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 Terraced Crater in Arcadia Planitia:   ESP_034319_2260   ESP_034754_2260   (Interval in Earth days: 34)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
45.67

198.

3.45

23.42

42.8

40.0

Meander in Central Channel in Nanedi Valles:   ESP_034236_1855   ESP_035792_1855   (Interval in Earth days: 121)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
5.183

310.

3.71

-19.7

44.7

53.6

Light-Toned Stratified Materials in Melas Chasma:   ESP_034250_1670   ESP_035450_1670   (Interval in Earth days: 93)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-12.8

289.

12.9

-23.9

53.7

63.6

Crater-Related Pitted Materials in 8-Kilometer Diameter Hellas Region Crater:   ESP_034297_1380   ESP_034363_1380   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-41.9

91.6

1.75

-17.4

75.1

76.9

Mesa in Olympica Fossae:   ESP_034146_2050   ESP_034436_2050   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
24.78

246.

-8.3

18.70

40.6

39.1

Outflow Channel Features Associated with Small Chaotic Terrain:   ESP_034355_1770   ESP_034922_1770   (Interval in Earth days: 44)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-2.88

302.

6.96

-7.21

49.3

54.3

North Polar Residual Cap:   ESP_034369_2690   ESP_034526_2690   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
89.00

280.

-27.

-22.1

69.1

67.5

Channel System in Tharsis Region:   ESP_034489_2005   ESP_034779_2005   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
20.24

241.

-3.1

18.59

41.9

41.3

Flows Near Echus Chasma:   ESP_034158_1865   ESP_037270_1865   (Interval in Earth days: 242)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
6.245

279.

6.61

-18.3

43.4

56.1

Northern Plains Features:   ESP_034200_2335   ESP_034266_2335   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
53.02

205.

4.92

-6.54

46.1

46.6


  


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