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Juno Jupiter image

Simon Calcutt

Emeritus

Sub department

  • Atmospheric, Oceanic and Planetary Physics

Research groups

  • Planetary atmosphere observation analysis
  • Solar system
  • Space instrumentation
  • Planetary surfaces
simon.calcutt@physics.ox.ac.uk
Telephone: 01865 (2)72916
Atmospheric Physics Clarendon Laboratory, room 308
  • About
  • Publications

SEARCH FOR SPATIAL VARIATIONS OF THE H2O ABUNDANCE IN THE LOWER ATMOSPHERE OF VENUS FROM NIMS-GALILEO

PLANETARY AND SPACE SCIENCE 41:7 (1993) 495-504

Authors:

P DROSSART, B BEZARD, T ENCRENAZ, E LELLOUCH, M ROOS, FW TAYLOR, AD COLLARD, SB CALCUTT, J POLLACK, DH GRINSPOON, RW CARLSON, KH BAINES, LW KAMP
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SPECTRAL PARAMETERS OF SELF-BROADENED AND HYDROGEN-BROADENED METHANE FROM 2000 CM(-1) TO 9500 CM(-1) FOR REMOTE SOUNDING OF THE ATMOSPHERE OF JUPITER

JOURNAL OF QUANTITATIVE SPECTROSCOPY & RADIATIVE TRANSFER 50:4 (1993) 363-429

Authors:

K STRONG, FW TAYLOR, SB CALCUTT, JJ REMEDIOS, J BALLARD
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TEST AND VALIDATION OF MCT DETECTORS FOR PMIRR ON THE MARS OBSERVER SPACECRAFT

NATO ADV SCI INST SE 245 (1993) 879-887

Authors:

S ASLAM, CL HEPPLEWHITE, SB CALCUTT
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THE UPPER CLOUDS OF VENUS - DETERMINATION OF THE SCALE HEIGHT FROM NIMS-GALILEO INFRARED DATA

PLANETARY AND SPACE SCIENCE 41:7 (1993) 505-&

Authors:

M ROOS, P DROSSART, T ENCRENAZ, E LELLOUCH, B BEZARD, RW CARLSON, KH BAINES, LW KAMP, FW TAYLOR, AD COLLARD, SB CALCUTT, JB POLLACK, DH GRINSPOON
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Galileo infrared imaging spectroscopy measurements at venus.

Science 253:5027 (1991) 1541-1548

Authors:

RW Carlson, KH Baines, T Encrenaz, FW Taylor, P Drossart, LW Kamp, JB Pollack, E Lellouch, AD Collard, SB Calcutt, D Grinspoon, PR Weissman, WD Smythe, AC Ocampo, GE Danielson, FP Fanale, TV Johnson, HH Kieffer, DL Matson, TB McCord, LA Soderblom

Abstract:

During the 1990 Galileo Venus flyby, the Near Infaied Mapping Spectrometer investigated the night-side atmosphere of Venus in the spectral range 0.7 to 5.2 micrometers. Multispectral images at high spatial resolution indicate substanmial cloud opacity variations in the lower cloud levels, centered at 50 kilometers altitude. Zonal and meridional winds were derived for this level and are consistent with motion of the upper branch of a Hadley cell. Northern and southern hemisphere clouds appear to be markedly different. Spectral profiles were used to derive lower atmosphere abundances of water vapor and other species.
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