A new VLT surface map of Titan at 1.575 microns

Astronomy and Astrophysics

Volumn 421, Issue 1, 2004, Pages

  Hartung, M ^a   Herbst, T M ^b   Close, L M ^c   Lenzen, R ^b   Brandner, W ^b   Marco, O ^a   Lidman, C ^a  

^a EUROPEAN SOUTHERN OBSERVATORY   (Chile)

^b MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

^c UNIVERSITY OF ARIZONA   (United States)

Author keywords

Infrared: solar system; Instrumentation: adaptive optics; Planets and satellites: individual: Titan

Indexed keywords

ADAPTIVE OPTICS; EXTRATERRESTRIAL ATMOSPHERES; IMAGE ANALYSIS; METHANE; NITROGEN; SAMPLING; SATELLITES; SURFACE PHENOMENA; UPPER ATMOSPHERE;

INFRARED: SOLAR SYSTEM; INSTRUMENTATION: ADAPTIVE OPTICS; PLANETS AND SATELLITES:INDIVIDUAL:TITAN; SPECKLE NOISE;

PLANETS;

EID: 3042621446     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20040171     Document Type: Article

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