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Vertical fine structure and time evolution of plasma irregularities in the Es layer observed by a high-resolution Ca+ lidar
The vertical fine structures and the time evolution of plasma irregularities in the sporadic E ( E s ) layer were observed via calcium ion (Ca + ) density measurements using a resonance scattering lidar with a high time-height resolution (5 s and 15 m) at Tachikawa (35.7°N, 139.4°E) on December 24,...
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Published in: | Earth, planets, and space planets, and space, 2019-01, Vol.71 (1), Article 3 |
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creator | Ejiri, Mitsumu K. Nakamura, Takuji Tsuda, Takuo T. Nishiyama, Takanori Abo, Makoto Takahashi, Toru Tsuno, Katsuhiko Kawahara, Takuya D. Ogawa, Takayo Wada, Satoshi |
description | The vertical fine structures and the time evolution of plasma irregularities in the sporadic
E
(
E
s
) layer were observed via calcium ion (Ca
+
) density measurements using a resonance scattering lidar with a high time-height resolution (5 s and 15 m) at Tachikawa (35.7°N, 139.4°E) on December 24, 2014. The observation successfully provided clearer fine structures of plasma irregularities, such as quasi-sinusoidal height variation, localized clumps, “cats-eye” structures, and twist structures, in the sporadic Ca
+
(
Ca
+
s
) layers at around 100 km altitude. These fine structures suggested that the Kelvin–Helmholtz instabilities occurred in the neutral atmosphere whose density changed temporarily or spatially. The maximum Ca
+
density in the
Ca
+
s
layer was two orders of magnitude smaller than the maximum electron density estimated from the critical frequency (
f
o
E
s
) simultaneously observed by the ionosonde at Kokubunji (35.7°N, 139.5°E). A strong positive correlation with a coefficient of 0.91 suggests that Ca
+
contributes forming the
E
s
layer as well as major metallic ions Fe
+
and Mg
+
in the lower thermosphere. Moreover, the formation of a new
Ca
+
s
layer at 110 km and the upward motions of the
Ca
+
s
layers at 100 km and 110 km were observed before the local sunrise and just after the sunrise time at the conjugation point. Although the presence or absence of a causal relationship with the sunrise time was not clear, a possible explanation for the formation and the upward motions of the
Ca
+
s
layers was the occurrence of strong horizontal wind, rather than the enhancement of the eastward electric field. |
doi_str_mv | 10.1186/s40623-019-0984-z |
format | article |
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E
(
E
s
) layer were observed via calcium ion (Ca
+
) density measurements using a resonance scattering lidar with a high time-height resolution (5 s and 15 m) at Tachikawa (35.7°N, 139.4°E) on December 24, 2014. The observation successfully provided clearer fine structures of plasma irregularities, such as quasi-sinusoidal height variation, localized clumps, “cats-eye” structures, and twist structures, in the sporadic Ca
+
(
Ca
+
s
) layers at around 100 km altitude. These fine structures suggested that the Kelvin–Helmholtz instabilities occurred in the neutral atmosphere whose density changed temporarily or spatially. The maximum Ca
+
density in the
Ca
+
s
layer was two orders of magnitude smaller than the maximum electron density estimated from the critical frequency (
f
o
E
s
) simultaneously observed by the ionosonde at Kokubunji (35.7°N, 139.5°E). A strong positive correlation with a coefficient of 0.91 suggests that Ca
+
contributes forming the
E
s
layer as well as major metallic ions Fe
+
and Mg
+
in the lower thermosphere. Moreover, the formation of a new
Ca
+
s
layer at 110 km and the upward motions of the
Ca
+
s
layers at 100 km and 110 km were observed before the local sunrise and just after the sunrise time at the conjugation point. Although the presence or absence of a causal relationship with the sunrise time was not clear, a possible explanation for the formation and the upward motions of the
Ca
+
s
