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.

Valleys on Western Hecates Tholus:   ESP_024207_2130   ESP_024352_2130   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
32.52

149.

-0.4

16.28

43.3

41.0

Possible Mud Volcanoes Located in Acidalia Planitia:   ESP_024227_2240   ESP_024359_2240   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
43.66

318.

23.1

-2.47

48.5

48.7

Possible Mud Volcanoes in Acidalia Planitia Region:   ESP_024253_2210   ESP_024530_2210   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
40.48

332.

2.39

-15.8

47.5

46.4

Pits and Gullies:   ESP_024205_1435   ESP_031919_1435   (Interval in Earth days: 601)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-35.9

214.

-18.

-5.67

52.7

37.0

Candidate Future Landing Site North of Hellas Basin:   ESP_024224_1540   ESP_031872_1540   (Interval in Earth days: 595)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-25.8

54.7

-24.

9.444

47.0

32.1

Windstreak and Bedform Changes:   ESP_024241_1985   ESP_025085_1985   (Interval in Earth days: 66)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.24

302.

-0.0

-28.1

36.9

41.0

Well-Preserved 8 Kilometer Crater:   ESP_024080_1340   ESP_032928_1340   (Interval in Earth days: 690)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-45.4

25.7

6.66

20.83

55.9

56.0

Prominent Channel Form on Tyrrhena Patera:   ESP_024222_1590   ESP_024723_1590   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-20.9

107.

-7.9

15.92

43.1

48.9

Cerberus Fossae Streak and Bedform Changes:   ESP_024075_1930   ESP_024563_1930   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
12.74

154.

3.78

-23.4

35.2

38.4

Landforms Including Fans in Terrain Northwest of Gale Crater:   ESP_023944_1775   ESP_026990_1775   (Interval in Earth days: 237)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-2.56

135.

-24.

1.169

35.7

54.8


  


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