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.

Small Delta or Fan:   ESP_073960_1630   ESP_074105_1630   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-16.6

211.

-5.2

10.88

53.8

51.2

Channel along Edge of Crater:   ESP_074028_1445   ESP_066233_1445   (Interval in Earth days: 607)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-35.1

156.

7.22

-5.51

52.2

41.6

Inlet Valley to Jezero Crater:   ESP_074268_1990   ESP_074413_1990   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.58

76.8

6.94

20.62

63.9

62.7

Gorgonum Chaos:   ESP_074251_1425   ESP_074396_1425   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-36.9

188.

6.08

18.51

49.3

46.2

Small Delta or Fan:   ESP_074009_1900   ESP_082053_1900   (Interval in Earth days: 626)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.837

310.

-3.3

22.98

60.6

57.3

Ridge and Pits in Cydonia Mensae:   ESP_073599_2100   ESP_073454_2100   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
29.59

339.

1.89

-14.1

66.8

66.6

Rayed Impact Crater in Meridiani Planum:   ESP_073572_1785   ESP_073638_1785   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.56

0.52

-0.7

-20.9

57.4

59.0

Landslides inside Impact Crater:   ESP_073749_1860   ESP_073815_1860   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
5.745

207.

7.31

-11.9

58.3

59.8

Gullies on Pole-Facing Slope of Ice-Filled Crater:   ESP_073591_1385   ESP_073446_1385   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-40.9

206.

8.21

-8.15

59.6

62.9

Ares Vallis Landform:   ESP_073639_1950   ESP_073916_1950   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
14.59

329.

-4.6

-18.6

61.8

63.7


  


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