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.

Very Recent Small Impact Crater:   ESP_016630_1720   ESP_030291_1720   (Interval in Earth days: 1064)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.08

17.6

-3.5

8.058

52.4

48.4

Possible MSL Rover Landing Site in Northeast Syrtis Region:   ESP_016575_1980   ESP_016509_1980   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.81

77.2

-17.

2.958

42.7

40.7

Possible Phyllosilicates:   ESP_016891_1710   ESP_017669_1710   (Interval in Earth days: 61)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.92

91.9

2.12

-13.6

54.8

59.8

Mesa Island in East Acidalia Planitia:   ESP_016301_2250   ESP_016578_2250   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
44.70

352.

-3.9

-20.7

44.9

45.2

Eroded Material Adjacent to Cerberus Fossae:   ESP_016506_1890   ESP_017495_1890   (Interval in Earth days: 77)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.114

160.

2.89

-11.8

42.9

49.1

Small Rampart Crater Near the Central Peak of Lyot Crater:   ESP_016326_2305   ESP_060026_2305   (Interval in Earth days: 3405)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
50.39

29.2

-3.9

16.71

47.2

47.4

Possible Landslide Triggered by Impact:   ESP_016386_1475   ESP_016531_1475   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-32.4

201.

1.20

16.67

65.1

65.9

Crater with Central Uplift Northwest of Argyre Planitia:   ESP_016712_1435   ESP_018914_1435   (Interval in Earth days: 172)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-36.1

302.

-0.8

14.26

71.9

74.4

Extensive Crater Ejecta Blanket in Galaxias Colles:   ESP_016704_2180   ESP_017337_2180   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
37.86

150.

8.31

-9.63

40.7

42.0

Layers Exposed in Wall of Crater in the Floor of Hydaspis Chaos:   ESP_016513_1850   ESP_017502_1850   (Interval in Earth days: 77)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
5.146

329.

3.09

-12.0

44.4

51.1


  


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