Comparisons of VHF radar, optical, and temperature fluctuation measurements ofCn2,r0 andθ0

Summary Comparisons are made of profiles of the refractive index structure parameter (Cn2) and two derived quantities, transverse coherence length (r0) and isoplanatic angle (θ0), from measurements taken with a suite of instruments including a 49.25 MHz pulsed Doppler radar with a phased array anten...
Ausführliche Beschreibung

Gespeichert in:

Autor*in:	Eaton, F. D. [verfasserIn] Peterson, W. A. Hines, J. R. Peterman, K. R. Good, R. E. Beland, R. R. Brown, J. H.

Format:	Artikel
Sprache:	Englisch

Erschienen:	1988

Schlagwörter:	Radar Array Antenna Doppler Radar Radar Reflectivity Phase Array Antenna

Systematik:	RA 1000

Anmerkung:	© Springer-Verlag 1988

Übergeordnetes Werk:	Enthalten in: Theoretical and applied climatology - Springer-Verlag, 1986, 39(1988), 1 vom: März, Seite 17-29
Übergeordnetes Werk:	volume:39 ; year:1988 ; number:1 ; month:03 ; pages:17-29

Links:	Volltext

DOI / URN:	10.1007/BF00867654

Katalog-ID:	OLC2048430112

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520			\|a Summary Comparisons are made of profiles of the refractive index structure parameter (Cn2) and two derived quantities, transverse coherence length (r0) and isoplanatic angle (θ0), from measurements taken with a suite of instruments including a 49.25 MHz pulsed Doppler radar with a phased array antenna, an isoplanometer, anr0 system, a stellar scintillometer, and temperature fluctuation sensors mounted on a thermosonde. The radar, which obtained data from 2 to 22 km above ground level (AGL), was operated to provide 150 m height resolution ofCn2. The stellar scintillometer obtained aCn2 profile defined at seven heights from 2.2 to 18.5 km AGL, while the thermosonde obtained and transmitted data every 20 m. The isoplanometer andr0 system provided integratedpath (ground-to-space) values. The method used for calibrating the radar is discussed as well as the angular dependency of radar-returned power as influenced by specular reflections. The method used for extracting opticalCn2 from radar reflectivity by eliminating humidity effects is discussed, as is speculation as to differences in results found from the different measurement techniques.
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allfields	10.1007/BF00867654 doi (DE-627)OLC2048430112 (DE-He213)BF00867654-p DE-627 ger DE-627 rakwb eng 550 VZ 14 ssgn RA 1000 VZ rvk Eaton, F. D. verfasserin aut Comparisons of VHF radar, optical, and temperature fluctuation measurements ofCn2,r0 andθ0 1988 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer-Verlag 1988 Summary Comparisons are made of profiles of the refractive index structure parameter (Cn2) and two derived quantities, transverse coherence length (r0) and isoplanatic angle (θ0), from measurements taken with a suite of instruments including a 49.25 MHz pulsed Doppler radar with a phased array antenna, an isoplanometer, anr0 system, a stellar scintillometer, and temperature fluctuation sensors mounted on a thermosonde. The radar, which obtained data from 2 to 22 km above ground level (AGL), was operated to provide 150 m height resolution ofCn2. The stellar scintillometer obtained aCn2 profile defined at seven heights from 2.2 to 18.5 km AGL, while the thermosonde obtained and transmitted data every 20 m. The isoplanometer andr0 system provided integratedpath (ground-to-space) values. The method used for calibrating the radar is discussed as well as the angular dependency of radar-returned power as influenced by specular reflections. The method used for extracting opticalCn2 from radar reflectivity by eliminating humidity effects is discussed, as is speculation as to differences in results found from the different measurement techniques. Radar Array Antenna Doppler Radar Radar Reflectivity Phase Array Antenna Peterson, W. A. aut Hines, J. R. aut Peterman, K. R. aut Good, R. E. aut Beland, R. R. aut Brown, J. H. aut Enthalten in Theoretical and applied climatology