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.

Margin of Lobate Deposit in Nereidum Montes:   ESP_086272_1405   ESP_085903_1405   (Interval in Earth days: 29)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-39.4

323.

23.9

-13.2

60.4

56.6

Trough in Nilosyrtis Mensae:   ESP_086255_2300   ESP_086888_2300   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
49.43

59.1

-3.7

-23.5

52.4

49.3

Mesa Stratigraphy at Terby Crater:   ESP_086268_1525   ESP_086835_1525   (Interval in Earth days: 44)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.1

73.7

3.54

-8.39

53.5

62.3

Layers in Crater in Northeast Sinus Meridiani:   ESP_086244_1805   ESP_086666_1805   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
0.362

5.66

2.87

-23.9

40.6

46.6

Hillslope Morphologies Southeast of Ostrov Crater:   ESP_086219_1520   ESP_085375_1520   (Interval in Earth days: 66)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.5

332.

-6.1

8.78

53.6

40.3

Features around Cerberus Palus:   ESP_086252_1850   ESP_086819_1850   (Interval in Earth days: 44)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
4.904

146.

5.75

-7.57

39.5

45.0

North-Pole-Facing Deposit in Crater:   ESP_086208_2275   ESP_086841_2275   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
47.24

261.

5.23

-18.4

51.0

48.1

A Slice through the Layercake:   ESP_084979_1975   ESP_085045_1975   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.49

336.

16.6

-4.34

44.6

45.3

Exposure of Layered Materials along Hellas Planitia Rim Escarpment:   ESP_085807_1590   ESP_086242_1590   (Interval in Earth days: 34)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-20.7

63.1

-16.

0.443

44.6

49.5

Steep Dark-Floored Crater with Wind Streak and Dunes:   ESP_085783_1830   ESP_085717_1830   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.996

354.

-8.0

6.889

38.0

36.5


  


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