File:MRO-MCS-Seasonal-Temperature-Pattern-Dust-Storms.jpg
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[edit]DescriptionMRO-MCS-Seasonal-Temperature-Pattern-Dust-Storms.jpg |
English: This graphic shows Martian atmospheric temperature data related to seasonal patterns in occurrence of large regional dust storms. The data shown here were collected by the Mars Climate Sounder instrument on NASA's Mars Reconnaissance Orbiter over the course of one-half of a Martian year, during 2012 and 2013. The color coding indicates daytime temperatures of a layer of the atmosphere centered about 16 miles (25 kilometers) above ground level, corresponding to the color-key bar at the bottom of the graphic.
Three regional dust storms indicated by increased temperatures are labeled A, B and C. A similar sequence of three large regional dust storms has been seen in atmosphere-temperature data from five other Martian years. The vertical axis is latitude on Mars, from the north pole at the top to south pole at the bottom. Each graphed data point is an average for all Martian longitudes around the planet. The horizontal axis is the time of year, spanning from the beginning of Mars' southern-hemisphere spring (on the left) to the end of southern-hemisphere summer. This is the half of the year when large Martian dust storms are most active. NASA's Jet Propulsion Laboratory, Pasadena, California, built and operates the Mars Climate Sounder, and manages the Mars Reconnaissance Orbiter mission. Lockheed Martin Space Systems, Denver, built the orbiter.Русский: Дневная температура атмосферы Марса (слоя на высоте в среднем 25 км) на разных широтах и в разное время года на основании данных инструмента Mars Climate Sounder на борту аппарата Mars Reconnaissance Orbiter, собранных в течение половины марсианского года в 2012/2013 гг. Величина температуры показана цветом от тёмно-синего до ярко-красного, вертикальная ось - широта (от -90° - южного полюса - до 90° - северного), горизонтальная - время года - от начала весны до конца лета в южном полушарии, когда наиболее интенсивно формируются пылевые бури. Три таких крупных пылевых бури обозначены буквами A, B и C - в областях с повышенной температурой. |
Date |
circa 2013 date QS:P,+2013-00-00T00:00:00Z/9,P1480,Q5727902 |
Source | https://mars.nasa.gov/resources/7851/ |
Author | NASA/JPL-Caltech |
Licensing
[edit]Public domainPublic domainfalsefalse |
This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.) | ||
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Orientation | Normal |
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Horizontal resolution | 72 dpi |
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Software used | Adobe Photoshop CS5 Windows |
File change date and time | 12:53, 3 June 2016 |
Color space | Uncalibrated |
Date and time of digitizing | 01:43, 1 June 2016 |
Date metadata was last modified | 05:53, 3 June 2016 |
Unique ID of original document | xmp.did:0B2830790728E6118EF3D11D114CF6FF |