Travelling wave packets generated by the solar terminator in the upper atmosphere

Abstract For the first time, the morphology of a new type of midlatitude, medium scale, travelling ionospheric disturbances—travelling wave packets (TWPs)—is presented with the use of total electron content (TEC) measurements from the data of a global net of GPS receivers over a long time period fro...
Ausführliche Beschreibung

Gespeichert in:

Autor*in:	Afraimovich, E. L. [verfasserIn] Edemskiy, I. K. Voeykov, S. V. Yasyukevich, Yu. V. Zhivetiev, I. V.

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2010

Schlagwörter:	Wave Packet Total Electron Content Vertical Total Electron Content Total Electron Content Variation Total Electron Content Measurement

Anmerkung:	© Pleiades Publishing, Ltd. 2010

Übergeordnetes Werk:	Enthalten in: Atmospheric and oceanic optics - Dordrecht [u.a.] : Springer Science + Business Media B.V, 2009, 23(2010), 1 vom: Feb., Seite 21-27
Übergeordnetes Werk:	volume:23 ; year:2010 ; number:1 ; month:02 ; pages:21-27

Links:	Volltext

DOI / URN:	10.1134/S1024856010010057

Katalog-ID:	SPR026316609

Internformat


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100	1		\|a Afraimovich, E. L. \|e verfasserin \|4 aut
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520			\|a Abstract For the first time, the morphology of a new type of midlatitude, medium scale, travelling ionospheric disturbances—travelling wave packets (TWPs)—is presented with the use of total electron content (TEC) measurements from the data of a global net of GPS receivers over a long time period from 1998 to 2007. The total amount of registered TWPs exceeds 275 000. In the context of time, TWPs are narrow-band TEC oscillations of an hour length with a period of about 10–20 min. TWPs are predominantly observed within 3 h after passing the morning solar terminator, when the TEC derivatives reach their maximum.
650		4	\|a Wave Packet \|7 (dpeaa)DE-He213
650		4	\|a Total Electron Content \|7 (dpeaa)DE-He213
650		4	\|a Vertical Total Electron Content \|7 (dpeaa)DE-He213
650		4	\|a Total Electron Content Variation \|7 (dpeaa)DE-He213
650		4	\|a Total Electron Content Measurement \|7 (dpeaa)DE-He213
700	1		\|a Edemskiy, I. K. \|4 aut
700	1		\|a Voeykov, S. V. \|4 aut
700	1		\|a Yasyukevich, Yu. V. \|4 aut
700	1		\|a Zhivetiev, I. V. \|4 aut
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856	4	0	\|u https://dx.doi.org/10.1134/S1024856010010057 \|z lizenzpflichtig \|3 Volltext
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912			\|a GBV_ILN_70
912			\|a GBV_ILN_73
