Seasonal and Long-Term Changes in the Intensity of O2(b1Σ) and OH(X2Π) Airglow in the Mesopause Region
Spectral observations of the mesopause airglow at the Zvenigorod Scientific Station have been used to obtain the midnight emission intensities of molecular oxygen (О 2 А(0-1) band) and hydroxyl (OH (6-2) band) for 2000–2019. Spectral analysis of the variations has made it possible to determine the a...
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| Veröffentlicht in: | Geomagnetism and Aeronomy 2021-07, Vol.61 (4), p.589-599 |
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| container_title | Geomagnetism and Aeronomy |
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| creator | Perminov, V. I. Pertsev, N. N. Dalin, P. A. Zheleznov, Yu. A. Sukhodoev, V. A. Orekhov, M. D. |
| description | Spectral observations of the mesopause airglow at the Zvenigorod Scientific Station have been used to obtain the midnight emission intensities of molecular oxygen (О
2
А(0-1) band) and hydroxyl (OH (6-2) band) for 2000–2019. Spectral analysis of the variations has made it possible to determine the annual variability for each emission, which is described by the sum of four harmonics. The time lag in seasonal variations of the hydroxyl emission relative to variations in the emission of molecular oxygen is 5–18 days. Long-term changes in the average annual emission intensities have been studied. The linear trend (–3.3 ± 0.3% per year for О
2
А(0-1) and –2.6 ± 0.2% per year for ОН(6-2)), the dependences on the 11-year solar cycle (response to changes in the Lyman-alpha solar radiation (18.5 ± 3.3% per 10
11
photons cm
–2
s
–1
for О
2
А(0-1) and 10.5 ± 2.5% per 10
11
photons cm
–2
s
–1
for OH (6-2)) and the 22-year solar cycle (response to changes in the solar magnetic field strength (23.2 ± 4.5% per 100 μТ for О
2
А(0-1) and 12.1 ± 3.5% per 100 μТ for ОН (6-2)), as well as quasi-eight-year oscillations have been found. |
| doi_str_mv | 10.1134/S0016793221040113 |
| format | Article |
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2
А(0-1) band) and hydroxyl (OH (6-2) band) for 2000–2019. Spectral analysis of the variations has made it possible to determine the annual variability for each emission, which is described by the sum of four harmonics. The time lag in seasonal variations of the hydroxyl emission relative to variations in the emission of molecular oxygen is 5–18 days. Long-term changes in the average annual emission intensities have been studied. The linear trend (–3.3 ± 0.3% per year for О
2
А(0-1) and –2.6 ± 0.2% per year for ОН(6-2)), the dependences on the 11-year solar cycle (response to changes in the Lyman-alpha solar radiation (18.5 ± 3.3% per 10
11
photons cm
–2
s
–1
for О
2
А(0-1) and 10.5 ± 2.5% per 10
11
photons cm
–2
s
–1
for OH (6-2)) and the 22-year solar cycle (response to changes in the solar magnetic field strength (23.2 ± 4.5% per 100 μТ for О
2
А(0-1) and 12.1 ± 3.5% per 100 μТ for ОН (6-2)), as well as quasi-eight-year oscillations have been found.</description><identifier>ISSN: 0016-7932</identifier><identifier>EISSN: 1555-645X</identifier><identifier>EISSN: 0016-7940</identifier><identifier>DOI: 10.1134/S0016793221040113</identifier><language>eng</language><publisher>Moscow: Pleiades Publishing</publisher><subject>Airglow ; Alpha rays ; Annual variations ; Earth and Environmental Science ; Earth Sciences ; Emission analysis ; Emissions ; Field strength ; Geophysics/Geodesy ; Hydroxyl emission ; Magnetic fields ; Mesopause ; Oxygen ; Photons ; Seasonal variations ; Solar cycle ; Solar magnetic field ; Solar radiation ; Spectral analysis ; Spectrum analysis ; Time lag</subject><ispartof>Geomagnetism and Aeronomy, 2021-07, Vol.61 (4), p.589-599</ispartof><rights>Pleiades Publishing, Ltd. 2021. ISSN 0016-7932, Geomagnetism and Aeronomy, 2021, Vol. 61, No. 4, pp. 589–599. © Pleiades Publishing, Ltd., 2021. Russian Text © The Author(s), 2021, published in Geomagnetizm i Aeronomiya, 2021, Vol. 61, No. 4, pp. 532–543.