Spectra of L-band ionospheric scintillation over Nanjing

Abstract We report the spatiotemporal statistical characteristics of amplitude scintillation over Nanjing. A FFT method for computing scintillation intensity power spectra is briefly described. Using this method, the data with ISATM in Nanjing is analyzed. Spectra characteristic is presented and the...
Ausführliche Beschreibung

Gespeichert in:

Autor*in:	Fang, HanXian [verfasserIn] Yang, ShengGao [verfasserIn] Wang, SiCheng [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2012

Schlagwörter:	ionospheric scintillation scintillation power spectra electronic density irregularity spectra index

Übergeordnetes Werk:	Enthalten in: Chinese science bulletin - Beijing, China : Chinese Acad. of Sciences, 1997, 57(2012), 25 vom: 18. Aug., Seite 3375-3380
Übergeordnetes Werk:	volume:57 ; year:2012 ; number:25 ; day:18 ; month:08 ; pages:3375-3380

Links:	Volltext

DOI / URN:	10.1007/s11434-012-5365-y

Katalog-ID:	SPR019443455

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520			\|a Abstract We report the spatiotemporal statistical characteristics of amplitude scintillation over Nanjing. A FFT method for computing scintillation intensity power spectra is briefly described. Using this method, the data with ISATM in Nanjing is analyzed. Spectra characteristic is presented and the irregularities property is discussed preliminarily. The results reveal that the power spectra obtained for Nanjing is consistent with theoretical modeling. At frequencies below the Fresnel frequency, the power density plotted on log-log scale is almost constant whereas above it asymptotes to a straight line. The spectral index ranges from 1.71 to 1.92, which has positive correlation with the S4 index. Finally, the average drift velocity of irregularities is computed assumably and compared with that obtained for Xinxiang and Haikou.
650		4	\|a ionospheric scintillation \|7 (dpeaa)DE-He213
650		4	\|a scintillation power spectra \|7 (dpeaa)DE-He213
650		4	\|a electronic density irregularity \|7 (dpeaa)DE-He213
650		4	\|a spectra index \|7 (dpeaa)DE-He213
700	1		\|a Yang, ShengGao \|e verfasserin \|4 aut
700	1		\|a Wang, SiCheng \|e verfasserin \|4 aut
773	0	8	\|i Enthalten in \|t Chinese science bulletin \|d Beijing, China : Chinese Acad. of Sciences, 1997 \|g 57(2012), 25 vom: 18. Aug., Seite 3375-3380 \|w (DE-627)341897809 \|w (DE-600)2069521-4 \|x 1861-9541 \|7 nnns
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matchkey_str	article:18619541:2012----::pcroladoopeisitlai
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publishDate	2012
allfields	10.1007/s11434-012-5365-y doi (DE-627)SPR019443455 (SPR)s11434-012-5365-y-e DE-627 ger DE-627 rakwb eng 500 ASE 30.00 bkl Fang, HanXian verfasserin aut Spectra of L-band ionospheric scintillation over Nanjing 2012 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract We report the spatiotemporal statistical characteristics of amplitude scintillation over Nanjing. A FFT method for computing scintillation intensity power spectra is briefly described. Using this method, the data with ISATM in Nanjing is analyzed. Spectra characteristic is presented and the irregularities property is discussed preliminarily. The results reveal that the power spectra obtained for Nanjing is consistent with theoretical modeling. At frequencies below the Fresnel frequency, the power density plotted on log-log scale is almost constant whereas above it asymptotes to a straight line. The spectral index ranges from 1.71 to 1.92, which has positive correlation with the S4 index. Finally, the average drift velocity of irregularities is computed assumably and compared with that obtained for Xinxiang and Haikou. ionospheric scintillation (dpeaa)DE-He213 scintillation power spectra (dpeaa)DE-He213 electronic density irregularity (dpeaa)DE-He213 spectra index (dpeaa)DE-He213 Yang, ShengGao verfasserin aut Wang, SiCheng verfasserin aut Enthalten in Chinese science bulletin Beijing, China : Chinese Acad. of Sciences, 1997 57(2012), 25 vom: 18. Aug., Seite 3375-3380 (DE-627)341897809 (DE-600)2069521-4 1861-9541 nnns volume:57 year:2012 number:25 day:18 month:08 pages:3375-3380 https://dx.doi.org/10.1007/s11434-012-5365-y kostenfrei 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_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_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_213 GBV_ILN_230 GBV_ILN_266 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2055 GBV_ILN_2059 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2106 GBV_ILN_2108 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_2522 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 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_4328 GBV_ILN_4333 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 30.00 ASE AR 57 2012 25 18 08 3375-3380