912			\|a GBV_ILN_74
912			\|a GBV_ILN_90
912			\|a GBV_ILN_95
912			\|a GBV_ILN_100
912			\|a GBV_ILN_101
912			\|a GBV_ILN_105
912			\|a GBV_ILN_110
912			\|a GBV_ILN_120
912			\|a GBV_ILN_138
912			\|a GBV_ILN_150
912			\|a GBV_ILN_151
912			\|a GBV_ILN_152
912			\|a GBV_ILN_161
912			\|a GBV_ILN_170
912			\|a GBV_ILN_171
912			\|a GBV_ILN_187
912			\|a GBV_ILN_213
912			\|a GBV_ILN_224
912			\|a GBV_ILN_230
912			\|a GBV_ILN_250
912			\|a GBV_ILN_281
912			\|a GBV_ILN_285
912			\|a GBV_ILN_293
912			\|a GBV_ILN_370
912			\|a GBV_ILN_602
912			\|a GBV_ILN_636
912			\|a GBV_ILN_702
912			\|a GBV_ILN_2001
912			\|a GBV_ILN_2003
912			\|a GBV_ILN_2004
912			\|a GBV_ILN_2005
912			\|a GBV_ILN_2006
912			\|a GBV_ILN_2007
912			\|a GBV_ILN_2008
912			\|a GBV_ILN_2009
912			\|a GBV_ILN_2010
912			\|a GBV_ILN_2011
912			\|a GBV_ILN_2014
912			\|a GBV_ILN_2015
912			\|a GBV_ILN_2020
912			\|a GBV_ILN_2021
912			\|a GBV_ILN_2025
912			\|a GBV_ILN_2026
912			\|a GBV_ILN_2027
912			\|a GBV_ILN_2031
912			\|a GBV_ILN_2034
912			\|a GBV_ILN_2037
912			\|a GBV_ILN_2038
912			\|a GBV_ILN_2039
912			\|a GBV_ILN_2044
912			\|a GBV_ILN_2048
912			\|a GBV_ILN_2049
912			\|a GBV_ILN_2050
912			\|a GBV_ILN_2055
912			\|a GBV_ILN_2057
912			\|a GBV_ILN_2059
912			\|a GBV_ILN_2061
912			\|a GBV_ILN_2064
912			\|a GBV_ILN_2065
912			\|a GBV_ILN_2068
912			\|a GBV_ILN_2070
912			\|a GBV_ILN_2086
912			\|a GBV_ILN_2088
912			\|a GBV_ILN_2093
912			\|a GBV_ILN_2106
912			\|a GBV_ILN_2107
912			\|a GBV_ILN_2108
912			\|a GBV_ILN_2110
912			\|a GBV_ILN_2111
912			\|a GBV_ILN_2112
912			\|a GBV_ILN_2113
912			\|a GBV_ILN_2116
912			\|a GBV_ILN_2118
912			\|a GBV_ILN_2119
912			\|a GBV_ILN_2122
912			\|a GBV_ILN_2129
912			\|a GBV_ILN_2143
912			\|a GBV_ILN_2144
912			\|a GBV_ILN_2147
912			\|a GBV_ILN_2148
912			\|a GBV_ILN_2152
912			\|a GBV_ILN_2153
912			\|a GBV_ILN_2188
912			\|a GBV_ILN_2190
912			\|a GBV_ILN_2232
912			\|a GBV_ILN_2336
912			\|a GBV_ILN_2446
912			\|a GBV_ILN_2470
912			\|a GBV_ILN_2472
912			\|a GBV_ILN_2507
912			\|a GBV_ILN_2522
912			\|a GBV_ILN_2548
912			\|a GBV_ILN_4035
912			\|a GBV_ILN_4037
912			\|a GBV_ILN_4046
912			\|a GBV_ILN_4112
912			\|a GBV_ILN_4125
912			\|a GBV_ILN_4242
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912			\|a GBV_ILN_4322
912			\|a GBV_ILN_4323
912			\|a GBV_ILN_4324
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912			\|a GBV_ILN_4326
912			\|a GBV_ILN_4333
912			\|a GBV_ILN_4334
912			\|a GBV_ILN_4335
912			\|a GBV_ILN_4336
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952			\|d 23 \|j 2010 \|e 1 \|c 02 \|h 21-27

