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.

Interesting Crater Ejecta in Columbus Crater:   ESP_016861_1505   ESP_017639_1505   (Interval in Earth days: 60)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-29.3

193.

1.16

-12.7

68.3

73.7

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

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 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

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

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

Northern Plains West of Erebus Montes:   ESP_016650_2205   ESP_035427_2205   (Interval in Earth days: 1464)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
40.26

185.

-1.2

27.98

42.1

39.3

Ejecta of Crater Sectioned by Erosion:   ESP_016896_1710   ESP_025678_1710   (Interval in Earth days: 684)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.92

315.

6.04

-5.75

54.6

53.8

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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