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.

Crater and Ice-Rich Terrain:   ESP_086346_2250   ESP_086992_2250   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
44.64

95.4

-5.9

13.11

49.1

43.8

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

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

Impact Monitoring in Arcadia Planitia:   ESP_086330_2205   ESP_089389_2205   (Interval in Earth days: 238)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
40.34

173.

-8.4

7.166

47.3

47.9

Thermophysical Boundary West of Hebrus Valles:   ESP_086345_2015   ESP_087123_2015   (Interval in Earth days: 60)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
21.09

124.

5.18

-9.06

39.9

43.0

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

Crater in Cerberus Fossae:   ESP_086212_1890   ESP_086858_1890   (Interval in Earth days: 51)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.700

158.

4.61

25.42

38.9

41.3

Young Impact on Layers in Protonilus Mensae:   ESP_086295_2230   ESP_086717_2230   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
42.61

46.9

5.28

-12.4

47.7

46.4

Fluvial Valley South of Ares Vallis:   ESP_086311_1890   ESP_087168_1890   (Interval in Earth days: 67)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.094

335.

4.24

24.34

39.5

43.5

Head of Lethe Vallis:   ESP_086199_1840   ESP_087056_1840   (Interval in Earth days: 67)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
3.785

153.

5.44

20.19

39.3

45.1


  


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