</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c2313-df207160a6a55fe4971edf6b528c2932aac9f88339ac145c221a76cdc58ad0763</citedby><cites>FETCH-LOGICAL-c2313-df207160a6a55fe4971edf6b528c2932aac9f88339ac145c221a76cdc58ad0763</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.1134/S0016793221040113$$EPDF$$P50$$Gspringer$$H</linktopdf><linktohtml>$$Uhttps://link.springer.com/10.1134/S0016793221040113$$EHTML$$P50$$Gspringer$$H</linktohtml><link.rule.ids>314,780,784,27924,27925,41488,42557,51319</link.rule.ids></links><search><creatorcontrib>Perminov, V. I.</creatorcontrib><creatorcontrib>Pertsev, N. N.</creatorcontrib><creatorcontrib>Dalin, P. A.</creatorcontrib><creatorcontrib>Zheleznov, Yu. A.</creatorcontrib><creatorcontrib>Sukhodoev, V. A.</creatorcontrib><creatorcontrib>Orekhov, M. D.</creatorcontrib><title>Seasonal and Long-Term Changes in the Intensity of O2(b1Σ) and OH(X2Π) Airglow in the Mesopause Region</title><title>Geomagnetism and Aeronomy</title><addtitle>Geomagn. Aeron</addtitle><description>Spectral observations of the mesopause airglow at the Zvenigorod Scientific Station have been used to obtain the midnight emission intensities of molecular oxygen (О
2
А(0-1) band) and hydroxyl (OH (6-2) band) for 2000–2019. Spectral analysis of the variations has made it possible to determine the annual variability for each emission, which is described by the sum of four harmonics. The time lag in seasonal variations of the hydroxyl emission relative to variations in the emission of molecular oxygen is 5–18 days. Long-term changes in the average annual emission intensities have been studied. The linear trend (–3.3 ± 0.3% per year for О
2
А(0-1) and –2.6 ± 0.2% per year for ОН(6-2)), the dependences on the 11-year solar cycle (response to changes in the Lyman-alpha solar radiation (18.5 ± 3.3% per 10
11
photons cm
–2
s
–1
for О
2
А(0-1) and 10.5 ± 2.5% per 10
11
photons cm
–2
s
–1
for OH (6-2)) and the 22-year solar cycle (response to changes in the solar magnetic field strength (23.2 ± 4.5% per 100 μТ for О
2
А(0-1) and 12.1 ± 3.5% per 100 μТ for ОН (6-2)), as well as quasi-eight-year oscillations have been found.</description><subject>Airglow</subject><subject>Alpha rays</subject><subject>Annual variations</subject><subject>Earth and Environmental Science</subject><subject>Earth Sciences</subject><subject>Emission analysis</subject><subject>Emissions</subject><subject>Field strength</subject><subject>Geophysics/Geodesy</subject><subject>Hydroxyl emission</subject><subject>Magnetic fields</subject><subject>Mesopause</subject><subject>Oxygen</subject><subject>Photons</subject><subject>Seasonal variations</subject><subject>Solar cycle</subject><subject>Solar magnetic field</subject><subject>Solar radiation</subject><subject>Spectral analysis</subject><subject>Spectrum analysis</subject><subject>Time lag</subject><issn>0016-7932</issn><issn>1555-645X</issn><issn>0016-7940</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2021</creationdate><recordtype>article</recordtype><recordid>eNp1kM1KAzEUhYMoWKsP4C7gpl2M5n9mlqWoLVQKtkJ3Q5pJplPapCZTpG8j-D59JlOruBBXF-493-GeA8A1RrcYU3Y3QQiLNKeEYMRQXJ2AFuacJ4Lx2SloHc7J4X4OLkJYIkQR57gFFhMtg7NyBaUt4cjZKplqv4b9hbSVDrC2sFloOLSNtqFudtAZOCadOd5_dL-Q8aAzI_v3LuzVvlq5tx_iSQe3kdug4bOuamcvwZmRq6CvvmcbvDzcT_uDZDR-HPZ7o0QRimlSGoJSLJAUknOjWZ5iXRox5yRTJL4vpcpNllGaS4UZVzGvTIUqFc9kiVJB2-Dm6Lvx7nWrQ1Ms3dbHgKEgXGQkZTllUYWPKuVdCF6bYuPrtfS7AqPiUGjxp9DIkCMTojaW43-d_4c-AUu1dc0</recordid><startdate>20210701</startdate><enddate>20210701</enddate><creator>Perminov, V. I.</creator><creator>Pertsev, N. N.</creator><creator>Dalin, P. A.</creator><creator>Zheleznov, Yu. A.</creator><creator>Sukhodoev, V. A.</creator><creator>Orekhov, M. D.</creator><general>Pleiades Publishing</general><general>Springer Nature B.V</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>8FD</scope><scope>H8D</scope><scope>KL.</scope><scope>L7M</scope></search><sort><creationdate>20210701</creationdate><title>Seasonal and Long-Term Changes in the Intensity of O2(b1Σ) and OH(X2Π) Airglow in the Mesopause Region</title><author>Perminov, V. I. ; Pertsev, N. N. ; Dalin, P. A. ; Zheleznov, Yu. A. ; Sukhodoev, V. A. ; Orekhov, M. D.