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 ExoMars Near Hypanis Valles:   ESP_040091_1925   ESP_047884_1925   (Interval in Earth days: 607)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
12.47

314.

2.78

22.11

51.3

55.0

Candidate Landing Site for 2020 Mission at Sabrina Vallis Delta:   ESP_039801_1920   ESP_049717_1920   (Interval in Earth days: 773)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
11.75

313.

-5.0

-14.4

54.7

39.5

Alluvial Fans in Southeastern Mojave Crater:   ESP_039695_1875   ESP_040618_1875   (Interval in Earth days: 72)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.214

327.

-7.2

11.40

53.2

41.0

Channels in Savich Crater:   ESP_039664_1530   ESP_047444_1530   (Interval in Earth days: 606)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-26.8

96.9

3.06

-14.4

40.0

49.9

Barchan Dune Changes:   ESP_039666_1380   ESP_039732_1380   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-41.4

44.6

1.20

-14.9

41.0

41.6

Ridges in Zephyria Planum:   ESP_039675_1760   ESP_040097_1760   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.03

153.

5.34

-6.18

46.5

42.2

Candidate ExoMars Landing Site Near Hypanis Valles:   ESP_039735_1920   ESP_040658_1920   (Interval in Earth days: 72)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
11.86

314.

0.25

14.90

55.2

43.0

Palikir Crater Wall Gullies and Linear Dune Gullies:   ESP_039713_1380   ESP_039647_1380   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-41.6

202.

-4.3

11.91

41.0

40.4

Light-Toned Stratified Materials in Hebes Chasma:   ESP_039723_1790   ESP_040211_1790   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-0.57

282.

13.9

-22.8

47.1

43.8

Northeast Syrtis Major Planum Lava and Hydrated Minerals:   ESP_039836_1965   ESP_048486_1965   (Interval in Earth days: 674)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
16.50

76.7

-1.0

19.24

57.2

54.7


  


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