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.

Ridges in Western Elysium Planitia:   ESP_037342_2010   ESP_068108_2010   (Interval in Earth days: 2397)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
20.90

110.

-5.0

-24.9

54.7

47.3

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

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

Layered Rocks of Ophir Mensa:   ESP_037217_1760   ESP_036795_1760   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-3.95

286.

-3.9

17.29

57.2

55.7

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

Biblis Patera:   ESP_037588_1825   ESP_037865_1825   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.431

236.

9.06

-10.7

55.4

57.6

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

Crater Floor in CTX Image:   ESP_037234_1520   ESP_037801_1520   (Interval in Earth days: 44)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.3

185.

-6.6

11.01

66.5

60.9

Crater on North Polar Layered Deposits:   ESP_037220_2680   ESP_037169_2680   (Interval in Earth days: 4)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
87.97

134.

-8.9

-21.3

78.2

77.9


  


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