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.

Ridges or Flows in Northeast Gale Crater:   ESP_025790_1750   ESP_027135_1750   (Interval in Earth days: 104)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.71

137.

-6.0

3.949

52.2

55.9

Small Mounds in Chryse Planitia:   ESP_025427_1995   ESP_025282_1995   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
19.37

322.

6.11

-10.3

39.2

40.0

Mantle Layers in Crater in Terra Cimmeria:   ESP_025474_1380   ESP_051847_1380   (Interval in Earth days: 2055)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-41.6

127.

4.28

-18.6

74.1

73.7

Well-Preserved Impact Crater in Utopia Planitia:   ESP_025514_2045   ESP_025870_2045   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
24.44

107.

0.69

16.37

39.3

39.0

Clusters of Buttes and Mesas among Flows South of Western Cerberus Fossae:   ESP_025684_1885   ESP_026040_1880   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.775

149.

-6.7

6.019

45.2

46.2

Well Preserved 7-Kilometer Impact Crater in Utopia Planitia:   ESP_025791_1945   ESP_025646_1945   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
14.46

104.

24.6

6.969

40.6

41.4

Wrinkle Ridge Superimposed on Well-Preserved Crater:   ESP_025468_1640   ESP_024835_1640   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.7

288.

-5.8

12.96

56.2

47.5

Finely Stratified Units in Northeast of Gale Crater:   ESP_025724_1755   ESP_025579_1755   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.54

137.

5.03

-14.8

50.9

51.1

Flow Draped over Crater Rim Visible in CTX Image :   ESP_025563_1975   ESP_025207_1975   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.48

209.

15.2

2.131

39.4

38.8

Contact between Yardang-Forming Material and Platy Flow Material:   ESP_025473_1840   ESP_034255_1840   (Interval in Earth days: 684)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
3.897

149.

-3.9

28.53

45.2

43.3


  


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