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 Mission in Jezero Crater :   ESP_058996_1985   ESP_058930_1985   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.44

77.2

-9.3

12.63

38.8

37.8

Candidate Mars 2020 Landing Site in Gusev Crater :   ESP_058742_1645   ESP_066562_1645   (Interval in Earth days: 609)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.2

175.

0.28

-10.4

30.7

41.2

Landslide in Hydraotes Chaos :   ESP_058776_1815   ESP_058842_1815   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
1.538

324.

11.2

-12.9

31.2

32.9

Colorful Impact Ejecta in Ladon Valles:   ESP_058565_1620   ESP_067282_1620   (Interval in Earth days: 680)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-17.7

328.

2.23

-7.96

30.1

38.5

East Candor Chasma Wall :   ESP_058619_1735   ESP_058764_1735   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.52

293.

-4

8.404

30.8

29.8

Candidate Landing Site for 2020 Mission in Jezero Crater :   ESP_058574_1985   ESP_058640_1985   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.45

77.3

10.7

-12.5

41.6

42.2

Looking for Impact Craters near Nili Fossae :   ESP_058561_2015   ESP_058627_2015   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
21.42

72.1

8.07

-14.6

43.9

44.5

South Polar Layered Deposits :   ESP_058589_0915   ESP_058393_0885   (Interval in Earth days: 15)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-88.5

118.

16.1

19.12

78.3

76.1

Fan-Shaped Group of Ridges Northwest of Hellas Region :   ESP_058417_1490   ESP_059419_1490   (Interval in Earth days: 78)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-30.4

52.3

-11.

18.51

33.8

45.2

Gully System in Thaumasia Fossae Crater :   ESP_058383_1325   ESP_058106_1325   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-47.1

263.

-13.

19.20

42.7

38.0


  


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