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c2313-df207160a6a55fe4971edf6b528c2932aac9f88339ac145c221a76cdc58ad0763</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2021</creationdate><topic>Airglow</topic><topic>Alpha rays</topic><topic>Annual variations</topic><topic>Earth and Environmental Science</topic><topic>Earth Sciences</topic><topic>Emission analysis</topic><topic>Emissions</topic><topic>Field strength</topic><topic>Geophysics/Geodesy</topic><topic>Hydroxyl emission</topic><topic>Magnetic fields</topic><topic>Mesopause</topic><topic>Oxygen</topic><topic>Photons</topic><topic>Seasonal variations</topic><topic>Solar cycle</topic><topic>Solar magnetic field</topic><topic>Solar radiation</topic><topic>Spectral analysis</topic><topic>Spectrum analysis</topic><topic>Time lag</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Perminov, V. I.</creatorcontrib><creatorcontrib>Pertsev, N. N.</creatorcontrib><creatorcontrib>Dalin, P. A.</creatorcontrib><creatorcontrib>Zheleznov, Yu. A.</creatorcontrib><creatorcontrib>Sukhodoev, V. A.</creatorcontrib><creatorcontrib>Orekhov, M. D.</creatorcontrib><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Geomagnetism and Aeronomy</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Perminov, V. I.</au><au>Pertsev, N. N.</au><au>Dalin, P. A.</au><au>Zheleznov, Yu. A.</au><au>Sukhodoev, V. A.</au><au>Orekhov, M. D.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Seasonal and Long-Term Changes in the Intensity of O2(b1Σ) and OH(X2Π) Airglow in the Mesopause Region</atitle><jtitle>Geomagnetism and Aeronomy</jtitle><stitle>Geomagn. Aeron</stitle><date>2021-07-01</date><risdate>2021</risdate><volume>61</volume><issue>4</issue><spage>589</spage><epage>599</epage><pages>589-599</pages><issn>0016-7932</issn><eissn>1555-645X</eissn><eissn>0016-7940</eissn><abstract>Spectral observations of the mesopause airglow at the Zvenigorod Scientific Station have been used to obtain the midnight emission intensities of molecular oxygen (О
2
А(0-1) band) and hydroxyl (OH (6-2) band) for 2000–2019. Spectral analysis of the variations has made it possible to determine the annual variability for each emission, which is described by the sum of four harmonics. The time lag in seasonal variations of the hydroxyl emission relative to variations in the emission of molecular oxygen is 5–18 days. Long-term changes in the average annual emission intensities have been studied. The linear trend (–3.3 ± 0.3% per year for О
2
А(0-1) and –2.6 ± 0.2% per year for ОН(6-2)), the dependences on the 11-year solar cycle (response to changes in the Lyman-alpha solar radiation (18.5 ± 3.3% per 10
11
photons cm
–2
s
–1
for О
2
А(0-1) and 10.5 ± 2.5% per 10
11
photons cm
–2
s
–1
for OH (6-2)) and the 22-year solar cycle (response to changes in the solar magnetic field strength (23.2 ± 4.5% per 100 μТ for О
2
А(0-1) and 12.1 ± 3.5% per 100 μТ for ОН (6-2)), as well as quasi-eight-year oscillations have been found.</abstract><cop>Moscow</cop><pub>Pleiades Publishing</pub><doi>10.1134/S0016793221040113</doi><tpages>11</tpages></addata></record> |
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| identifier | ISSN: 0016-7932 |
| ispartof | Geomagnetism and Aeronomy, 2021-07, Vol.61 (4), p.589-599 |
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| language | eng |
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| source | SpringerNature Journals |
| subjects | Airglow Alpha rays Annual variations Earth and Environmental Science Earth Sciences Emission analysis Emissions Field strength Geophysics/Geodesy Hydroxyl emission Magnetic fields Mesopause Oxygen Photons Seasonal variations Solar cycle Solar magnetic field Solar radiation Spectral analysis Spectrum analysis Time lag |
| title | Seasonal and Long-Term Changes in the Intensity of O2(b1Σ) and OH(X2Π) Airglow in the Mesopause Region |
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