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 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

Crater between Branches of Athabasca Valles:   ESP_013460_1900   ESP_013737_1900   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.648

157.

4.42

-23.9

51.5

50.0

Central Structure of Verlaine Crater:   ESP_013213_1705   ESP_013635_1705   (Interval in Earth days: 32)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-9.25

64.1

-1.2

-15.7

44.8

40.8

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

Hale Crater Impact Ejecta:   ESP_012808_1420   ESP_013665_1420   (Interval in Earth days: 67)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-37.6

324.

0

27.24

45.6

34.9

Columbus Crater Wall with Possible Kaolinite Exposure:   ESP_013327_1510   ESP_013960_1510   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-28.8

193.

8.88

-14.5

38.1

35.7

Mantled Deposits in Reull Vallis:   ESP_014148_1365   ESP_014438_1365   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-43.3

101.

-3.5

22.39

40.7

41.8

Light-Toned Outcrop in Hummock of Iani Chaos:   ESP_013717_1790   ESP_013862_1790   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.05

342.

5.13

18.19

42.1

39.5

Diverse Layers and Morphologies in North Rim of Hellas Planitia:   ESP_013490_1525   ESP_058166_1530   (Interval in Earth days: 3481)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.3

64.2

-5.3

5.215

37.6

30.5

Light-Toned Materials Eroding from Ponded Materials in Kontum Crater:   ESP_012730_1475   ESP_020866_1475   (Interval in Earth days: 634)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-32.1

292.

5.03

-17.8

46.0

54.9


  


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