Indexfelder

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allfields	10.1134/S1024856010010057 doi (DE-627)SPR026316609 (SPR)S1024856010010057-e DE-627 ger DE-627 rakwb eng Afraimovich, E. L. verfasserin aut Travelling wave packets generated by the solar terminator in the upper atmosphere 2010 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Pleiades Publishing, Ltd. 2010 Abstract For the first time, the morphology of a new type of midlatitude, medium scale, travelling ionospheric disturbances—travelling wave packets (TWPs)—is presented with the use of total electron content (TEC) measurements from the data of a global net of GPS receivers over a long time period from 1998 to 2007. The total amount of registered TWPs exceeds 275 000. In the context of time, TWPs are narrow-band TEC oscillations of an hour length with a period of about 10–20 min. TWPs are predominantly observed within 3 h after passing the morning solar terminator, when the TEC derivatives reach their maximum. Wave Packet (dpeaa)DE-He213 Total Electron Content (dpeaa)DE-He213 Vertical Total Electron Content (dpeaa)DE-He213 Total Electron Content Variation (dpeaa)DE-He213 Total Electron Content Measurement (dpeaa)DE-He213 Edemskiy, I. K. aut Voeykov, S. V. aut Yasyukevich, Yu. V. aut Zhivetiev, I. V. aut Enthalten in Atmospheric and oceanic optics Dordrecht [u.a.] : Springer Science + Business Media B.V, 2009 23(2010), 1 vom: Feb., Seite 21-27 (DE-627)599674695 (DE-600)2493873-7 2070-0393 nnns volume:23 year:2010 number:1 month:02 pages:21-27 https://dx.doi.org/10.1134/S1024856010010057 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 23 2010 1 02 21-27
spelling	10.1134/S1024856010010057 doi (DE-627)SPR026316609 (SPR)S1024856010010057-e DE-627 ger DE-627 rakwb eng Afraimovich, E. L. verfasserin aut Travelling wave packets generated by the solar terminator in the upper atmosphere 2010 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Pleiades Publishing, Ltd. 2010 Abstract For the first time, the morphology of a new type of midlatitude, medium scale, travelling ionospheric disturbances—travelling wave packets (TWPs)—is presented with the use of total electron content (TEC) measurements from the data of a global net of GPS receivers over a long time period from 1998 to 2007. The total amount of registered TWPs exceeds 275 000. In the context of time, TWPs are narrow-band TEC oscillations of an hour length with a period of about 10–20 min. TWPs are predominantly observed within 3 h after passing the morning solar terminator, when the TEC derivatives reach their maximum. Wave Packet (dpeaa)DE-He213 Total Electron Content (dpeaa)DE-He213 Vertical Total Electron Content (dpeaa)DE-He213 Total Electron Content Variation (dpeaa)DE-He213 Total Electron Content Measurement (dpeaa)DE-He213 Edemskiy, I. K. aut Voeykov, S. V. aut Yasyukevich, Yu. V. aut Zhivetiev, I. V. aut Enthalten in Atmospheric and oceanic optics Dordrecht [u.a.] : Springer Science + Business Media B.V, 2009 23(2010), 1 vom: Feb., Seite 21-27 (DE-627)599674695 (DE-600)2493873-7 2070-0393 nnns volume:23 year:2010 number:1 month:02 pages:21-27 https://dx.doi.org/10.1134/S1024856010010057 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 23 2010 1 02 21-27
allfields_unstemmed	10.1134/S1024856010010057 doi (DE-627)SPR026316609 (SPR)S1024856010010057-e DE-627 ger DE-627 rakwb eng Afraimovich, E. L. verfasserin aut Travelling wave packets generated by the solar terminator in the upper atmosphere 2010 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Pleiades Publishing, Ltd. 2010 Abstract For the first time, the morphology of a new type of midlatitude, medium scale, travelling ionospheric disturbances—travelling wave packets (TWPs)—is presented with the use of total electron content (TEC) measurements from the data of a global net of GPS receivers over a long time period from 1998 to 2007. The total amount of registered TWPs exceeds 275 000. In the context of time, TWPs are narrow-band TEC oscillations of an hour length with a period of about 10–20 min. TWPs are predominantly observed within 3 h after passing the morning solar terminator, when the TEC derivatives reach their maximum. Wave Packet (dpeaa)DE-He213 Total Electron Content (dpeaa)DE-He213 Vertical Total Electron Content (dpeaa)DE-He213 Total Electron Content Variation (dpeaa)DE-He213 Total Electron Content Measurement (dpeaa)DE-He213 Edemskiy, I. K. aut Voeykov, S. V. aut Yasyukevich, Yu. V. aut Zhivetiev, I. V. aut Enthalten in Atmospheric and oceanic optics Dordrecht [u.a.] : Springer Science + Business Media B.V, 2009 23(2010), 1 vom: Feb., Seite 21-27 (DE-627)599674695 (DE-600)2493873-7 2070-0393 nnns volume:23 year:2010 number:1 month:02 pages:21-27 https://dx.doi.org/10.1134/S1024856010010057 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 23 2010 1 02 21-27