Springer-Verlag, 1986 39(1988), 1 vom: März, Seite 17-29 (DE-627)129958808 (DE-600)405799-5 (DE-576)01552857X 0177-798X nnns volume:39 year:1988 number:1 month:03 pages:17-29 https://doi.org/10.1007/BF00867654 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-GEO SSG-OPC-GGO GBV_ILN_11 GBV_ILN_22 GBV_ILN_31 GBV_ILN_40 GBV_ILN_62 GBV_ILN_70 GBV_ILN_130 GBV_ILN_601 GBV_ILN_2001 GBV_ILN_2006 GBV_ILN_2010 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_4012 GBV_ILN_4029 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4103 GBV_ILN_4125 GBV_ILN_4193 GBV_ILN_4305 GBV_ILN_4307 GBV_ILN_4311 GBV_ILN_4325 GBV_ILN_4330 RA 1000 AR 39 1988 1 03 17-29
spelling	10.1007/BF00867654 doi (DE-627)OLC2048430112 (DE-He213)BF00867654-p DE-627 ger DE-627 rakwb eng 550 VZ 14 ssgn RA 1000 VZ rvk Eaton, F. D. verfasserin aut Comparisons of VHF radar, optical, and temperature fluctuation measurements ofCn2,r0 andθ0 1988 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer-Verlag 1988 Summary Comparisons are made of profiles of the refractive index structure parameter (Cn2) and two derived quantities, transverse coherence length (r0) and isoplanatic angle (θ0), from measurements taken with a suite of instruments including a 49.25 MHz pulsed Doppler radar with a phased array antenna, an isoplanometer, anr0 system, a stellar scintillometer, and temperature fluctuation sensors mounted on a thermosonde. The radar, which obtained data from 2 to 22 km above ground level (AGL), was operated to provide 150 m height resolution ofCn2. The stellar scintillometer obtained aCn2 profile defined at seven heights from 2.2 to 18.5 km AGL, while the thermosonde obtained and transmitted data every 20 m. The isoplanometer andr0 system provided integratedpath (ground-to-space) values. The method used for calibrating the radar is discussed as well as the angular dependency of radar-returned power as influenced by specular reflections. The method used for extracting opticalCn2 from radar reflectivity by eliminating humidity effects is discussed, as is speculation as to differences in results found from the different measurement techniques. Radar Array Antenna Doppler Radar Radar Reflectivity Phase Array Antenna Peterson, W. A. aut Hines, J. R. aut Peterman, K. R. aut Good, R. E. aut Beland, R. R. aut Brown, J. H. aut Enthalten in Theoretical and applied climatology Springer-Verlag, 1986 39(1988), 1 vom: März, Seite 17-29 (DE-627)129958808 (DE-600)405799-5 (DE-576)01552857X 0177-798X nnns volume:39 year:1988 number:1 month:03 pages:17-29 https://doi.org/10.1007/BF00867654 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-GEO SSG-OPC-GGO GBV_ILN_11 GBV_ILN_22 GBV_ILN_31 GBV_ILN_40 GBV_ILN_62 GBV_ILN_70 GBV_ILN_130 GBV_ILN_601 GBV_ILN_2001 GBV_ILN_2006 GBV_ILN_2010 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_4012 GBV_ILN_4029 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4103 GBV_ILN_4125 GBV_ILN_4193 GBV_ILN_4305 GBV_ILN_4307 GBV_ILN_4311 GBV_ILN_4325 GBV_ILN_4330 RA 1000 AR 39 1988 1 03 17-29
allfields_unstemmed	10.1007/BF00867654 doi (DE-627)OLC2048430112 (DE-He213)BF00867654-p DE-627 ger DE-627 rakwb eng 550 VZ 14 ssgn RA 1000 VZ rvk Eaton, F. D. verfasserin aut Comparisons of VHF radar, optical, and temperature fluctuation measurements ofCn2,r0 andθ0 1988 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer-Verlag 1988 Summary Comparisons are made of profiles of the refractive index structure parameter (Cn2) and two derived quantities, transverse coherence length (r0) and isoplanatic angle (θ0), from measurements taken with a suite of instruments including a 49.25 MHz pulsed Doppler radar with a phased array antenna, an isoplanometer, anr0 system, a stellar scintillometer, and temperature fluctuation sensors mounted on a thermosonde. The radar, which obtained data from 2 to 22 km above ground level (AGL), was operated to provide 150 m height resolution ofCn2. The stellar scintillometer obtained aCn2 profile defined at seven heights from 2.2 to 18.5 km AGL, while