layers was the occurrence of strong horizontal wind, rather than the enhancement of the eastward electric field.</description><identifier>ISSN: 1880-5981</identifier><identifier>EISSN: 1880-5981</identifier><identifier>DOI: 10.1186/s40623-019-0984-z</identifier><language>eng</language><publisher>Berlin/Heidelberg: Springer Berlin Heidelberg</publisher><subject>2. Aeronomy ; Earth and Environmental Science ; Earth Sciences ; Geology ; Geophysics/Geodesy</subject><ispartof>Earth, planets, and space, 2019-01, Vol.71 (1), Article 3</ispartof><rights>The Author(s) 2019</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c382t-5d25df8af880f1a4add5e9d9398e97a3659098237fd7178a19d37cdddc25f5393</citedby><cites>FETCH-LOGICAL-c382t-5d25df8af880f1a4add5e9d9398e97a3659098237fd7178a19d37cdddc25f5393</cites><orcidid>0000-0002-1742-3558</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,776,780,27903,27904</link.rule.ids></links><search><creatorcontrib>Ejiri, Mitsumu K.</creatorcontrib><creatorcontrib>Nakamura, Takuji</creatorcontrib><creatorcontrib>Tsuda, Takuo T.</creatorcontrib><creatorcontrib>Nishiyama, Takanori</creatorcontrib><creatorcontrib>Abo, Makoto</creatorcontrib><creatorcontrib>Takahashi, Toru</creatorcontrib><creatorcontrib>Tsuno, Katsuhiko</creatorcontrib><creatorcontrib>Kawahara, Takuya D.</creatorcontrib><creatorcontrib>Ogawa, Takayo</creatorcontrib><creatorcontrib>Wada, Satoshi</creatorcontrib><title>Vertical fine structure and time evolution of plasma irregularities in the Es layer observed by a high-resolution Ca+ lidar</title><title>Earth, planets, and space</title><addtitle>Earth Planets Space</addtitle><description>The vertical fine structures and the time evolution of plasma irregularities in the sporadic
E
(
E
s
) layer were observed via calcium ion (Ca
+
) density measurements using a resonance scattering lidar with a high time-height resolution (5 s and 15 m) at Tachikawa (35.7°N, 139.4°E) on December 24, 2014. The observation successfully provided clearer fine structures of plasma irregularities, such as quasi-sinusoidal height variation, localized clumps, “cats-eye” structures, and twist structures, in the sporadic Ca
+
(
Ca
+
s
) layers at around 100 km altitude. These fine structures suggested that the Kelvin–Helmholtz instabilities occurred in the neutral atmosphere whose density changed temporarily or spatially. The maximum Ca
+
density in the
Ca
+
s
layer was two orders of magnitude smaller than the maximum electron density estimated from the critical frequency (
f
o
E
s
) simultaneously observed by the ionosonde at Kokubunji (35.7°N, 139.5°E). A strong positive correlation with a coefficient of 0.91 suggests that Ca
+
contributes forming the
E
s
layer as well as major metallic ions Fe
+
and Mg
+
in the lower thermosphere. Moreover, the formation of a new
Ca
+
s
layer at 110 km and the upward motions of the
Ca
+
s
layers at 100 km and 110 km were observed before the local sunrise and just after the sunrise time at the conjugation point. Although the presence or absence of a causal relationship with the sunrise time was not clear, a possible explanation for the formation and the upward motions of the
Ca
+
s
layers was the occurrence of strong horizontal wind, rather than the enhancement of the eastward electric field.</description><subject>2. Aeronomy</subject><subject>Earth and Environmental Science</subject><subject>Earth Sciences</subject><subject>Geology</subject><subject>Geophysics/Geodesy</subject><issn>1880-5981</issn><issn>1880-5981</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2019</creationdate><recordtype>article</recordtype><recordid>eNp9kE1LAzEQhoMoWKs_wNvcJZpsdrvJUUr9gIIX9RrSzaRN2e6WyW6h9c-7pQqePM0c5nmZ92HsVop7KfXkIeVikikupOHC6JwfzthIai14YbQ8_7NfsquU1kIokU_UiH19InWxcjWE2CCkjvqq6wnBNR66uEHAXVv3XWwbaANsa5c2DiIRLvvaUewiJogNdCuEWYLa7ZGgXSSkHXpY7MHBKi5XnDD9xkzdHdTRO7pmF8HVCW9-5ph9PM3epy98_vb8On2c80rprOOFzwoftAtDhSBd7rwv0HijjEZTOjUpzFA5U2XwpSy1k8arsvLeV1kRCmXUmMlTbkVtSoTBbiluHO2tFPZoz57s2cGePdqzh4HJTkwabpslkl23PTXDm_9A3wzddZ8</recordid><startdate>20190111</startdate><enddate>20190111</enddate><creator>Ejiri, Mitsumu K.</creator><creator>Nakamura, Takuji</creator><creator>Tsuda, Takuo T.</creator><creator>Nishiyama, Takanori</creator><creator>Abo, Makoto</creator><creator>Takahashi, Toru</creator><creator>Tsuno, Katsuhiko</creator><creator>Kawahara, Takuya D.