Venus' cloud top wind study: Coordinated Akatsuki/UVI with cloud tracking and TNG/HARPS-N with Doppler velocimetry observations

We present new wind velocities and its variability at Venus cloud-tops (≈70 km) based on coordinated observations with two complementary techniques: (1) space-based cloud-tracking using JAXA's Akatsuki/UVI imaging and (2) ground-based Doppler velocimetry using the TNG/HARPS-N (Telescopio Nazion...
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Autor*in:	Gonçalves, Ruben [verfasserIn] Machado, Pedro [verfasserIn] Widemann, Thomas [verfasserIn] Peralta, Javier [verfasserIn] Watanabe, Shigeto [verfasserIn] Yamazaki, Atsushi [verfasserIn] Satoh, Takehiko [verfasserIn] Takagi, Masahiro [verfasserIn] Ogohara, Kazunori [verfasserIn] Lee, Yeon-Joo [verfasserIn] Harutyunyan, Avet [verfasserIn] Silva, José [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2019

Schlagwörter:	Venus Atmosphere Dynamics Akatsuki Spectroscopy Cloud tracking Doppler velocimetry

Übergeordnetes Werk:	Enthalten in: Icarus - Orlando, Fla. : Academ. Press, 1962, 335
Übergeordnetes Werk:	volume:335

DOI / URN:	10.1016/j.icarus.2019.113418

Katalog-ID:	ELV003277844

Internformat


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100	1		\|a Gonçalves, Ruben \|e verfasserin \|4 aut
245	1	0	\|a Venus' cloud top wind study: Coordinated Akatsuki/UVI with cloud tracking and TNG/HARPS-N with Doppler velocimetry observations
264		1	\|c 2019
336			\|a nicht spezifiziert \|b zzz \|2 rdacontent
337			\|a Computermedien \|b c \|2 rdamedia
338			\|a Online-Ressource \|b cr \|2 rdacarrier
520			\|a We present new wind velocities and its variability at Venus cloud-tops (≈70 km) based on coordinated observations with two complementary techniques: (1) space-based cloud-tracking using JAXA's Akatsuki/UVI imaging and (2) ground-based Doppler velocimetry using the TNG/HARPS-N (Telescopio Nazionale Galileo). This was the first use of HARPS-N to observe a Solar system planetary atmosphere. The measurement of both zonal and meridional wind velocities and the constraints of temporal and spatial wind variability at cloud top is essential to our understanding of the mechanisms which yield and maintain the dynamics of Venus' atmospheric superrotational circulation.
650		4	\|a Venus
650		4	\|a Atmosphere
650		4	\|a Dynamics
650		4	\|a Akatsuki
650		4	\|a Spectroscopy
650		4	\|a Cloud tracking
650		4	\|a Doppler velocimetry
700	1		\|a Machado, Pedro \|e verfasserin \|4 aut
700	1		\|a Widemann, Thomas \|e verfasserin \|4 aut
700	1		\|a Peralta, Javier \|e verfasserin \|4 aut
700	1		\|a Watanabe, Shigeto \|e verfasserin \|4 aut
700	1		\|a Yamazaki, Atsushi \|e verfasserin \|4 aut
700	1		\|a Satoh, Takehiko \|e verfasserin \|4 aut
700	1		\|a Takagi, Masahiro \|e verfasserin \|4 aut
700	1		\|a Ogohara, Kazunori \|e verfasserin \|4 aut
700	1		\|a Lee, Yeon-Joo \|e verfasserin \|4 aut
700	1		\|a Harutyunyan, Avet \|e verfasserin \|4 aut
700	1		\|a Silva, José \|e verfasserin \|4 aut
773	0	8	\|i Enthalten in \|t Icarus \|d Orlando, Fla. : Academ. Press, 1962 \|g 335 \|h Online-Ressource \|w (DE-627)266881521 \|w (DE-600)1467991-7 \|w (DE-576)104193743 \|x 0019-1035 \|7 nnns
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912			\|a GBV_ILN_602
912			\|a GBV_ILN_702
912			\|a GBV_ILN_2003
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912			\|a GBV_ILN_2021
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912			\|a GBV_ILN_4338
912			\|a GBV_ILN_4393
936	b	k	\|a 39.50 \|j Sonnensystem: Allgemeines
951			\|a AR
952			\|d 335

