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

Very Large Pit Crater in Daedalia Planum:   ESP_016411_1605   ESP_024481_1605   (Interval in Earth days: 629)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-19.4

237.

0

-21.9

56.8

47.0

Aureum Chaos:   ESP_016803_1770   ESP_088144_1770   (Interval in Earth days: 5559)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-3.11

334.

-3.6

-16.2

51.1

57.8

Terrain South of Newcomb Crater:   ESP_016736_1520   ESP_068970_1525   (Interval in Earth days: 4070)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.6

5.59

4.65

-7.50

65.7

63.9

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

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

Central Uplift and Olivine-Rich Ponded Material in Elorza Crater:   ESP_016659_1710   ESP_017081_1710   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.77

304.

10.5

-3.93

52.2

56.4

Crater in Acidalia Planitia:   ESP_016841_2340   ESP_017830_2340   (Interval in Earth days: 77)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
53.72

7.48

5.69

-6.67

45.4

44.9

Cerberus Fossae:   ESP_016822_1865   ESP_017600_1865   (Interval in Earth days: 60)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
6.281

173.

2.06

-11.4

46.2

50.8

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


  


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