allfieldsGer	10.1134/S1024856010010057 doi (DE-627)SPR026316609 (SPR)S1024856010010057-e DE-627 ger DE-627 rakwb eng Afraimovich, E. L. verfasserin aut Travelling wave packets generated by the solar terminator in the upper atmosphere 2010 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Pleiades Publishing, Ltd. 2010 Abstract For the first time, the morphology of a new type of midlatitude, medium scale, travelling ionospheric disturbances—travelling wave packets (TWPs)—is presented with the use of total electron content (TEC) measurements from the data of a global net of GPS receivers over a long time period from 1998 to 2007. The total amount of registered TWPs exceeds 275 000. In the context of time, TWPs are narrow-band TEC oscillations of an hour length with a period of about 10–20 min. TWPs are predominantly observed within 3 h after passing the morning solar terminator, when the TEC derivatives reach their maximum. Wave Packet (dpeaa)DE-He213 Total Electron Content (dpeaa)DE-He213 Vertical Total Electron Content (dpeaa)DE-He213 Total Electron Content Variation (dpeaa)DE-He213 Total Electron Content Measurement (dpeaa)DE-He213 Edemskiy, I. K. aut Voeykov, S. V. aut Yasyukevich, Yu. V. aut Zhivetiev, I. V. aut Enthalten in Atmospheric and oceanic optics Dordrecht [u.a.] : Springer Science + Business Media B.V, 2009 23(2010), 1 vom: Feb., Seite 21-27 (DE-627)599674695 (DE-600)2493873-7 2070-0393 nnns volume:23 year:2010 number:1 month:02 pages:21-27 https://dx.doi.org/10.1134/S1024856010010057 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 23 2010 1 02 21-27
allfieldsSound	10.1134/S1024856010010057 doi (DE-627)SPR026316609 (SPR)S1024856010010057-e DE-627 ger DE-627 rakwb eng Afraimovich, E. L. verfasserin aut Travelling wave packets generated by the solar terminator in the upper atmosphere 2010 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Pleiades Publishing, Ltd. 2010 Abstract For the first time, the morphology of a new type of midlatitude, medium scale, travelling ionospheric disturbances—travelling wave packets (TWPs)—is presented with the use of total electron content (TEC) measurements from the data of a global net of GPS receivers over a long time period from 1998 to 2007. The total amount of registered TWPs exceeds 275 000. In the context of time, TWPs are narrow-band TEC oscillations of an hour length with a period of about 10–20 min. TWPs are predominantly observed within 3 h after passing the morning solar terminator, when the TEC derivatives reach their maximum. Wave Packet (dpeaa)DE-He213 Total Electron Content (dpeaa)DE-He213 Vertical Total Electron Content (dpeaa)DE-He213 Total Electron Content Variation (dpeaa)DE-He213 Total Electron Content Measurement (dpeaa)DE-He213 Edemskiy, I. K. aut Voeykov, S. V. aut Yasyukevich, Yu. V. aut Zhivetiev, I. V. aut Enthalten in Atmospheric and oceanic optics Dordrecht [u.a.] : Springer Science + Business Media B.V, 2009 23(2010), 1 vom: Feb., Seite 21-27 (DE-627)599674695 (DE-600)2493873-7 2070-0393 nnns volume:23 year:2010 number:1 month:02 pages:21-27 https://dx.doi.org/10.1134/S1024856010010057 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 23 2010 1 02 21-27
language	English
source	Enthalten in Atmospheric and oceanic optics 23(2010), 1 vom: Feb., Seite 21-27 volume:23 year:2010 number:1 month:02 pages:21-27
sourceStr	Enthalten in Atmospheric and oceanic optics 23(2010), 1 vom: Feb., Seite 21-27 volume:23 year:2010 number:1 month:02 pages:21-27
format_phy_str_mv	Article
institution	findex.gbv.de
topic_facet	Wave Packet Total Electron Content Vertical Total Electron Content Total Electron Content Variation Total Electron Content Measurement
isfreeaccess_bool	false
container_title	Atmospheric and oceanic optics
authorswithroles_txt_mv	Afraimovich, E. L. @@aut@@ Edemskiy, I. K. @@aut@@ Voeykov, S. V. @@aut@@ Yasyukevich, Yu. V. @@aut@@ Zhivetiev, I. V. @@aut@@
publishDateDaySort_date	2010-02-01T00:00:00Z
hierarchy_top_id	599674695
id	SPR026316609
language_de	englisch
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author	Afraimovich, E. L.
spellingShingle	Afraimovich, E. L. misc Wave Packet misc Total Electron Content misc Vertical Total Electron Content misc Total Electron Content Variation misc Total Electron Content Measurement Travelling wave packets generated by the solar terminator in the upper atmosphere
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topic_title	Travelling wave packets generated by the solar terminator in the upper atmosphere Wave Packet (dpeaa)DE-He213 Total Electron Content (dpeaa)DE-He213 Vertical Total Electron Content (dpeaa)DE-He213 Total Electron Content Variation (dpeaa)DE-He213 Total Electron Content Measurement (dpeaa)DE-He213
topic	misc Wave Packet misc Total Electron Content misc Vertical Total Electron Content misc Total Electron Content Variation misc Total Electron Content Measurement
topic_unstemmed	misc Wave Packet misc Total Electron Content misc Vertical Total Electron Content misc Total Electron Content Variation misc Total Electron Content Measurement