Indexfelder

author_variant	r g rg p m pm t w tw j p jp s w sw a y ay t s ts m t mt k o ko y j l yjl a h ah j s js
matchkey_str	article:00191035:2019----::eucodownsuyoriaeaaskuiihlutaknadnhrswtd
hierarchy_sort_str	2019
bklnumber	39.50
publishDate	2019
allfields	10.1016/j.icarus.2019.113418 doi (DE-627)ELV003277844 (ELSEVIER)S0019-1035(19)30277-5 DE-627 ger DE-627 rda eng 520 530 DE-600 39.50 bkl Gonçalves, Ruben verfasserin aut Venus' cloud top wind study: Coordinated Akatsuki/UVI with cloud tracking and TNG/HARPS-N with Doppler velocimetry observations 2019 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We present new wind velocities and its variability at Venus cloud-tops (≈70 km) based on coordinated observations with two complementary techniques: (1) space-based cloud-tracking using JAXA's Akatsuki/UVI imaging and (2) ground-based Doppler velocimetry using the TNG/HARPS-N (Telescopio Nazionale Galileo). This was the first use of HARPS-N to observe a Solar system planetary atmosphere. The measurement of both zonal and meridional wind velocities and the constraints of temporal and spatial wind variability at cloud top is essential to our understanding of the mechanisms which yield and maintain the dynamics of Venus' atmospheric superrotational circulation. Venus Atmosphere Dynamics Akatsuki Spectroscopy Cloud tracking Doppler velocimetry Machado, Pedro verfasserin aut Widemann, Thomas verfasserin aut Peralta, Javier verfasserin aut Watanabe, Shigeto verfasserin aut Yamazaki, Atsushi verfasserin aut Satoh, Takehiko verfasserin aut Takagi, Masahiro verfasserin aut Ogohara, Kazunori verfasserin aut Lee, Yeon-Joo verfasserin aut Harutyunyan, Avet verfasserin aut Silva, José verfasserin aut Enthalten in Icarus Orlando, Fla. : Academ. Press, 1962 335 Online-Ressource (DE-627)266881521 (DE-600)1467991-7 (DE-576)104193743 0019-1035 nnns volume:335 GBV_USEFLAG_U SYSFLAG_U GBV_ELV SSG-OPC-AST GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 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_150 GBV_ILN_151 GBV_ILN_224 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2336 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4313 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4393 39.50 Sonnensystem: Allgemeines AR 335
spelling	10.1016/j.icarus.2019.113418 doi (DE-627)ELV003277844 (ELSEVIER)S0019-1035(19)30277-5 DE-627 ger DE-627 rda eng 520 530 DE-600 39.50 bkl Gonçalves, Ruben verfasserin aut Venus' cloud top wind study: Coordinated Akatsuki/UVI with cloud tracking and TNG/HARPS-N with Doppler velocimetry observations 2019 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We present new wind velocities and its variability at Venus cloud-tops (≈70 km) based on coordinated observations with two complementary techniques: (1) space-based cloud-tracking using JAXA's Akatsuki/UVI imaging and (2) ground-based Doppler velocimetry using the TNG/HARPS-N (Telescopio Nazionale Galileo). This was the first use of HARPS-N to observe a Solar system planetary atmosphere. The measurement of both zonal and meridional wind velocities and the constraints of temporal and spatial wind variability at cloud top is essential to our understanding of the mechanisms which yield and maintain the dynamics of Venus' atmospheric superrotational circulation. Venus Atmosphere Dynamics Akatsuki Spectroscopy Cloud tracking Doppler velocimetry Machado, Pedro verfasserin aut Widemann, Thomas verfasserin aut Peralta, Javier verfasserin aut Watanabe, Shigeto verfasserin aut Yamazaki, Atsushi verfasserin aut Satoh, Takehiko verfasserin aut Takagi, Masahiro verfasserin aut Ogohara, Kazunori verfasserin aut Lee, Yeon-Joo verfasserin aut Harutyunyan, Avet verfasserin aut Silva, José verfasserin aut Enthalten in Icarus Orlando, Fla. : Academ. Press, 1962 335 Online-Ressource (DE-627)266881521 (DE-600)1467991-7 (DE-576)104193743 0019-1035 nnns volume:335 GBV_USEFLAG_U SYSFLAG_U GBV_ELV SSG-OPC-AST GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 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_150 GBV_ILN_151 GBV_ILN_224 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2336 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4313 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4393 39.50 Sonnensystem: Allgemeines AR 335
