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The measurement of the length of the shadow depends on the height of the obstacle and the elevation of the sun, the formula is: The length of the shadow map is normalized (changing with the zoom), and the direction is opposite azimuth. The first column contain the date the others columns contain E=elevation A=azimuth and time (from 00:00 to 23:59).įor the annual SunRise SunSet Calendar additionally on excel file you’ll be able to use this link: Sunrise Sunset Calendar The excel file contain the sun path for one year, with step (5,10,15,20,30,60 min), for the moment restricted as a result of is just too heavy for the server. Set the data as you wish and click on email image to get the file in attach.
GREEN SKY CALCULATOR MOBILE PDF
Features on Jupiter appear closer to the central meridian than to the limb - and thus are well placed for viewing - for 50 minutes before and after their transit times.| Data + Map | Chart Polar | Chart Cartesian | Table | Annual sun path | shadow | download PDF | If the GRS moves elsewhere, it will transit 1 2⁄ 3 minutes late for every 1° of longitude greater than that used in this tool or 1 2⁄ 3 minutes early for every 1° less than the longitude in this tool. These predictions assume the Red Spot was at Jovian System II longitude 8° in November 2021 and continues to drift 1.75° per month, based on historical trends noted by JUPOS.
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Available on the iTunes App Store for only $2.99. JupiterMoons is your essential guide to observing Jupiter whenever the king of planets reigns the night sky, showing you the locations of Io, Europa, Ganymede, Callisto, and the Great Red Spot at any date and time. If you enjoy using this utility and own an iPhone or iPad, you might be interested in our app. The listed times should be accurate to within a few minutes. Or you can enter any date this year to find other transit times. Click "Initialize to today" to view the dates and times of the next three transits of the GRS. It appears slightly more distinct when Jupiter is viewed through a light green or blue filter.īelow is a calculator you can use to predict the local and Universal Times and dates when the center of the Great Red Spot should cross Jupiter's central meridian, the imaginary line down the center of the planet's disk from pole to pole. That's a good thing, because for something so famous, it can be surprisingly difficult to see. Of course there's a lot more to look for in Jupiter's atmosphere than the GRS. However, unlike low-pressure cyclones and hurricanes on Earth, the GRS rotates in a counter-clockwise direction in Jupiter's southern hemisphere, showing that it is a high-pressure system. The Red Spot is a vast, long-lived storm, spinning like a cyclone. The spot was named around 1878 when it turned a vivid brick red, but in recent decades it has generally been a much less conspicuous pale tan. Jupiter's most famous feature is its Great Red Spot (GRS). South is up to match the view in many astronomical telescopes. The Great Red Spot always stays in the south edge of the brownish South Equatorial Belt.
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This image of Jupiter was taken by NASA's Cassini spacecraft on October 8, 2000.