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.

Gullies and Lobate Flow Feature in Nereidum Montes :   ESP_058223_1335   ESP_058790_1335   (Interval in Earth days: 44)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-46.0

311.

-1.1

-15.9

39.6

47.7

Possible Mud Volcano :   ESP_058214_1555   ESP_075266_1555   (Interval in Earth days: 1329)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-24.4

193.

4.81

16.57

30.0

36.2

Channel East of Majuro Crater :   ESP_058073_1465   ESP_058864_1465   (Interval in Earth days: 62)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-33.3

84.9

0.97

21.34

32.3

38.1

Western Rim of Rayed Crater in Daedalia Planum :   ESP_058094_1565   ESP_067721_1565   (Interval in Earth days: 750)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-23.0

230.

0.94

10.31

30.2

41.6

Possible Jarosite-Rich Terrain in North Mawrth Vallis :   ESP_058182_2060   ESP_058749_2060   (Interval in Earth days: 44)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
25.59

340.

4.30

-14.0

52.2

45.9

Fans in Roddy Crater :   ESP_058117_1580   ESP_058684_1580   (Interval in Earth days: 45)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-21.5

320.

12.1

-11.2

29.2

32.7

Crater Partially Buried by Ejecta from Yuty Crater:   ESP_058143_2020   ESP_058855_2020   (Interval in Earth days: 56)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
21.98

325.

7.78

-1.45

49.8

41.6

Terrain in Lyot Crater :   ESP_058035_2295   ESP_058101_2295   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
48.88

30.3

8.51

-7.35

73.2

73.1

South Polar Layered Deposits :   ESP_057906_0925   ESP_057891_0925   (Interval in Earth days: 1)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-87.5

54.9

2.46

13.98

69.5

67.4

North Mid-Latitude Crater :   ESP_058190_2115   ESP_085422_2115   (Interval in Earth days: 2122)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
31.27

122.

-3.3

8.468

57.0

49.0


  


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