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.

Tongue-Shaped Flow Feature in Hellas Montes Region:   ESP_023141_1435   ESP_023642_1435   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-36.0

101.

-5.7

15.39

37.1

41.8

Clay-Bearing Layered Deposit in Unnamed Crater North of Proctor Crater:   ESP_023302_1345   ESP_023803_1345   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-45.3

27.9

-8.6

6.167

44.4

51.2

Proposed Landing Site in Mawrth Vallis:   ESP_023488_2050   ESP_023554_2050   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
24.53

338.

6.73

-14.0

44.9

45.5

Pitted Materials in Bakhuysen Crater:   ESP_020309_1570   ESP_020731_1570   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-22.8

16.2

8.95

-6.93

57.0

54.4

A Pedestal Crater in Malea Planum:   ESP_022787_1085   ESP_030580_1085   (Interval in Earth days: 607)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-71.3

55.1

-4.6

21.88

56.9

53.9

Exposure of South Polar Layered Deposits:   ESP_022839_0930   ESP_023009_0930   (Interval in Earth days: 13)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-87.1

141.

0.01

14.35

71.4

71.9

Bedrock Exposed in 60-Kilometer Crater East of Valles Marineris:   ESP_023027_1740   ESP_029884_1740   (Interval in Earth days: 535)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.80

328.

7

22.75

33.0

50.6

Layered Deposits and Possible MSL Rover Landing Site in Niesten Crater:   ESP_022892_1520   ESP_022470_1520   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.6

57.8

-3.8

11.01

32.8

33.0

Knob in South Polar Layered Deposits:   ESP_023066_0955   ESP_032020_0955   (Interval in Earth days: 698)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-84.4

12.1

6.73

-6.06

70.6

73.7

Proposed Landing Site in Ismenius Cavus:   ESP_022880_2140   ESP_031161_2140   (Interval in Earth days: 645)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
33.82

17.2

-0.3

23.84

60.4

65.9


  


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