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.

Candidate Landing Site for 2020 and Sample Return Missions at Jezero Crater:   ESP_062240_1985   ESP_062174_1985   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.37

76.9

2.90

25.46

45.0

42.8

Furrows and Dunes in Hyperborei Cavi:   ESP_062244_2605   ESP_062270_2605   (Interval in Earth days: 2)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
80.33

308.

-1.2

15.13

57.6

56.8

Pedestal Crater West of Lyot Crater:   ESP_062242_2265   ESP_062967_2265   (Interval in Earth days: 56)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
45.92

18.4

1.19

28.58

42.7

45.6

Dunes Dubbed Del Mar:   ESP_062326_2600   ESP_062418_2600   (Interval in Earth days: 8)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
79.84

234.

-8.8

5.037

58.1

57.7

Ice-Filled Crater:   ESP_062339_2640   ESP_062167_2640   (Interval in Earth days: 13)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
84.16

237.

-16.

-0.17

61.3

59.8

Polar Barchan Dunes:   ESP_062237_2635   ESP_062198_2635   (Interval in Earth days: 4)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
83.64

121.

8.2

-7.26

59.3

59.9

Undulations on Dokka Crater Ice Dome:   ESP_062353_2570   ESP_062406_2570   (Interval in Earth days: 4)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
77.05

213.

4.78

-11.2

55.7

57.1

Ice-Filled Graben:   ESP_062432_2260   ESP_062366_2260   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
45.75

229.

4.83

20.49

43.4

41.6

Low Relief Polar Cap Outlier in Olympia Mensae:   ESP_062581_2550   ESP_062568_2550   (Interval in Earth days: 1)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
74.76

110.

5.44

-8.33

55.8

56.7

Ophir Chasma:   ESP_062417_1755   ESP_062483_1755   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.29

286.

0.50

-24.7

56.3

58.1


  


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