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.

Layers with Iron Magnesium Phyllosilicate on Crater Floor:   PSP_010419_2140   PSP_010841_2140   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
33.71

17.1

16.6

1.275

49.7

55.7

Uplift in Oudemans Crater:   ESP_011966_1700   ESP_012467_1700   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-9.73

268.

2.38

27.90

55.8

50.3

Possible MSL Rover Landing Site Eberswalde Crater:   ESP_011265_1560   ESP_011331_1560   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-23.8

326.

20.4

-1.11

60.2

61.4

Distributary Channel South of Ascraeus Mons:   PSP_010872_1865   ESP_011373_1865   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
6.197

254.

-2.2

20.12

55.7

55.8

Lonar Crater Ejecta:   PSP_010800_2535   PSP_010787_2535   (Interval in Earth days: 1)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
73.30

39.0

20.1

6.293

68.3

68.9

Disrupted Terrain in Southeastern Cerberus Palus:   ESP_011377_1835   ESP_011522_1835   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
3.357

147.

-2.2

13.96

57.5

56.5

Valley Features and Light-Toned Deposits along Melas Region Southern Wall:   ESP_011293_1710   ESP_019218_1710   (Interval in Earth days: 617)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-9.12

282.

0.24

-21.3

58.2

59.7

Well-Preserved Unnamed Crater in Acidalia Planitia:   PSP_010579_2170   ESP_016104_2170   (Interval in Earth days: 431)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
36.66

329.

4.65

19.26

52.8

40.8

Very Recent Small Crater:   PSP_010772_2145   ESP_045136_2145   (Interval in Earth days: 2678)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
34.38

100.

4.13

-8.37

54.7

42.8

Phyllosilicate Ring in Terra Sirenum:   PSP_010901_1510   ESP_055194_1510   (Interval in Earth days: 3452)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-28.9

187.

0.35

-23.2

66.4

62.6


  


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