allfields_unstemmed	10.1016/j.icarus.2019.113418 doi (DE-627)ELV003277844 (ELSEVIER)S0019-1035(19)30277-5 DE-627 ger DE-627 rda eng 520 530 DE-600 39.50 bkl Gonçalves, Ruben verfasserin aut Venus' cloud top wind study: Coordinated Akatsuki/UVI with cloud tracking and TNG/HARPS-N with Doppler velocimetry observations 2019 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We present new wind velocities and its variability at Venus cloud-tops (≈70 km) based on coordinated observations with two complementary techniques: (1) space-based cloud-tracking using JAXA's Akatsuki/UVI imaging and (2) ground-based Doppler velocimetry using the TNG/HARPS-N (Telescopio Nazionale Galileo). This was the first use of HARPS-N to observe a Solar system planetary atmosphere. The measurement of both zonal and meridional wind velocities and the constraints of temporal and spatial wind variability at cloud top is essential to our understanding of the mechanisms which yield and maintain the dynamics of Venus' atmospheric superrotational circulation. Venus Atmosphere Dynamics Akatsuki Spectroscopy Cloud tracking Doppler velocimetry Machado, Pedro verfasserin aut Widemann, Thomas verfasserin aut Peralta, Javier verfasserin aut Watanabe, Shigeto verfasserin aut Yamazaki, Atsushi verfasserin aut Satoh, Takehiko verfasserin aut Takagi, Masahiro verfasserin aut Ogohara, Kazunori verfasserin aut Lee, Yeon-Joo verfasserin aut Harutyunyan, Avet verfasserin aut Silva, José verfasserin aut Enthalten in Icarus Orlando, Fla. : Academ. Press, 1962 335 Online-Ressource (DE-627)266881521 (DE-600)1467991-7 (DE-576)104193743 0019-1035 nnns volume:335 GBV_USEFLAG_U SYSFLAG_U GBV_ELV SSG-OPC-AST GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 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_150 GBV_ILN_151 GBV_ILN_224 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2336 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4313 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4393 39.50 Sonnensystem: Allgemeines AR 335
allfieldsGer	10.1016/j.icarus.2019.113418 doi (DE-627)ELV003277844 (ELSEVIER)S0019-1035(19)30277-5 DE-627 ger DE-627 rda eng 520 530 DE-600 39.50 bkl Gonçalves, Ruben verfasserin aut Venus' cloud top wind study: Coordinated Akatsuki/UVI with cloud tracking and TNG/HARPS-N with Doppler velocimetry observations 2019 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We present new wind velocities and its variability at Venus cloud-tops (≈70 km) based on coordinated observations with two complementary techniques: (1) space-based cloud-tracking using JAXA's Akatsuki/UVI imaging and (2) ground-based Doppler velocimetry using the TNG/HARPS-N (Telescopio Nazionale Galileo). This was the first use of HARPS-N to observe a Solar system planetary atmosphere. The measurement of both zonal and meridional wind velocities and the constraints of temporal and spatial wind variability at cloud top is essential to our understanding of the mechanisms which yield and maintain the dynamics of Venus' atmospheric superrotational circulation. Venus Atmosphere Dynamics Akatsuki Spectroscopy Cloud tracking Doppler velocimetry Machado, Pedro verfasserin aut Widemann, Thomas verfasserin aut Peralta, Javier verfasserin aut Watanabe, Shigeto verfasserin aut Yamazaki, Atsushi verfasserin aut Satoh, Takehiko verfasserin aut Takagi, Masahiro verfasserin aut Ogohara, Kazunori verfasserin aut Lee, Yeon-Joo verfasserin aut Harutyunyan, Avet verfasserin aut Silva, José verfasserin aut Enthalten in Icarus Orlando, Fla. : Academ. Press, 1962 335 Online-Ressource (DE-627)266881521 (DE-600)1467991-7 (DE-576)104193743 0019-1035 nnns volume:335 GBV_USEFLAG_U SYSFLAG_U GBV_ELV SSG-OPC-AST GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 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_150 GBV_ILN_151 GBV_ILN_224 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2336 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4313 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4393 39.50 Sonnensystem: Allgemeines AR 335
