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The Lumix DMC-F1 was Panasonic's first digital camera to use the Venus Engine. The Venus Engine is an image-processing engine for digital cameras. It was developed by the company Panasonic. Almost all of their Lumix cameras use a version of the Venus Engine. [1] It is based on the Panasonic MN103/MN103S. All image processors operate in four steps.
As with most Panasonic Lumix cameras it uses a Venus Engine, in this case the Venus Engine III. The camera has a 2.5" color LCD display and a color electronic viewfinder, and is available in two colors, black (suffix K) and silver (suffix S). The DMC-FZ18 became available in the United States in July 2007. The successor to the FZ18 is the FZ28.
[363] [364] In 2011, electronics company Panasonic produced the Panasonic Lumix FX77, a camera praised for its use of face-altering functions such as adding makeup onto a photographed bare face. This was commercialized in collaboration with at-the-time gyaru model Yuka Obara , presented by the American news program CBS News on their YouTube ...
Lander landed at 03:20 UTC on 21 December 1978. Both cameras on lander failed Proton-K/D-1: Pioneer Venus 1 (PV Orbiter) 20 May 1978: NASA United States: Orbiter Successful Entered orbit on 4 December 1978, decayed on 22 October 1992 Atlas SLV-3D Centaur-D1AR: Pioneer Venus 2 (PV Multiprobe) 8 August 1978: NASA United States: Atmospheric Successful
During the mapping cycle 1 (left-looking) radar surface mapping on Venus (September 15, 1990 to May 15, 1991), around 70% of the Venusian surface was mapped by synthetic aperture radar. In cycle 2 (right-looking), 54.5% of the surface was mapped, mainly the south pole regions and gaps from cycle 1 during May 15, 1991 to January 14, 1992.
the longwave infrared camera (LIR) is studying the structure of high-altitude clouds at a wavelength where they emit heat (10 μm) the infrared 1 μm camera (IR1) is imaging on the night side heat radiation (0.90–1.01 μm) emitted from Venus's surface and help researchers to spot active volcanoes, if they exist. While on the day side, it ...
As the cruise stage flew by Venus, the bus acted as a data relay for the lander before continuing on to a heliocentric orbit.The probe was equipped with a gamma-ray spectrometer, UV grating monochromator, electron and proton spectrometers, gamma-ray burst detectors, solar wind plasma detectors, and two-frequency transmitters which made measurements before, during, and after the Venus flyby.
The 1882 transit is a member of #2. The 2004 transit is a member of #3, and the 2012 transit is a member of #4. The 2117 transit is a member of #1, and so on. However, the ascending node (December transits) of the orbit of Venus moves backwards after each 243 years so the transit of 2854 is the last member of series #3 instead of series #1.