LP observations trace this aerosol plume to the meteor that struck near Chelyabinsk, Russia on 15 February 2013. This new dust layer, located above the Junge aerosol layer, has persisted over at least a 3 month period. Material collected on the ground following the bolide explosion showed that the meteor was mostly composed of olivine and pyroxenes. Simulations using Lagrangian and Eulerian atmospheric models trace the plume back to Chelyabinsk and confirm that the plume altitude was at altitudes between 25 and 45 km. The models also confirm the plume circumpolar longitudinal spreading observed by OMPS/LP, with propagation speeds up to 85 m/s.
Key Points
Simulations using atmospheric models confirm that the belt related to bolide
Limb profiler has proven to be a valuable tool to track the meteor plume</description><identifier>ISSN: 0094-8276</identifier><identifier>EISSN: 1944-8007</identifier><identifier>DOI: 10.1002/grl.50788</identifier><language>eng</language><publisher>Washington: Blackwell Publishing Ltd</publisher><subject>aerosol ; Aerosols ; Altitude ; Atmospheric models ; bolide ; Bolides ; Chelyabinsk ; Computer simulation ; Dust ; Meteors ; Meteors & meteorites ; NPP/Suomi ; Plumes ; Profilers ; Stratosphere</subject><ispartof>Geophysical research letters, 2013-09, Vol.40 (17), p.4728-4733</ispartof><rights>2013. American Geophysical Union. All Rights Reserved.</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-a4928-14a1e4dc6f1703f36362a6f0d99dac34604f6203af9a7b9cfc4cf5556e99016b3</citedby><cites>FETCH-LOGICAL-a4928-14a1e4dc6f1703f36362a6f0d99dac34604f6203af9a7b9cfc4cf5556e99016b3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://onlinelibrary.wiley.com/doi/pdf/10.1002%2Fgrl.50788$$EPDF$$P50$$Gwiley$$H</linktopdf><linktohtml>$$Uhttps://onlinelibrary.wiley.com/doi/full/10.1002%2Fgrl.50788$$EHTML$$P50$$Gwiley$$H</linktohtml><link.rule.ids>314,776,780,1411,1427,11494,27903,27904,45553,45554,46388,46447,46812,46871</link.rule.ids></links><search><creatorcontrib>Gorkavyi, Nick</creatorcontrib><creatorcontrib>Rault, D. F.</creatorcontrib><creatorcontrib>Newman, P. A.</creatorcontrib><creatorcontrib>da Silva, A. M.</creatorcontrib><creatorcontrib>Dudorov, A. E.</creatorcontrib><title>New stratospheric dust belt due to the Chelyabinsk bolide</title><title>Geophysical research letters</title><addtitle>Geophys. Res. Lett</addtitle><description>The Ozone Mapping Profiler Suite (OMPS) Limb Profiler (LP) on the recently launched NASA/NOAA NPP/Suomi satellite detected aerosol excess in the mid‐stratosphere (25–45 km altitude) between 50°N and 70°N latitudes. OMPS/LP observations trace this aerosol plume to the meteor that struck near Chelyabinsk, Russia on 15 February 2013. This new dust layer, located above the Junge aerosol layer, has persisted over at least a 3 month period. Material collected on the ground following the bolide explosion showed that the meteor was mostly composed of olivine and pyroxenes. Simulations using Lagrangian and Eulerian atmospheric models trace the plume back to Chelyabinsk and confirm that the plume altitude was at altitudes between 25 and 45 km. The models also confirm the plume circumpolar longitudinal spreading observed by OMPS/LP, with propagation speeds up to 85 m/s.
Key Points
Simulations using atmospheric models confirm that the belt related to bolide
Limb profiler has proven to be a valuable tool to track the meteor plume</description><subject>aerosol</subject><subject>Aerosols</subject><subject>Altitude</subject><subject>Atmospheric models</subject><subject>bolide</subject><subject>Bolides</subject><subject>Chelyabinsk</subject><subject>Computer simulation</subject><subject>Dust</subject><subject>Meteors</subject><subject>Meteors & meteorites</subject><subject>NPP/Suomi</subject><subject>Plumes</subject><subject>Profilers</subject><subject>Stratosphere</subject><issn>0094-8276</issn><issn>1944-8007</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2013</creationdate><recordtype>article</recordtype><recordid>eNp1kD1PwzAQhi0EEqUw8A8iscCQ9hx_JB5RBSlSBaICMVqOY9O0aVNsR6X_nkCAAYnp3uF57k4vQucYRhggGb-6esQgzbIDNMCC0jgDSA_RAEB0OUn5MTrxfgkABAgeIHFvdpEPToXGbxfGVToqWx-iwtShSyYKTRQWJposTL1XRbXxq6ho6qo0p-jIqtqbs-85RM-3N0-TaTx7yO8m17NYUZFkMaYKG1pqbnEKxBJOeKK4hVKIUmlCOVDLEyDKCpUWQltNtWWMcSMEYF6QIbrs925d89YaH-S68trUtdqYpvUSs0QIljCedOjFH3TZtG7TfScxp92RjDLRUVc9pV3jvTNWbl21Vm4vMcjPEmVXovwqsWPHPburarP_H5T5fPZjxL1R-WDefw3lVpKnJGXy5T6X4nGa42xOZU4-AAUigII</recordid><startdate>20130916</startdate><enddate>20130916</enddate><creator>Gorkavyi, Nick</creator><creator>Rault, D. F.</creator><creator>Newman, P. A.</creator><creator>da Silva, A. M.</creator><creator>Dudorov, A. E.</creator><general>Blackwell Publishing Ltd</general><general>John Wiley & Sons, Inc</general><scope>BSCLL</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>7TN</scope><scope>8FD</scope><scope>F1W</scope><scope>FR3</scope><scope>H8D</scope><scope>H96</scope><scope>KL.