spelling	10.1007/s11434-012-5365-y doi (DE-627)SPR019443455 (SPR)s11434-012-5365-y-e DE-627 ger DE-627 rakwb eng 500 ASE 30.00 bkl Fang, HanXian verfasserin aut Spectra of L-band ionospheric scintillation over Nanjing 2012 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract We report the spatiotemporal statistical characteristics of amplitude scintillation over Nanjing. A FFT method for computing scintillation intensity power spectra is briefly described. Using this method, the data with ISATM in Nanjing is analyzed. Spectra characteristic is presented and the irregularities property is discussed preliminarily. The results reveal that the power spectra obtained for Nanjing is consistent with theoretical modeling. At frequencies below the Fresnel frequency, the power density plotted on log-log scale is almost constant whereas above it asymptotes to a straight line. The spectral index ranges from 1.71 to 1.92, which has positive correlation with the S4 index. Finally, the average drift velocity of irregularities is computed assumably and compared with that obtained for Xinxiang and Haikou. ionospheric scintillation (dpeaa)DE-He213 scintillation power spectra (dpeaa)DE-He213 electronic density irregularity (dpeaa)DE-He213 spectra index (dpeaa)DE-He213 Yang, ShengGao verfasserin aut Wang, SiCheng verfasserin aut Enthalten in Chinese science bulletin Beijing, China : Chinese Acad. of Sciences, 1997 57(2012), 25 vom: 18. Aug., Seite 3375-3380 (DE-627)341897809 (DE-600)2069521-4 1861-9541 nnns volume:57 year:2012 number:25 day:18 month:08 pages:3375-3380 https://dx.doi.org/10.1007/s11434-012-5365-y kostenfrei 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_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_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_213 GBV_ILN_230 GBV_ILN_266 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2055 GBV_ILN_2059 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2106 GBV_ILN_2108 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_2522 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 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_4328 GBV_ILN_4333 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 30.00 ASE AR 57 2012 25 18 08 3375-3380
allfields_unstemmed	10.1007/s11434-012-5365-y doi (DE-627)SPR019443455 (SPR)s11434-012-5365-y-e DE-627 ger DE-627 rakwb eng 500 ASE 30.00 bkl Fang, HanXian verfasserin aut Spectra of L-band ionospheric scintillation over Nanjing 2012 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract We report the spatiotemporal statistical characteristics of amplitude scintillation over Nanjing. A FFT method for computing scintillation intensity power spectra is briefly described. Using this method, the data with ISATM in Nanjing is analyzed. Spectra characteristic is presented and the irregularities property is discussed preliminarily. The results reveal that the power spectra obtained for Nanjing is consistent with theoretical modeling. At frequencies below the Fresnel frequency, the power density plotted on log-log scale is almost constant whereas above it asymptotes to a straight line. The spectral index ranges from 1.71 to 1.92, which has positive correlation with the S4 index. Finally, the average drift velocity of irregularities is computed assumably and compared with that obtained for Xinxiang and Haikou. ionospheric scintillation (dpeaa)DE-He213 scintillation power spectra (dpeaa)DE-He213 electronic density irregularity (dpeaa)DE-He213 spectra index (dpeaa)DE-He213 Yang, ShengGao verfasserin aut Wang, SiCheng verfasserin aut Enthalten in Chinese science bulletin Beijing, China : Chinese Acad. of Sciences, 1997 57(2012), 25 vom: 18. Aug., Seite 3375-3380 (DE-627)341897809 (DE-600)2069521-4 1861-9541 nnns volume:57 year:2012 number:25 day:18 month:08 pages:3375-3380 https://dx.doi.org/10.1007/s11434-012-5365-y kostenfrei 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_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_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_213 GBV_ILN_230 GBV_ILN_266 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2055 GBV_ILN_2059 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2106 GBV_ILN_2108 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_2522 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 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_4328 GBV_ILN_4333 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 30.00 ASE AR 57 2012 25 18 08 3375-3380