the thermosonde obtained and transmitted data every 20 m. The isoplanometer andr0 system provided integratedpath (ground-to-space) values. The method used for calibrating the radar is discussed as well as the angular dependency of radar-returned power as influenced by specular reflections. The method used for extracting opticalCn2 from radar reflectivity by eliminating humidity effects is discussed, as is speculation as to differences in results found from the different measurement techniques. Radar Array Antenna Doppler Radar Radar Reflectivity Phase Array Antenna Peterson, W. A. aut Hines, J. R. aut Peterman, K. R. aut Good, R. E. aut Beland, R. R. aut Brown, J. H. aut Enthalten in Theoretical and applied climatology Springer-Verlag, 1986 39(1988), 1 vom: März, Seite 17-29 (DE-627)129958808 (DE-600)405799-5 (DE-576)01552857X 0177-798X nnns volume:39 year:1988 number:1 month:03 pages:17-29 https://doi.org/10.1007/BF00867654 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-GEO SSG-OPC-GGO GBV_ILN_11 GBV_ILN_22 GBV_ILN_31 GBV_ILN_40 GBV_ILN_62 GBV_ILN_70 GBV_ILN_130 GBV_ILN_601 GBV_ILN_2001 GBV_ILN_2006 GBV_ILN_2010 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_4012 GBV_ILN_4029 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4103 GBV_ILN_4125 GBV_ILN_4193 GBV_ILN_4305 GBV_ILN_4307 GBV_ILN_4311 GBV_ILN_4325 GBV_ILN_4330 RA 1000 AR 39 1988 1 03 17-29
allfieldsGer	10.1007/BF00867654 doi (DE-627)OLC2048430112 (DE-He213)BF00867654-p DE-627 ger DE-627 rakwb eng 550 VZ 14 ssgn RA 1000 VZ rvk Eaton, F. D. verfasserin aut Comparisons of VHF radar, optical, and temperature fluctuation measurements ofCn2,r0 andθ0 1988 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer-Verlag 1988 Summary Comparisons are made of profiles of the refractive index structure parameter (Cn2) and two derived quantities, transverse coherence length (r0) and isoplanatic angle (θ0), from measurements taken with a suite of instruments including a 49.25 MHz pulsed Doppler radar with a phased array antenna, an isoplanometer, anr0 system, a stellar scintillometer, and temperature fluctuation sensors mounted on a thermosonde. The radar, which obtained data from 2 to 22 km above ground level (AGL), was operated to provide 150 m height resolution ofCn2. The stellar scintillometer obtained aCn2 profile defined at seven heights from 2.2 to 18.5 km AGL, while the thermosonde obtained and transmitted data every 20 m. The isoplanometer andr0 system provided integratedpath (ground-to-space) values. The method used for calibrating the radar is discussed as well as the angular dependency of radar-returned power as influenced by specular reflections. The method used for extracting opticalCn2 from radar reflectivity by eliminating humidity effects is discussed, as is speculation as to differences in results found from the different measurement techniques. Radar Array Antenna Doppler Radar Radar Reflectivity Phase Array Antenna Peterson, W. A. aut Hines, J. R. aut Peterman, K. R. aut Good, R. E. aut Beland, R. R. aut Brown, J. H. aut Enthalten in Theoretical and applied climatology Springer-Verlag, 1986 39(1988), 1 vom: März, Seite 17-29 (DE-627)129958808 (DE-600)405799-5 (DE-576)01552857X 0177-798X nnns volume:39 year:1988 number:1 month:03 pages:17-29 https://doi.org/10.1007/BF00867654 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-GEO SSG-OPC-GGO GBV_ILN_11 GBV_ILN_22 GBV_ILN_31 GBV_ILN_40 GBV_ILN_62 GBV_ILN_70 GBV_ILN_130 GBV_ILN_601 GBV_ILN_2001 GBV_ILN_2006 GBV_ILN_2010 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_4012 GBV_ILN_4029 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4103 GBV_ILN_4125 GBV_ILN_4193 GBV_ILN_4305 GBV_ILN_4307 GBV_ILN_4311 GBV_ILN_4325 GBV_ILN_4330 RA 1000 AR 39 1988 1 03 17-29