topic_browse	misc Wave Packet misc Total Electron Content misc Vertical Total Electron Content misc Total Electron Content Variation misc Total Electron Content Measurement
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title	Travelling wave packets generated by the solar terminator in the upper atmosphere
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title_full	Travelling wave packets generated by the solar terminator in the upper atmosphere
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author_browse	Afraimovich, E. L. Edemskiy, I. K. Voeykov, S. V. Yasyukevich, Yu. V. Zhivetiev, I. V.
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title_sort	travelling wave packets generated by the solar terminator in the upper atmosphere
title_auth	Travelling wave packets generated by the solar terminator in the upper atmosphere
abstract	Abstract For the first time, the morphology of a new type of midlatitude, medium scale, travelling ionospheric disturbances—travelling wave packets (TWPs)—is presented with the use of total electron content (TEC) measurements from the data of a global net of GPS receivers over a long time period from 1998 to 2007. The total amount of registered TWPs exceeds 275 000. In the context of time, TWPs are narrow-band TEC oscillations of an hour length with a period of about 10–20 min. TWPs are predominantly observed within 3 h after passing the morning solar terminator, when the TEC derivatives reach their maximum. © Pleiades Publishing, Ltd. 2010
abstractGer	Abstract For the first time, the morphology of a new type of midlatitude, medium scale, travelling ionospheric disturbances—travelling wave packets (TWPs)—is presented with the use of total electron content (TEC) measurements from the data of a global net of GPS receivers over a long time period from 1998 to 2007. The total amount of registered TWPs exceeds 275 000. In the context of time, TWPs are narrow-band TEC oscillations of an hour length with a period of about 10–20 min. TWPs are predominantly observed within 3 h after passing the morning solar terminator, when the TEC derivatives reach their maximum. © Pleiades Publishing, Ltd. 2010
abstract_unstemmed	Abstract For the first time, the morphology of a new type of midlatitude, medium scale, travelling ionospheric disturbances—travelling wave packets (TWPs)—is presented with the use of total electron content (TEC) measurements from the data of a global net of GPS receivers over a long time period from 1998 to 2007. The total amount of registered TWPs exceeds 275 000. In the context of time, TWPs are narrow-band TEC oscillations of an hour length with a period of about 10–20 min. TWPs are predominantly observed within 3 h after passing the morning solar terminator, when the TEC derivatives reach their maximum. © Pleiades Publishing, Ltd. 2010
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title_short	Travelling wave packets generated by the solar terminator in the upper atmosphere
url	https://dx.doi.org/10.1134/S1024856010010057
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author2	Edemskiy, I. K. Voeykov, S. V. Yasyukevich, Yu. V. Zhivetiev, I. V.
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up_date	2024-07-03T20:12:51.504Z
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fullrecord_marcxml	<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">SPR026316609</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230331234001.0</controlfield><controlfield tag="007">cr uuu---uuuuu</controlfield><controlfield tag="008">201007s2010 xx \|\|\|\|\|o 00\| \|\|eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1134/S1024856010010057</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)SPR026316609</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(SPR)S1024856010010057-e</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Afraimovich, E. L.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Travelling wave packets generated by the solar terminator in the upper atmosphere</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2010</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">Computermedien</subfield><subfield code="b">c</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Online-Ressource</subfield><subfield code="b">cr</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">© Pleiades Publishing, Ltd. 2010</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract For the first time, the morphology of a new type of midlatitude, medium scale, travelling ionospheric disturbances—travelling wave packets (TWPs)—is presented with the use of total electron content (TEC) measurements from the data of a global net of GPS receivers over a long time period from 1998 to 2007. 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Travelling wave packets generated by the solar terminator in the upper atmosphere

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