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.

Shalbatana Vallis Perched Remnant Fan Deposits:   ESP_093089_1805   ESP_092944_1805   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
0.551

314.

26.2

15.59

41.5

44.1

Bedding in Hellas Planitia:   ESP_092954_1400   ESP_093033_1400   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-39.8

49.5

-13.

15.98

39.3

36.9

Seasonal Monitoring near Dorsa Argentea:   ESP_092838_1005   ESP_093036_1005   (Interval in Earth days: 15)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-79.3

345.

11.8

-3.15

59.0

61.0

Features around Crater near Hellas Planitia:   ESP_092807_1375   ESP_092596_1375   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-42.1

102.

1.17

19.52

39.6

39.7

Dune Field:   ESP_093057_1040   ESP_093426_1040   (Interval in Earth days: 29)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-75.7

125.

3.99

22.48

58.1

60.6

Candidate Tianwen-3 Landing Region:   ESP_092701_2070   ESP_092912_2070   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
26.64

107.

5.00

-11.5

64.8

63.5

Pie-Like Feature near Amenthes Cavi:   ESP_092740_1915   ESP_093386_1915   (Interval in Earth days: 51)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
11.45

125.

-1.4

26.34

54.2

44.5

Southeast Aeolis Dorsa Inverted Delta Trunk Channel:   ESP_093095_1735   ESP_093240_1735   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.31

153.

-0.0

16.51

39.9

37.3

South Polar Residual Cap Stereo Campaign:   ESP_093055_0910   ESP_093014_0910   (Interval in Earth days: 3)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-89.2

253.

23.5

26.98

67.5

66.6

Kasei Valles Flood Grooves and Pedestal Crater:   ESP_092892_2035   ESP_092958_2035   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
23.01

293.

-3.1

-24.3

60.5

61.1


  


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