</scope><scope>KR7</scope><scope>L.G</scope><scope>L7M</scope></search><sort><creationdate>20130916</creationdate><title>New stratospheric dust belt due to the Chelyabinsk bolide</title><author>Gorkavyi, Nick ; Rault, D. F. ; Newman, P. A. ; da Silva, A. M. ; Dudorov, A. E.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a4928-14a1e4dc6f1703f36362a6f0d99dac34604f6203af9a7b9cfc4cf5556e99016b3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2013</creationdate><topic>aerosol</topic><topic>Aerosols</topic><topic>Altitude</topic><topic>Atmospheric models</topic><topic>bolide</topic><topic>Bolides</topic><topic>Chelyabinsk</topic><topic>Computer simulation</topic><topic>Dust</topic><topic>Meteors</topic><topic>Meteors & meteorites</topic><topic>NPP/Suomi</topic><topic>Plumes</topic><topic>Profilers</topic><topic>Stratosphere</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Gorkavyi, Nick</creatorcontrib><creatorcontrib>Rault, D. F.</creatorcontrib><creatorcontrib>Newman, P. A.</creatorcontrib><creatorcontrib>da Silva, A. M.</creatorcontrib><creatorcontrib>Dudorov, A. E.</creatorcontrib><collection>Istex</collection><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Oceanic Abstracts</collection><collection>Technology Research Database</collection><collection>ASFA: Aquatic Sciences and Fisheries Abstracts</collection><collection>Engineering Research Database</collection><collection>Aerospace Database</collection><collection>Aquatic Science & Fisheries Abstracts (ASFA) 2: Ocean Technology, Policy & Non-Living Resources</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Civil Engineering Abstracts</collection><collection>Aquatic Science & Fisheries Abstracts (ASFA) Professional</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Geophysical research letters</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Gorkavyi, Nick</au><au>Rault, D. F.</au><au>Newman, P. A.</au><au>da Silva, A. M.</au><au>Dudorov, A. E.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>New stratospheric dust belt due to the Chelyabinsk bolide</atitle><jtitle>Geophysical research letters</jtitle><addtitle>Geophys. Res. Lett</addtitle><date>2013-09-16</date><risdate>2013</risdate><volume>40</volume><issue>17</issue><spage>4728</spage><epage>4733</epage><pages>4728-4733</pages><issn>0094-8276</issn><eissn>1944-8007</eissn><abstract>The Ozone Mapping Profiler Suite (OMPS) Limb Profiler (LP) on the recently launched NASA/NOAA NPP/Suomi satellite detected aerosol excess in the mid‐stratosphere (25–45 km altitude) between 50°N and 70°N latitudes. OMPS/LP observations trace this aerosol plume to the meteor that struck near Chelyabinsk, Russia on 15 February 2013. This new dust layer, located above the Junge aerosol layer, has persisted over at least a 3 month period. Material collected on the ground following the bolide explosion showed that the meteor was mostly composed of olivine and pyroxenes. Simulations using Lagrangian and Eulerian atmospheric models trace the plume back to Chelyabinsk and confirm that the plume altitude was at altitudes between 25 and 45 km. The models also confirm the plume circumpolar longitudinal spreading observed by OMPS/LP, with propagation speeds up to 85 m/s.
Key Points
Simulations using atmospheric models confirm that the belt related to bolide
Limb profiler has proven to be a valuable tool to track the meteor plume</abstract><cop>Washington</cop><pub>Blackwell Publishing Ltd</pub><doi>10.1002/grl.50788</doi><tpages>6</tpages><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 0094-8276 |
| ispartof | Geophysical research letters, 2013-09, Vol.40 (17), p.4728-4733 |
| issn | 0094-8276 1944-8007 |
| language | eng |
| recordid | cdi_proquest_miscellaneous_1529952562 |
| source | Wiley Online Library Journals Frontfile Complete; Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals; Wiley Free Content; Wiley-Blackwell AGU Digital Library |
| subjects | aerosol Aerosols Altitude Atmospheric models bolide Bolides Chelyabinsk Computer simulation Dust Meteors Meteors & meteorites NPP/Suomi Plumes Profilers Stratosphere |
| title | New stratospheric dust belt due to the Chelyabinsk bolide |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-23T10%3A57%3A19IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=New%20stratospheric%20dust%20belt%20due%20to%20the%20Chelyabinsk%20bolide&rft.jtitle=Geophysical%20research%20letters&rft.au=Gorkavyi,%20Nick&rft.date=2013-09-16&rft.volume=40&rft.issue=17&rft.spage=4728&rft.epage=4733&rft.pages=4728-4733&rft.issn=0094-8276&rft.eissn=1944-8007&rft_id=info:doi/10.1002/grl.50788&rft_dat=%3Cproquest_cross%3E1529952562%3C/proquest_cross%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=1642038459&rft_id=info:pmid/&rfr_iscdi=true |