allfieldsSound	10.1016/j.icarus.2019.113418 doi (DE-627)ELV003277844 (ELSEVIER)S0019-1035(19)30277-5 DE-627 ger DE-627 rda eng 520 530 DE-600 39.50 bkl Gonçalves, Ruben verfasserin aut Venus' cloud top wind study: Coordinated Akatsuki/UVI with cloud tracking and TNG/HARPS-N with Doppler velocimetry observations 2019 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We present new wind velocities and its variability at Venus cloud-tops (≈70 km) based on coordinated observations with two complementary techniques: (1) space-based cloud-tracking using JAXA's Akatsuki/UVI imaging and (2) ground-based Doppler velocimetry using the TNG/HARPS-N (Telescopio Nazionale Galileo). This was the first use of HARPS-N to observe a Solar system planetary atmosphere. The measurement of both zonal and meridional wind velocities and the constraints of temporal and spatial wind variability at cloud top is essential to our understanding of the mechanisms which yield and maintain the dynamics of Venus' atmospheric superrotational circulation. Venus Atmosphere Dynamics Akatsuki Spectroscopy Cloud tracking Doppler velocimetry Machado, Pedro verfasserin aut Widemann, Thomas verfasserin aut Peralta, Javier verfasserin aut Watanabe, Shigeto verfasserin aut Yamazaki, Atsushi verfasserin aut Satoh, Takehiko verfasserin aut Takagi, Masahiro verfasserin aut Ogohara, Kazunori verfasserin aut Lee, Yeon-Joo verfasserin aut Harutyunyan, Avet verfasserin aut Silva, José verfasserin aut Enthalten in Icarus Orlando, Fla. : Academ. Press, 1962 335 Online-Ressource (DE-627)266881521 (DE-600)1467991-7 (DE-576)104193743 0019-1035 nnns volume:335 GBV_USEFLAG_U SYSFLAG_U GBV_ELV SSG-OPC-AST GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 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_150 GBV_ILN_151 GBV_ILN_224 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2336 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4313 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4393 39.50 Sonnensystem: Allgemeines AR 335
language	English
source	Enthalten in Icarus 335 volume:335
sourceStr	Enthalten in Icarus 335 volume:335
format_phy_str_mv	Article
bklname	Sonnensystem: Allgemeines
institution	findex.gbv.de
topic_facet	Venus Atmosphere Dynamics Akatsuki Spectroscopy Cloud tracking Doppler velocimetry
dewey-raw	520
isfreeaccess_bool	false
container_title	Icarus
authorswithroles_txt_mv	Gonçalves, Ruben @@aut@@ Machado, Pedro @@aut@@ Widemann, Thomas @@aut@@ Peralta, Javier @@aut@@ Watanabe, Shigeto @@aut@@ Yamazaki, Atsushi @@aut@@ Satoh, Takehiko @@aut@@ Takagi, Masahiro @@aut@@ Ogohara, Kazunori @@aut@@ Lee, Yeon-Joo @@aut@@ Harutyunyan, Avet @@aut@@ Silva, José @@aut@@
publishDateDaySort_date	2019-01-01T00:00:00Z
hierarchy_top_id	266881521
dewey-sort	3520
id	ELV003277844
language_de	englisch
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author	Gonçalves, Ruben
spellingShingle	Gonçalves, Ruben ddc 520 bkl 39.50 misc Venus misc Atmosphere misc Dynamics misc Akatsuki misc Spectroscopy misc Cloud tracking misc Doppler velocimetry Venus' cloud top wind study: Coordinated Akatsuki/UVI with cloud tracking and TNG/HARPS-N with Doppler velocimetry observations
authorStr	Gonçalves, Ruben
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topic_title	520 530 DE-600 39.50 bkl Venus' cloud top wind study: Coordinated Akatsuki/UVI with cloud tracking and TNG/HARPS-N with Doppler velocimetry observations Venus Atmosphere Dynamics Akatsuki Spectroscopy Cloud tracking Doppler velocimetry
topic	ddc 520 bkl 39.50 misc Venus misc Atmosphere misc Dynamics misc Akatsuki misc Spectroscopy misc Cloud tracking misc Doppler velocimetry
topic_unstemmed	ddc 520 bkl 39.50 misc Venus misc Atmosphere misc Dynamics misc Akatsuki misc Spectroscopy misc Cloud tracking misc Doppler velocimetry
