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 Stratified Materials in Hebes Chasma:   ESP_030479_1785   ESP_039446_1785   (Interval in Earth days: 699)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.29

283.

13.6

22.69

49.2

49.2

Possible Future Landing Site in Mawrth Vallis:   ESP_030490_2000   ESP_021866_2000   (Interval in Earth days: 672)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
19.99

342.

-8.0

3.916

62.6

60.8

Layered Deposits in Crater:   ESP_030356_1475   ESP_066171_1470   (Interval in Earth days: 2791)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-32.2

47.2

-5.9

7.542

44.8

41.1

Crater with Moat:   ESP_030483_1830   ESP_030905_1830   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.777

175.

-6.0

-23.6

52.5

49.7

Possible Future Landing Site in Mawrth Vallis:   ESP_030200_2060   ESP_030622_2060   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
25.48

339.

-6.0

-20.5

66.5

66.5

Monitor Seasonal Changes at South Polar Site:   ESP_030501_0980   ESP_030554_0980   (Interval in Earth days: 4)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-81.6

66.2

4.66

-8.45

62.2

62.8

Bedform Changes Southwest of Schiaparelli Crater:   ESP_030555_1735   ESP_030489_1735   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.37

11.8

-18.

4.51

48.5

47.5

Streamlined Forms in Elysium Planitia:   ESP_030312_1955   ESP_031169_1955   (Interval in Earth days: 67)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
15.42

161.

0.70

22.58

59.9

52.0

Light-Toned Stratified Material of Northeast Meridiani Planum:   ESP_030331_1815   ESP_030476_1815   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
1.333

4.59

4.80

18.55

52.1

50.1

Central Uplift of Saheki Crater:   ESP_030355_1580   ESP_030856_1580   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-21.6

73.1

-6.6

13.11

45.4

37.8


  


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