Global View of Venus

Venus

金星

This global view of the surface of Venus is centered at 0 degrees east longitude. Magellan synthetic aperture radar mosaics from the first cycle of Magellan mapping are mapped onto a computer- simulated globe to create this image. Data gaps are filled with Pioneer-Venus Orbiter data, or a constant mid-range value. Simulated color is used to enhance small-scale structure. The simulated hues are based on color images recorded by the Soviet Venera 13 and 14 spacecraft. The image was produced by the Solar System Visualization project and the Magellan Science team at the JPL Multimission Image Processing Laboratory, and was released on October 29, 1991.

这张关于金星表面的全球视图以0度东经为中心。Magellan合成孔径雷达拼接图像基于Magellan测绘第一轮数据，映射到计算机模拟的球体上生成。数据缺口用先锋-金星轨道器数据或一个中等范围的常数值填补。模拟的颜色用于增强小尺度结构。模拟的颜色基于苏联维纳拉13和14号飞船记录的彩色图像。这张图像由太阳系可视化项目和Magellan科学团队在JPL多任务图像处理实验室制作，并于1991年10月29日发布。

NASA提供的Magellan探测器图像。

Venus

金星

Constructed from NASA image using Pioneer-Venus data.

This is a radar map of Venus based on data from Pioneer-Venus Orbiter data. The false colors indicate altitude with red being the highest altitude, yellow and green representing successively lower altitudes, and the blue represents lowland plains. Some of the prominent geographic features are labled. Two major highland areas Ishtar Terra and Aphrodite Terra are like continents, with the regions labled "Regia" being smaller highland areas. Much of the surface is in the "Planitia" or plains regions.

这张雷达图是基于先驱-金星轨道器的数据制作的。假彩色表示高度，红色表示最高处，黄色和绿色表示依次较低的高度，蓝色表示低平原地区。一些显著的地理特征已标注。两个主要的高地区域Ishtar Terra和Aphrodite Terra类似于大陆，其中标注为“Regia”的区域是较小的高地区域。表面的大部分区域属于“Planitia”或平原区域。

利用先驱-金星数据构建的NASA图像