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.

Possible Mafic-Rich Armored Ejecta Deposits:   ESP_074190_1195   ESP_074058_1195   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-59.9

61.9

-20.

6.187

58.5

58.6

Light-Toned Deposits in Iani Chaos:   ESP_074087_1780   ESP_074021_1780   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-2.04

342.

-6.0

19.68

56.1

54.4

Tilted Layers in Electris Region:   ESP_073948_1435   ESP_073882_1435   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-36.2

181.

-8.9

7.304

54.7

54.4

Channel along Edge of Crater:   ESP_074028_1445   ESP_066233_1445   (Interval in Earth days: 607)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-35.1

156.

7.22

-5.51

52.2

41.6

Phaethontis Region Slope Monitoring:   ESP_074145_1390   ESP_073868_1390   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-40.7

204.

-14.

6.12

53.0

55.6

Small Delta or Fan:   ESP_073983_1385   ESP_074260_1385   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-41.3

306.

0.43

-26.6

54.4

52.4

Resistant Material in Olympus Mons Aureole Ridges:   ESP_073920_1990   ESP_074065_1990   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.79

218.

1.52

19.57

64.0

63.0

Lava-Crater Interaction in Elysium Planitia:   ESP_073949_1860   ESP_074239_1860   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
5.812

148.

-1.0

25.38

58.9

56.1

Well-Preserved 3-Km Impact Crater in Nereidum Montes:   ESP_074035_1360   ESP_073890_1360   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-43.6

326.

11.5

-7.18

53.3

56.9

Channel Crossing Heavily Eroded Wrinkle Ridge:   ESP_074146_1485   ESP_073790_1485   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-31.4

175.

-4.9

-20.8

51.1

57.1


  


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