MozartV1, PascalFrancis, Curation, bibRecord, 000057

Radar imagery of the southern Caloris region, Mercury

Identifieur interne : 000057 ( PascalFrancis/Curation ); précédent : 000056; suivant : 000058

Radar imagery of the southern Caloris region, Mercury

Auteurs : John K. Harmon [Porto Rico]

Source :

Icarus : (New York, NY) [ 0019-1035 ] ; 2008.

RBID : Pascal:08-0324895

Descripteurs français

Pascal (Inist)
- Imagerie radar, Diamètre, Observation radar, Système solaire.

English descriptors

KwdEn :
- Diameter, Radar imaging, Radar observation, Solar system.

Abstract

Radar imagery from July 2005 Arecibo observations has provided new information on surface relief over the southern portion of Caloris Basin and the smooth plains to the south of the basin. A lobe of smooth plains has been identified in the Mariner-unimaged region southwest of Mozart Crater that coincides precisely with topographically down-bowed terrain seen in earlier Arecibo radar altimetry. A 105-km-diameter crater has been found at 193.6° W, 25.6° N that appears to be the largest crater in the Caloris basin floor.

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A06				`@2 1`
A08	`01`	`1`	`ENG`	`@1 Radar imagery of the southern Caloris region, Mercury`
A11	`01`	`1`		`@1 HARMON (John K.)`
A14	`01`			`@1 National Astronomy and Ionosphere Center, Arecibo Observatory, HC3 Box 53995 @2 Arecibo, 00612 @3 PRI @Z 1 aut.`
A20				`@1 298-301`
A21				`@1 2008`
A23	`01`			`@0 ENG`
A43	`01`			`@1 INIST @2 10196 @5 354000197893210240`
A44				`@0 0000 @1 © 2008 INIST-CNRS. All rights reserved.`
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C01	`01`		`ENG`	@0 Radar imagery from July 2005 Arecibo observations has provided new information on surface relief over the southern portion of Caloris Basin and the smooth plains to the south of the basin. A lobe of smooth plains has been identified in the Mariner-unimaged region southwest of Mozart Crater that coincides precisely with topographically down-bowed terrain seen in earlier Arecibo radar altimetry. A 105-km-diameter crater has been found at 193.6° W, 25.6° N that appears to be the largest crater in the Caloris basin floor.
C02	`01`	`3`		`@0 001E03B`
C03	`01`	`3`	`FRE`	`@0 Imagerie radar @5 26`
C03	`01`	`3`	`ENG`	`@0 Radar imaging @5 26`
C03	`02`	`X`	`FRE`	`@0 Diamètre @5 27`
C03	`02`	`X`	`ENG`	`@0 Diameter @5 27`
C03	`02`	`X`	`SPA`	`@0 Diámetro @5 27`
C03	`03`	`X`	`FRE`	`@0 Observation radar @5 28`
C03	`03`	`X`	`ENG`	`@0 Radar observation @5 28`
C03	`03`	`X`	`SPA`	`@0 Observación radar @5 28`
C03	`04`	`3`	`FRE`	`@0 Système solaire @5 29`
C03	`04`	`3`	`ENG`	`@0 Solar system @5 29`
N21				`@1 203`
N44	`01`			`@1 OTO`
N82				`@1 OTO`

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Pascal:08-0324895

Le document en format XML

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<front><div type="abstract" xml:lang="en">Radar imagery from July 2005 Arecibo observations has provided new information on surface relief over the southern portion of Caloris Basin and the smooth plains to the south of the basin. A lobe of smooth plains has been identified in the Mariner-unimaged region southwest of Mozart Crater that coincides precisely with topographically down-bowed terrain seen in earlier Arecibo radar altimetry. A 105-km-diameter crater has been found at 193.6° W, 25.6° N that appears to be the largest crater in the Caloris basin floor.</div>
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Radar imagery of the southern Caloris region, Mercury

Radar imagery of the southern Caloris region, Mercury

Source :

Descripteurs français

English descriptors

Abstract

Links toward previous steps (curation, corpus...)

Links to Exploration step

Le document en format XML

Pour manipuler ce document sous Unix (Dilib)

Pour mettre un lien sur cette page dans le réseau Wicri