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title	Venus' cloud top wind study: Coordinated Akatsuki/UVI with cloud tracking and TNG/HARPS-N with Doppler velocimetry observations
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title_full	Venus' cloud top wind study: Coordinated Akatsuki/UVI with cloud tracking and TNG/HARPS-N with Doppler velocimetry observations
author_sort	Gonçalves, Ruben
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author_browse	Gonçalves, Ruben Machado, Pedro Widemann, Thomas Peralta, Javier Watanabe, Shigeto Yamazaki, Atsushi Satoh, Takehiko Takagi, Masahiro Ogohara, Kazunori Lee, Yeon-Joo Harutyunyan, Avet Silva, José
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author-letter	Gonçalves, Ruben
doi_str_mv	10.1016/j.icarus.2019.113418
dewey-full	520 530
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title_sort	venus' cloud top wind study: coordinated akatsuki/uvi with cloud tracking and tng/harps-n with doppler velocimetry observations
title_auth	Venus' cloud top wind study: Coordinated Akatsuki/UVI with cloud tracking and TNG/HARPS-N with Doppler velocimetry observations
abstract	We present new wind velocities and its variability at Venus cloud-tops (≈70 km) based on coordinated observations with two complementary techniques: (1) space-based cloud-tracking using JAXA's Akatsuki/UVI imaging and (2) ground-based Doppler velocimetry using the TNG/HARPS-N (Telescopio Nazionale Galileo). This was the first use of HARPS-N to observe a Solar system planetary atmosphere. The measurement of both zonal and meridional wind velocities and the constraints of temporal and spatial wind variability at cloud top is essential to our understanding of the mechanisms which yield and maintain the dynamics of Venus' atmospheric superrotational circulation.
abstractGer	We present new wind velocities and its variability at Venus cloud-tops (≈70 km) based on coordinated observations with two complementary techniques: (1) space-based cloud-tracking using JAXA's Akatsuki/UVI imaging and (2) ground-based Doppler velocimetry using the TNG/HARPS-N (Telescopio Nazionale Galileo). This was the first use of HARPS-N to observe a Solar system planetary atmosphere. The measurement of both zonal and meridional wind velocities and the constraints of temporal and spatial wind variability at cloud top is essential to our understanding of the mechanisms which yield and maintain the dynamics of Venus' atmospheric superrotational circulation.
abstract_unstemmed	We present new wind velocities and its variability at Venus cloud-tops (≈70 km) based on coordinated observations with two complementary techniques: (1) space-based cloud-tracking using JAXA's Akatsuki/UVI imaging and (2) ground-based Doppler velocimetry using the TNG/HARPS-N (Telescopio Nazionale Galileo). This was the first use of HARPS-N to observe a Solar system planetary atmosphere. The measurement of both zonal and meridional wind velocities and the constraints of temporal and spatial wind variability at cloud top is essential to our understanding of the mechanisms which yield and maintain the dynamics of Venus' atmospheric superrotational circulation.
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title_short	Venus' cloud top wind study: Coordinated Akatsuki/UVI with cloud tracking and TNG/HARPS-N with Doppler velocimetry observations
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author2	Machado, Pedro Widemann, Thomas Peralta, Javier Watanabe, Shigeto Yamazaki, Atsushi Satoh, Takehiko Takagi, Masahiro Ogohara, Kazunori Lee, Yeon-Joo Harutyunyan, Avet Silva, José
author2Str	Machado, Pedro Widemann, Thomas Peralta, Javier Watanabe, Shigeto Yamazaki, Atsushi Satoh, Takehiko Takagi, Masahiro Ogohara, Kazunori Lee, Yeon-Joo Harutyunyan, Avet Silva, José
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doi_str	10.1016/j.icarus.2019.113418
up_date	2024-07-06T19:05:22.524Z
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Venus' cloud top wind study: Coordinated Akatsuki/UVI with cloud tracking and TNG/HARPS-N with Doppler velocimetry observations

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