allfieldsSound	10.1007/BF00867654 doi (DE-627)OLC2048430112 (DE-He213)BF00867654-p DE-627 ger DE-627 rakwb eng 550 VZ 14 ssgn RA 1000 VZ rvk Eaton, F. D. verfasserin aut Comparisons of VHF radar, optical, and temperature fluctuation measurements ofCn2,r0 andθ0 1988 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer-Verlag 1988 Summary Comparisons are made of profiles of the refractive index structure parameter (Cn2) and two derived quantities, transverse coherence length (r0) and isoplanatic angle (θ0), from measurements taken with a suite of instruments including a 49.25 MHz pulsed Doppler radar with a phased array antenna, an isoplanometer, anr0 system, a stellar scintillometer, and temperature fluctuation sensors mounted on a thermosonde. The radar, which obtained data from 2 to 22 km above ground level (AGL), was operated to provide 150 m height resolution ofCn2. The stellar scintillometer obtained aCn2 profile defined at seven heights from 2.2 to 18.5 km AGL, while the thermosonde obtained and transmitted data every 20 m. The isoplanometer andr0 system provided integratedpath (ground-to-space) values. The method used for calibrating the radar is discussed as well as the angular dependency of radar-returned power as influenced by specular reflections. The method used for extracting opticalCn2 from radar reflectivity by eliminating humidity effects is discussed, as is speculation as to differences in results found from the different measurement techniques. Radar Array Antenna Doppler Radar Radar Reflectivity Phase Array Antenna Peterson, W. A. aut Hines, J. R. aut Peterman, K. R. aut Good, R. E. aut Beland, R. R. aut Brown, J. H. aut Enthalten in Theoretical and applied climatology Springer-Verlag, 1986 39(1988), 1 vom: März, Seite 17-29 (DE-627)129958808 (DE-600)405799-5 (DE-576)01552857X 0177-798X nnns volume:39 year:1988 number:1 month:03 pages:17-29 https://doi.org/10.1007/BF00867654 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-GEO SSG-OPC-GGO GBV_ILN_11 GBV_ILN_22 GBV_ILN_31 GBV_ILN_40 GBV_ILN_62 GBV_ILN_70 GBV_ILN_130 GBV_ILN_601 GBV_ILN_2001 GBV_ILN_2006 GBV_ILN_2010 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_4012 GBV_ILN_4029 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4103 GBV_ILN_4125 GBV_ILN_4193 GBV_ILN_4305 GBV_ILN_4307 GBV_ILN_4311 GBV_ILN_4325 GBV_ILN_4330 RA 1000 AR 39 1988 1 03 17-29
language	English
source	Enthalten in Theoretical and applied climatology 39(1988), 1 vom: März, Seite 17-29 volume:39 year:1988 number:1 month:03 pages:17-29
sourceStr	Enthalten in Theoretical and applied climatology 39(1988), 1 vom: März, Seite 17-29 volume:39 year:1988 number:1 month:03 pages:17-29
format_phy_str_mv	Article
institution	findex.gbv.de
topic_facet	Radar Array Antenna Doppler Radar Radar Reflectivity Phase Array Antenna
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container_title	Theoretical and applied climatology
authorswithroles_txt_mv	Eaton, F. D. @@aut@@ Peterson, W. A. @@aut@@ Hines, J. R. @@aut@@ Peterman, K. R. @@aut@@ Good, R. E. @@aut@@ Beland, R. R. @@aut@@ Brown, J. H. @@aut@@
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author	Eaton, F. D.
spellingShingle	Eaton, F. D. ddc 550 ssgn 14 rvk RA 1000 misc Radar misc Array Antenna misc Doppler Radar misc Radar Reflectivity misc Phase Array Antenna Comparisons of VHF radar, optical, and temperature fluctuation measurements ofCn2,r0 andθ0
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topic_title	550 VZ 14 ssgn RA 1000 VZ rvk Comparisons of VHF radar, optical, and temperature fluctuation measurements ofCn2,r0 andθ0 Radar Array Antenna Doppler Radar Radar Reflectivity Phase Array Antenna
topic	ddc 550 ssgn 14 rvk RA 1000 misc Radar misc Array Antenna misc Doppler Radar misc Radar Reflectivity misc Phase Array Antenna
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title	Comparisons of VHF radar, optical, and temperature fluctuation measurements ofCn2,r0 andθ0
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title_full	Comparisons of VHF radar, optical, and temperature fluctuation measurements ofCn2,r0 andθ0
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author_browse	Eaton, F. D. Peterson, W. A. Hines, J. R. Peterman, K. R. Good, R. E. Beland, R. R. Brown, J. H.