</creator><creator>Ogawa, Takayo</creator><creator>Wada, Satoshi</creator><general>Springer Berlin Heidelberg</general><scope>C6C</scope><scope>AAYXX</scope><scope>CITATION</scope><orcidid>https://orcid.org/0000-0002-1742-3558</orcidid></search><sort><creationdate>20190111</creationdate><title>Vertical fine structure and time evolution of plasma irregularities in the Es layer observed by a high-resolution Ca+ lidar</title><author>Ejiri, Mitsumu K. ; Nakamura, Takuji ; Tsuda, Takuo T. ; Nishiyama, Takanori ; Abo, Makoto ; Takahashi, Toru ; Tsuno, Katsuhiko ; Kawahara, Takuya D. ; Ogawa, Takayo ; Wada, Satoshi</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c382t-5d25df8af880f1a4add5e9d9398e97a3659098237fd7178a19d37cdddc25f5393</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2019</creationdate><topic>2. Aeronomy</topic><topic>Earth and Environmental Science</topic><topic>Earth Sciences</topic><topic>Geology</topic><topic>Geophysics/Geodesy</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Ejiri, Mitsumu K.</creatorcontrib><creatorcontrib>Nakamura, Takuji</creatorcontrib><creatorcontrib>Tsuda, Takuo T.</creatorcontrib><creatorcontrib>Nishiyama, Takanori</creatorcontrib><creatorcontrib>Abo, Makoto</creatorcontrib><creatorcontrib>Takahashi, Toru</creatorcontrib><creatorcontrib>Tsuno, Katsuhiko</creatorcontrib><creatorcontrib>Kawahara, Takuya D.</creatorcontrib><creatorcontrib>Ogawa, Takayo</creatorcontrib><creatorcontrib>Wada, Satoshi</creatorcontrib><collection>SpringerOpen (Open Access)</collection><collection>CrossRef</collection><jtitle>Earth, planets, and space</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Ejiri, Mitsumu K.</au><au>Nakamura, Takuji</au><au>Tsuda, Takuo T.</au><au>Nishiyama, Takanori</au><au>Abo, Makoto</au><au>Takahashi, Toru</au><au>Tsuno, Katsuhiko</au><au>Kawahara, Takuya D.</au><au>Ogawa, Takayo</au><au>Wada, Satoshi</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Vertical fine structure and time evolution of plasma irregularities in the Es layer observed by a high-resolution Ca+ lidar</atitle><jtitle>Earth, planets, and space</jtitle><stitle>Earth Planets Space</stitle><date>2019-01-11</date><risdate>2019</risdate><volume>71</volume><issue>1</issue><artnum>3</artnum><issn>1880-5981</issn><eissn>1880-5981</eissn><abstract>The vertical fine structures and the time evolution of plasma irregularities in the sporadic
E
(
E
s
) layer were observed via calcium ion (Ca
+
) density measurements using a resonance scattering lidar with a high time-height resolution (5 s and 15 m) at Tachikawa (35.7°N, 139.4°E) on December 24, 2014. The observation successfully provided clearer fine structures of plasma irregularities, such as quasi-sinusoidal height variation, localized clumps, “cats-eye” structures, and twist structures, in the sporadic Ca
+
(
Ca
+
s
) layers at around 100 km altitude. These fine structures suggested that the Kelvin–Helmholtz instabilities occurred in the neutral atmosphere whose density changed temporarily or spatially. The maximum Ca
+
density in the
Ca
+
s
layer was two orders of magnitude smaller than the maximum electron density estimated from the critical frequency (
f
o
E
s
) simultaneously observed by the ionosonde at Kokubunji (35.7°N, 139.5°E). A strong positive correlation with a coefficient of 0.91 suggests that Ca
+
contributes forming the
E
s
layer as well as major metallic ions Fe
+
and Mg
+
in the lower thermosphere. Moreover, the formation of a new
Ca
+
s
layer at 110 km and the upward motions of the
Ca
+
s
layers at 100 km and 110 km were observed before the local sunrise and just after the sunrise time at the conjugation point. Although the presence or absence of a causal relationship with the sunrise time was not clear, a possible explanation for the formation and the upward motions of the
Ca
+
s
layers was the occurrence of strong horizontal wind, rather than the enhancement of the eastward electric field.</abstract><cop>Berlin/Heidelberg</cop><pub>Springer Berlin Heidelberg</pub><doi>10.1186/s40623-019-0984-z</doi><orcidid>https://orcid.org/0000-0002-1742-3558</orcidid><oa>free_for_read</oa></addata></record> |
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source | Publicly Available Content Database; Springer Nature - SpringerLink Journals - Fully Open Access |
subjects | 2. Aeronomy Earth and Environmental Science Earth Sciences Geology Geophysics/Geodesy |
title | Vertical fine structure and time evolution of plasma irregularities in the Es layer observed by a high-resolution Ca+ lidar |
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