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.

Light-Toned Fan-Like Features in Crater in Chryse Chaos:   ESP_013256_1885   ESP_022104_1885   (Interval in Earth days: 689)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.534

327.

-1.4

-13.8

53.6

52.2

Warrego Valles Headwater Region:   ESP_013153_1390   ESP_013298_1390   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-40.6

266.

-5.4

6.316

42.0

39.7

Gullies in Green Crater:   ESP_014007_1270   ESP_014297_1270   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-52.6

352.

3.08

23.96

44.4

45.9

Exposed Strata Near Melas Region Wall:   ESP_013719_1665   ESP_021789_1665   (Interval in Earth days: 629)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.2

289.

2.48

-8.89

37.2

44.6

Chain of Cones and Craters in Isidis Planitia:   ESP_013054_1900   ESP_013199_1900   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.766

83.1

-5.1

9.582

56.5

54.2

Pits in Hydrae Chasma:   ESP_013033_1730   ESP_013745_1730   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.83

297.

0

14.87

47.8

38.4

Gullies in Light-Toned Rock:   ESP_012795_1395   ESP_013507_1395   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-40.2

319.

2.74

16.59

45.9

37.2

Incipient Scalloped Terrain in Mid-Latitude Mantle at Peneus Patera:   ESP_013029_1235   ESP_013306_1235   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-56.1

54.6

-0.3

-19.2

47.7

46.9

Ejecta Flow from Bacolor Crater:   ESP_014147_2135   ESP_022494_2135   (Interval in Earth days: 651)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
33.32

118.

-1.3

-27.5

59.9

66.5

Exposure of Layers in South Gale Crater with Possible Sulfates:   ESP_014186_1745   ESP_020410_1745   (Interval in Earth days: 485)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.56

138.

8.10

-13.1

35.2

55.9


  


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