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| | [39.03] Nightside Venus Atmospheric Circulation from Nordic Optical Telescope Observations |
 | | Near infrared observations of Venus' nightside hemisphere were acquired from the 2.6-m Nordic Optical Telescope at the Roque de Los Muchachos Observatory located on La Palma, Canary Islands, Spain during May (117 - 126 degrees phase angle) and August 2004 (86 - 80 degrees phase angle). |
 | | Other participating observatories include, the 2-m Himalayan Chandra Telescope at Mt. Saraswati, Hanle, Indian Astronomical Observatory, the 1.2-m Mt Abu Telescope of the Physical Research Observatory, the Sacramento Peak Observatory, National Solar Observatory, New Mexico, USA, and the 3.6-m NASA Infrared Telescope Facility, Mauna Kea, Hawaii, USA. |
 | | The observations, mainly in the 2.1 micron K-band, were aquired to allow a study of the atmospheric circulation pattern and and cloud evolution, partly to support the European Space Agency's Venus Express mission. |
| www.aas.org /publications/baas/v36n4/dps2004/213.htm (294 words) |
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