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title_sort	comparisons of vhf radar, optical, and temperature fluctuation measurements ofcn2,r0 andθ0
title_auth	Comparisons of VHF radar, optical, and temperature fluctuation measurements ofCn2,r0 andθ0
abstract	Summary Comparisons are made of profiles of the refractive index structure parameter (Cn2) and two derived quantities, transverse coherence length (r0) and isoplanatic angle (θ0), from measurements taken with a suite of instruments including a 49.25 MHz pulsed Doppler radar with a phased array antenna, an isoplanometer, anr0 system, a stellar scintillometer, and temperature fluctuation sensors mounted on a thermosonde. The radar, which obtained data from 2 to 22 km above ground level (AGL), was operated to provide 150 m height resolution ofCn2. The stellar scintillometer obtained aCn2 profile defined at seven heights from 2.2 to 18.5 km AGL, while the thermosonde obtained and transmitted data every 20 m. The isoplanometer andr0 system provided integratedpath (ground-to-space) values. The method used for calibrating the radar is discussed as well as the angular dependency of radar-returned power as influenced by specular reflections. The method used for extracting opticalCn2 from radar reflectivity by eliminating humidity effects is discussed, as is speculation as to differences in results found from the different measurement techniques. © Springer-Verlag 1988
abstractGer	Summary Comparisons are made of profiles of the refractive index structure parameter (Cn2) and two derived quantities, transverse coherence length (r0) and isoplanatic angle (θ0), from measurements taken with a suite of instruments including a 49.25 MHz pulsed Doppler radar with a phased array antenna, an isoplanometer, anr0 system, a stellar scintillometer, and temperature fluctuation sensors mounted on a thermosonde. The radar, which obtained data from 2 to 22 km above ground level (AGL), was operated to provide 150 m height resolution ofCn2. The stellar scintillometer obtained aCn2 profile defined at seven heights from 2.2 to 18.5 km AGL, while the thermosonde obtained and transmitted data every 20 m. The isoplanometer andr0 system provided integratedpath (ground-to-space) values. The method used for calibrating the radar is discussed as well as the angular dependency of radar-returned power as influenced by specular reflections. The method used for extracting opticalCn2 from radar reflectivity by eliminating humidity effects is discussed, as is speculation as to differences in results found from the different measurement techniques. © Springer-Verlag 1988
abstract_unstemmed	Summary Comparisons are made of profiles of the refractive index structure parameter (Cn2) and two derived quantities, transverse coherence length (r0) and isoplanatic angle (θ0), from measurements taken with a suite of instruments including a 49.25 MHz pulsed Doppler radar with a phased array antenna, an isoplanometer, anr0 system, a stellar scintillometer, and temperature fluctuation sensors mounted on a thermosonde. The radar, which obtained data from 2 to 22 km above ground level (AGL), was operated to provide 150 m height resolution ofCn2. The stellar scintillometer obtained aCn2 profile defined at seven heights from 2.2 to 18.5 km AGL, while the thermosonde obtained and transmitted data every 20 m. The isoplanometer andr0 system provided integratedpath (ground-to-space) values. The method used for calibrating the radar is discussed as well as the angular dependency of radar-returned power as influenced by specular reflections. The method used for extracting opticalCn2 from radar reflectivity by eliminating humidity effects is discussed, as is speculation as to differences in results found from the different measurement techniques. © Springer-Verlag 1988
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title_short	Comparisons of VHF radar, optical, and temperature fluctuation measurements ofCn2,r0 andθ0
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