allfieldsGer	10.1007/s11434-012-5365-y doi (DE-627)SPR019443455 (SPR)s11434-012-5365-y-e DE-627 ger DE-627 rakwb eng 500 ASE 30.00 bkl Fang, HanXian verfasserin aut Spectra of L-band ionospheric scintillation over Nanjing 2012 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract We report the spatiotemporal statistical characteristics of amplitude scintillation over Nanjing. A FFT method for computing scintillation intensity power spectra is briefly described. Using this method, the data with ISATM in Nanjing is analyzed. Spectra characteristic is presented and the irregularities property is discussed preliminarily. The results reveal that the power spectra obtained for Nanjing is consistent with theoretical modeling. At frequencies below the Fresnel frequency, the power density plotted on log-log scale is almost constant whereas above it asymptotes to a straight line. The spectral index ranges from 1.71 to 1.92, which has positive correlation with the S4 index. Finally, the average drift velocity of irregularities is computed assumably and compared with that obtained for Xinxiang and Haikou. ionospheric scintillation (dpeaa)DE-He213 scintillation power spectra (dpeaa)DE-He213 electronic density irregularity (dpeaa)DE-He213 spectra index (dpeaa)DE-He213 Yang, ShengGao verfasserin aut Wang, SiCheng verfasserin aut Enthalten in Chinese science bulletin Beijing, China : Chinese Acad. of Sciences, 1997 57(2012), 25 vom: 18. Aug., Seite 3375-3380 (DE-627)341897809 (DE-600)2069521-4 1861-9541 nnns volume:57 year:2012 number:25 day:18 month:08 pages:3375-3380 https://dx.doi.org/10.1007/s11434-012-5365-y kostenfrei 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_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_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_213 GBV_ILN_230 GBV_ILN_266 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2055 GBV_ILN_2059 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2106 GBV_ILN_2108 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_2522 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 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_4328 GBV_ILN_4333 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 30.00 ASE AR 57 2012 25 18 08 3375-3380
allfieldsSound	10.1007/s11434-012-5365-y doi (DE-627)SPR019443455 (SPR)s11434-012-5365-y-e DE-627 ger DE-627 rakwb eng 500 ASE 30.00 bkl Fang, HanXian verfasserin aut Spectra of L-band ionospheric scintillation over Nanjing 2012 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract We report the spatiotemporal statistical characteristics of amplitude scintillation over Nanjing. A FFT method for computing scintillation intensity power spectra is briefly described. Using this method, the data with ISATM in Nanjing is analyzed. Spectra characteristic is presented and the irregularities property is discussed preliminarily. The results reveal that the power spectra obtained for Nanjing is consistent with theoretical modeling. At frequencies below the Fresnel frequency, the power density plotted on log-log scale is almost constant whereas above it asymptotes to a straight line. The spectral index ranges from 1.71 to 1.92, which has positive correlation with the S4 index. Finally, the average drift velocity of irregularities is computed assumably and compared with that obtained for Xinxiang and Haikou. ionospheric scintillation (dpeaa)DE-He213 scintillation power spectra (dpeaa)DE-He213 electronic density irregularity (dpeaa)DE-He213 spectra index (dpeaa)DE-He213 Yang, ShengGao verfasserin aut Wang, SiCheng verfasserin aut Enthalten in Chinese science bulletin Beijing, China : Chinese Acad. of Sciences, 1997 57(2012), 25 vom: 18. Aug., Seite 3375-3380 (DE-627)341897809 (DE-600)2069521-4 1861-9541 nnns volume:57 year:2012 number:25 day:18 month:08 pages:3375-3380 https://dx.doi.org/10.1007/s11434-012-5365-y kostenfrei 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_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_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_213 GBV_ILN_230 GBV_ILN_266 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2005 GBV_ILN_2007 GBV_ILN_2009 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2018 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2055 GBV_ILN_2059 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2106 GBV_ILN_2108 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_2522 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 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_4328 GBV_ILN_4333 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 30.00 ASE AR 57 2012 25 18 08 3375-3380
language	English
source	Enthalten in Chinese science bulletin 57(2012), 25 vom: 18. Aug., Seite 3375-3380 volume:57 year:2012 number:25 day:18 month:08 pages:3375-3380
sourceStr	Enthalten in Chinese science bulletin 57(2012), 25 vom: 18. Aug., Seite 3375-3380 volume:57 year:2012 number:25 day:18 month:08 pages:3375-3380
format_phy_str_mv	Article
institution	findex.gbv.de
