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.

Jezero Crater Outcrop:   ESP_078567_1985   ESP_080545_1985   (Interval in Earth days: 154)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.50

78.0

4.62

25.67

44.1

48.7

Scarp in Claritas Fossae:   ESP_078218_1575   ESP_078152_1575   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-22.4

254.

-26.

-3.06

63.2

61.0

Scarp with Yardangs:   ESP_078326_1735   ESP_078260_1735   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.21

181.

4.36

27.22

52.6

50.2

Small Shield East of Pavonis Mons:   ESP_078363_1775   ESP_079141_1775   (Interval in Earth days: 60)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-2.49

250.

1.99

-9.15

51.2

57.0

Light Toned Outcrop in Arsinoes Chaos:   ESP_078426_1715   ESP_086720_1715   (Interval in Earth days: 646)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.17

331.

-1.3

-15.6

55.0

50.1

Pavonis Mons Southern Caldera Wall Upper Flank and Caldera Floor Sample:   ESP_078495_1800   ESP_079207_1800   (Interval in Earth days: 56)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
0.212

247.

-8.1

8.909

51.6

54.6

Small Crater near Phoenix Landing Site:   ESP_077849_2485   ESP_078429_2485   (Interval in Earth days: 45)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
68.21

232.

0

14.36

59.8

53.5

Crater and Lava Fill in Elysium Planitia:   ESP_078195_1825   ESP_079474_1825   (Interval in Earth days: 99)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.309

156.

3.56

18.45

47.3

53.6

Athabasca Valles Side Channel:   ESP_077905_1880   ESP_079329_1880   (Interval in Earth days: 111)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.854

154.

-2.7

15.05

43.5

50.5

Ridge Network in Hellas Planitia:   ESP_077843_1420   ESP_086717_1420   (Interval in Earth days: 692)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-37.6

53.8

-2.3

22.29

67.0

66.0


  


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