Stereo Pairs 
An explanation of stereo pairs and their use (PDF)  

Planned stereo pairs have suitable stereo convergence angles and illumination by design. In addition to planned stereo pairs, the Pairendipity software can identify overlapping HiRISE images that are serendipitously suitable for stereo processing and find stereo pairs within the CTX dataset.

Planned HiRISE stereo pairs are listed in the “Stereo Pair List (CSV)” link below. Since this list is based on produced stereo anaglyphs it also contains a few serendipitous pairs that underwent special processing. Most serendipitous HiRISE stereo pairs are listed in the “Pairendipity Stereo” link, while CTX stereo pairs are listed in “Pairendipity CTX Stereo”.

Images taken close together in time minimize illumination and frost differences and are especially useful (see the Delta-Days column in the Pairendipity files or difference the orbit numbers in the image IDs in the Stereo Pair List file). Stereo pairs with both images planned within the same 14-day (168-orbit) operations cycle are known as SPORCs.

Well-Preserved Crater South of Hypanis Valles:   ESP_039379_1890   ESP_056930_1890   (Interval in Earth days: 1368)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.936

313.

-2.4

22.35

56.9

52.3

Candidate Landing Site for 2020 Mission in Firsoff Crater:   ESP_039404_1820   ESP_047184_1820   (Interval in Earth days: 607)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.148

350.

8.81

-2.08

52.3

52.6

Monitor Defrosting Patterns on Ridges in Region Dubbed Inca City:   ESP_039473_0985   ESP_039776_0985   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-81.4

296.

-7.5

8.443

62.2

60.3

Asimov Crater Gullies Present in MOC R1000011:   ESP_039206_1320   ESP_039694_1320   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-47.5

4.78

-5.6

-27.9

48.6

44.7

Pits in Hale Crater Ejecta:   ESP_039524_1445   ESP_039801_1445   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-35.0

320.

-2.4

-19.2

42.0

40.3

A Triple-Crater in Elysium Planitia:   ESP_039147_1940   ESP_039292_1940   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
13.78

167.

-3.4

8.285

61.2

59.7

Strange Flow: Landslide, Impact Melt or Lava?:   ESP_039117_1745   ESP_039539_1745   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.45

267.

14.2

-4.61

51.1

48.1

Well-Preserved 30-Kilometer Impact Crater:   ESP_039176_1615   ESP_039387_1615   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-18.5

98.5

6.16

-4.52

47.3

45.5

Osuga Valles Lowest Point:   ESP_039181_1650   ESP_039326_1650   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.7

322.

-5.4

7.662

49.0

46.3

Well-Preserved Impact Crater on Floor of Coprates Chasma:   ESP_039182_1675   ESP_048465_1675   (Interval in Earth days: 723)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-12.3

294.

-4.8

7.502

49.6

39.1


  


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