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 Oyama Crater:   ESP_037505_2035   ESP_037993_2035   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
23.46

340.

1.30

-13.3

55.9

62.0

Relaxed Crater:   ESP_037247_2160   ESP_063726_2155   (Interval in Earth days: 2064)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
35.50

181.

2.20

-8.78

54.9

56.1

Candidate New Impact Site:   ESP_037239_1820   ESP_042158_1820   (Interval in Earth days: 383)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.029

44.5

3.10

-15.4

55.1

40.2

Well-Preserved 1 to 2 Kilometer Impact Crater:   ESP_037208_1590   ESP_042694_1590   (Interval in Earth days: 428)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-20.8

173.

3.27

-23.6

62.9

56.6

Candidate Landing Site for 2020 Mission in Jezero Crater:   ESP_037330_1990   ESP_037818_1990   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.56

77.4

10.8

-8.98

53.2

58.8

Sand Monitoring in Pasteur Crater:   ESP_037332_1995   ESP_037477_1995   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
19.05

24.4

-7.5

10.11

54.8

54.5

Crater Floor:   ESP_037251_1740   ESP_063730_1740   (Interval in Earth days: 2063)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.99

78.3

-2.8

-17.1

57.7

58.7

Candidate ExoMars Landing Site:   ESP_037361_1920   ESP_045181_1920   (Interval in Earth days: 610)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
11.88

313.

-10.

4.934

55.3

45.4

Flows and Valleys in Northern Lycus Sulci Terrain:   ESP_037219_2130   ESP_037496_2130   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
32.90

225.

13.2

-5.40

53.1

58.1

InSight Mission Candidate Landing Site:   ESP_037552_1835   ESP_038317_1835   (Interval in Earth days: 60)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
3.445

138.

15.8

-6.93

54.6

58.2


  


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