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.

Bedrock in Walls of Well-Preserved Impact Crater in Tartarus Montes:   ESP_019222_2055   ESP_019367_2055   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
25.03

167.

-7.6

5.969

49.8

49.8

Exposure of North Polar Layered Deposits:   ESP_019343_2685   ESP_028008_2685   (Interval in Earth days: 675)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
88.28

50.8

-14.

-24.3

74.8

73.1

Flow Material in Equatorial Crater:   ESP_019267_1720   ESP_024858_1720   (Interval in Earth days: 436)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.05

23.2

-8.4

-26.9

58.1

46.5

Alpine Glacier:   ESP_019213_2210   ESP_019503_2210   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
40.86

51.3

-8.0

14.46

51.2

52.7

Steep North Polar Boundary Scarp:   ESP_018943_2655   ESP_019181_2655   (Interval in Earth days: 19)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
85.36

186.

0

-13.2

67.0

70.6

Thermally-Distinct Material at Distal Coogoon Valles:   ESP_019084_1980   ESP_060437_1980   (Interval in Earth days: 3222)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.85

336.

-5.5

5.547

49.5

37.7

Well-Preserved Impact Crater in Arabia Terra:   ESP_019162_1975   ESP_019439_1975   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.23

5.48

7.48

-19.6

48.9

52.7

Cluster of Zunil Crater Secondaries:   ESP_019064_1835   ESP_019209_1835   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
3.656

163.

2.92

17.53

52.6

51.6

Layered Terrains in Aeolis Planum:   ESP_018972_1755   ESP_019605_1755   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.27

154.

15.7

-5.86

55.1

56.0

Steep North-Polar Boundary Scarp:   ESP_018957_2655   ESP_019195_2655   (Interval in Earth days: 19)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
85.25

160.

3.29

-9.91

67.0

70.5


  


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