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.

Stunning Outcrop in Nilosyrtis Mensae:   ESP_088681_2160   ESP_088892_2160   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
35.47

65.6

-5.2

-14.7

44.7

46.4

Fan in Crater North of Nepenthes Mensae:   ESP_088705_1815   ESP_088916_1815   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
1.468

133.

4.91

-7.86

54.8

55.9

Steep Sandy Slopes in Coprates Chasma:   ESP_088554_1660   ESP_088620_1660   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.7

298.

11.2

-14.2

63.4

65.0

Kasei Valles Alluvial Fans:   ESP_088633_2040   ESP_088778_2040   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
23.55

298

-6.4

3.817

46.5

46.1

Ridged Flow-Like Features in Deuteronilus Mensae:   ESP_088445_2225   ESP_088511_2225   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
42.33

26.8

8.67

-8.24

42.8

44.5

Jezero Crater:   ESP_088562_1985   ESP_089208_1985   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.47

77.4

-8.9

15.11

48.1

47.9

Fan-Shaped Feature in Ismenius Lacus:   ESP_088485_2145   ESP_088696_2145   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
33.95

17.5

-4.9

-15.7

44.2

45.9

Structure of Viscous Flow Feature Exposed by Ice Degradation:   ESP_088510_2220   ESP_088431_2220   (Interval in Earth days: 7)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
41.58

51.9

11.0

-13.2

42.7

44.7

Flow Entering Fretted Terrain Valley:   ESP_088735_2170   ESP_088669_2170   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
36.59

32.1

-14.

4.335

45.7

43.8

North Polar Residual Cap Topography:   ESP_088751_2685   ESP_089016_2685   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
88.39

276.

-17.

-26.2

64.2

66.2


  


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