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.

High-Latitude Exposure of North Polar Layered Deposits:   ESP_019117_2720   ESP_019050_2720   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
87.74

6.00

-13.

-23.1

73.5

73.7

Layered Terrain in Aeolis Planum:   ESP_018959_1730   ESP_019025_1730   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.90

150.

4.52

-18.8

57.2

58.8

Steep North Polar Boundary Scarp:   ESP_018943_2655   ESP_019181_2655   (Interval in Earth days: 19)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
85.36

186.

0

-13.2

67.0

70.6

Small Cone in Hydraotes Chaos:   ESP_019124_1805   ESP_019269_1805   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
0.248

326.

-4.3

11.07

54.5

53.4

Well-Preserved Impact Crater in Arabia Terra:   ESP_019162_1975   ESP_019439_1975   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.23

5.48

7.48

-19.6

48.9

52.7

Central Structure of Jorn Crater:   ESP_019186_1525   ESP_025199_1525   (Interval in Earth days: 469)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.1

76.4

0

-29.5

67.8

62.4

Syrtis Major Planum Channel and Depression:   ESP_018988_1980   ESP_042882_1980   (Interval in Earth days: 1861)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.54

76.5

0

-26.9

48.6

42.2

North Polar Layers:   ESP_019188_2595   ESP_027904_2595   (Interval in Earth days: 679)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
79.25

0.75

-4.4

7.699

66.5

64.2

Steep North-Polar Boundary Scarp:   ESP_018957_2655   ESP_019195_2655   (Interval in Earth days: 19)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
85.25

160.

3.29

-9.91

67.0

70.5

Thermally-Distinct Material at Distal Coogoon Valles:   ESP_019084_1980   ESP_060437_1980   (Interval in Earth days: 3222)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.85

336.

-5.5

5.547

49.5

37.7


  


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