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.

InSight Mission Candidate Landing Site:   ESP_036484_1835   ESP_037051_1835   (Interval in Earth days: 44)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
3.321

137.

8.92

-5.29

53.1

55.1

Small Crater in Utopia Planitia:   ESP_036446_2250   ESP_037224_2250   (Interval in Earth days: 61)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
44.61

90.6

-3.2

-17.2

48.2

58.5

Crater Cluster on North Polar Layered Deposits:   ESP_036608_2620   ESP_036423_2620   (Interval in Earth days: 15)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
81.83

333.

-7.0

8.635

65.5

62.6

Steep North Polar Peripheral Scarp:   ESP_036548_2655   ESP_036799_2655   (Interval in Earth days: 19)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
85.23

160.

-6.8

-17.2

66.9

70.6

Very Fresh Small Crater:   ESP_036685_1670   ESP_037397_1670   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-12.8

52.7

-4.1

7.672

61.6

58.8

Landforms Near Nili Fossae:   ESP_036552_2000   ESP_036763_2000   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
19.67

78.9

8.38

-4.42

48.2

50.4

Head of Jezero Crater Fan:   ESP_036618_1985   ESP_037119_1985   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.51

77.2

5.83

17.35

49.0

51.0

Channels Near Contact Between Chryse Planitia and Vistula Valles:   ESP_036715_1945   ESP_037348_1945   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
14.31

309.

7.04

-18.6

50.3

55.9

Korolev Crater Changes:   ESP_036654_2530   ESP_036852_2530   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
72.79

164.

-4.5

-22.0

60.9

65.0

Light-Toned Deposits with Possible Inverted Channels in Eridani Region:   ESP_036509_1485   ESP_052768_1485   (Interval in Earth days: 1267)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-31.1

180.

-0.0

-18.7

72.6

72.9


  


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