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.

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

Gullies and Lobate Material in a Crater in the Nereidum Montes:   ESP_014127_1420   ESP_020786_1420   (Interval in Earth days: 519)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-37.5

314.

-2.1

19.93

37.6

54.3

Pit Crater:   ESP_013167_1785   ESP_013589_1785   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.32

239.

-7.4

-22.9

49.4

45.4

Phyllosilicate and Possible Chlorite Prehnite Northwest of Hellas Region:   ESP_012765_1535   ESP_013477_1535   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-26.2

56.4

7.51

22.87

45.6

35.6

Northwest Wall of Juventae Chasma:   ESP_013244_1760   ESP_030228_1760   (Interval in Earth days: 1323)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.14

296.

0

10.99

46.6

50.0

Very Fresh 3 Kilometer Diameter Impact Crater:   ESP_013159_1675   ESP_032121_1675   (Interval in Earth days: 1478)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-12.3

98.9

-2.3

-26.9

44.4

34.3

Basal Exposure of South Polar Layered Deposits:   ESP_013145_1070   ESP_013277_1070   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-73.0

133.

0.46

-14.5

55.6

56.1

Well-Preserved 8 Kilometer Diameter Crater:   ESP_013650_1230   ESP_013927_1230   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-56.4

20.2

1.13

-19.3

45.0

47.6

Gullies Observed by MOC:   ESP_012707_1445   ESP_013208_1445   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-35.4

201.

2.07

23.84

46.6

38.4

Well Preserved 20 Kilometer Diameter Impact Crater:   ESP_013684_1455   ESP_020910_1455   (Interval in Earth days: 563)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-34.0

168.

-2.8

19.71

36.4

51.7


  


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