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 ExoMars Landing Site in Oxia Planum:   ESP_088078_2000   ESP_088012_2000   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
19.56

334.

-28.

-7.03

48.3

46.2

Dune Monitoring in Northern Mid-Latitude Crater:   ESP_088171_2295   ESP_088395_2295   (Interval in Earth days: 18)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
49.11

309.

-5.5

19.83

44.5

42.6

Pedestal Crater Marginal Pits:   ESP_088126_2400   ESP_088205_2400   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
59.79

96.3

-9.1

6.586

47.8

46.5

Planned ExoMars Landing Site in Oxia Planum:   ESP_088157_1975   ESP_088447_1975   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.33

336.

-8.6

8.83

47.5

46.8

Crater Infill:   ESP_088354_1870   ESP_088565_1870   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
6.953

356.

10.0

-5.16

51.1

52.6

North-Pole-Facing Deposit in Crater Associated with Headwall Erosion:   ESP_088226_2150   ESP_088661_2150   (Interval in Earth days: 34)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
34.60

249.

-5.8

17.63

43.6

42.7

Group of Channels along Old Crater Wall:   ESP_088288_2130   ESP_088499_2130   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
32.59

357.

-6.7

-18.5

44.0

45.7

Patterned Ground in Elysium Planitia:   ESP_088335_1845   ESP_088546_1845   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
4.634

156.

3.81

-11.4

52.6

54.2

Distinct Crater Wall Layers in Oxia Planum:   ESP_088236_1995   ESP_087946_1995   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
19.08

338.

-1.7

-16.6

46.5

47.0

Dune Monitoring in Northern Mid-Latitude Crater:   ESP_088230_2400   ESP_088454_2400   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
59.81

135.

-4.2

14.96

47.5

46.2


  


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