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.

Region North of Samara Valles:   ESP_039998_1620   ESP_040987_1620   (Interval in Earth days: 77)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-17.5

338.

-4.3

-19.4

38.3

35.5

Valleys in Crater in Noachis Terra:   ESP_039931_1555   ESP_040788_1555   (Interval in Earth days: 67)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-24.0

8.50

-4.8

21.63

37.9

32.5

Pasted-on Material on Crater Ejecta:   ESP_040131_1930   ESP_040487_1930   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
13.00

302.

3.43

15.22

51.1

45.8

Candidate Landing Site for 2020 Mission in Hadriacus Palus:   ESP_040113_1525   ESP_040390_1525   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.0

78.4

8.57

-18.6

35.1

35.9

Daedalia Planum Lava Flow:   ESP_039910_1470   ESP_040543_1470   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-32.8

222.

5.35

-14.7

37.2

36.8

Crater with Light-Toned Wall Rock in Outflow Channel Floor:   ESP_040038_1760   ESP_041238_1760   (Interval in Earth days: 93)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-3.97

324.

-5.5

-20.6

42.9

36.0

Dunes Seen in MOC Images:   ESP_040023_1910   ESP_041434_1910   (Interval in Earth days: 110)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
10.74

12.1

-4.2

-27.4

51.4

39.6

Gullied Crater:   ESP_040251_1345   ESP_040607_1345   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-45.1

274.

0.28

13.24

39.6

40.6

Layers in Terra Sirenum:   ESP_040293_1520   ESP_047506_1520   (Interval in Earth days: 562)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.8

203.

20.9

-0.04

33.1

48.1

Crater with Breached Rim and Interior Terraced Landform:   ESP_040182_1405   ESP_058485_1405   (Interval in Earth days: 1426)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-39.2

356.

6.48

-5.70

36.9

38.4


  


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