topic_facet	ionospheric scintillation scintillation power spectra electronic density irregularity spectra index
dewey-raw	500
isfreeaccess_bool	true
container_title	Chinese science bulletin
authorswithroles_txt_mv	Fang, HanXian @@aut@@ Yang, ShengGao @@aut@@ Wang, SiCheng @@aut@@
publishDateDaySort_date	2012-08-18T00:00:00Z
hierarchy_top_id	341897809
dewey-sort	3500
id	SPR019443455
language_de	englisch
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author	Fang, HanXian
spellingShingle	Fang, HanXian ddc 500 bkl 30.00 misc ionospheric scintillation misc scintillation power spectra misc electronic density irregularity misc spectra index Spectra of L-band ionospheric scintillation over Nanjing
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topic_title	500 ASE 30.00 bkl Spectra of L-band ionospheric scintillation over Nanjing ionospheric scintillation (dpeaa)DE-He213 scintillation power spectra (dpeaa)DE-He213 electronic density irregularity (dpeaa)DE-He213 spectra index (dpeaa)DE-He213
topic	ddc 500 bkl 30.00 misc ionospheric scintillation misc scintillation power spectra misc electronic density irregularity misc spectra index
topic_unstemmed	ddc 500 bkl 30.00 misc ionospheric scintillation misc scintillation power spectra misc electronic density irregularity misc spectra index
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title	Spectra of L-band ionospheric scintillation over Nanjing
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title_full	Spectra of L-band ionospheric scintillation over Nanjing
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author_browse	Fang, HanXian Yang, ShengGao Wang, SiCheng
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title_sort	spectra of l-band ionospheric scintillation over nanjing
title_auth	Spectra of L-band ionospheric scintillation over Nanjing
abstract	Abstract We report the spatiotemporal statistical characteristics of amplitude scintillation over Nanjing. A FFT method for computing scintillation intensity power spectra is briefly described. Using this method, the data with ISATM in Nanjing is analyzed. Spectra characteristic is presented and the irregularities property is discussed preliminarily. The results reveal that the power spectra obtained for Nanjing is consistent with theoretical modeling. At frequencies below the Fresnel frequency, the power density plotted on log-log scale is almost constant whereas above it asymptotes to a straight line. The spectral index ranges from 1.71 to 1.92, which has positive correlation with the S4 index. Finally, the average drift velocity of irregularities is computed assumably and compared with that obtained for Xinxiang and Haikou.
abstractGer	Abstract We report the spatiotemporal statistical characteristics of amplitude scintillation over Nanjing. A FFT method for computing scintillation intensity power spectra is briefly described. Using this method, the data with ISATM in Nanjing is analyzed. Spectra characteristic is presented and the irregularities property is discussed preliminarily. The results reveal that the power spectra obtained for Nanjing is consistent with theoretical modeling. At frequencies below the Fresnel frequency, the power density plotted on log-log scale is almost constant whereas above it asymptotes to a straight line. The spectral index ranges from 1.71 to 1.92, which has positive correlation with the S4 index. Finally, the average drift velocity of irregularities is computed assumably and compared with that obtained for Xinxiang and Haikou.
abstract_unstemmed	Abstract We report the spatiotemporal statistical characteristics of amplitude scintillation over Nanjing. A FFT method for computing scintillation intensity power spectra is briefly described. Using this method, the data with ISATM in Nanjing is analyzed. Spectra characteristic is presented and the irregularities property is discussed preliminarily. The results reveal that the power spectra obtained for Nanjing is consistent with theoretical modeling. At frequencies below the Fresnel frequency, the power density plotted on log-log scale is almost constant whereas above it asymptotes to a straight line. The spectral index ranges from 1.71 to 1.92, which has positive correlation with the S4 index. Finally, the average drift velocity of irregularities is computed assumably and compared with that obtained for Xinxiang and Haikou.
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title_short	Spectra of L-band ionospheric scintillation over Nanjing
url	https://dx.doi.org/10.1007/s11434-012-5365-y
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score	7.399932

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Spectra of L-band ionospheric scintillation over Nanjing

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