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.

Gullied Crater Wall in Southeastern Terra Cimmeria:   ESP_024286_1330   ESP_024576_1330   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-46.4

163.

-3.9

19.77

60.7

64.3

Remnant of Unconformable Deposit in Electris:   ESP_023929_1425   ESP_024074_1425   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-37.0

189.

-20.

-5.72

49.1

50.5

Crater Rim with Possible Columnar Jointing:   ESP_024288_1945   ESP_024710_1945   (Interval in Earth days: 32)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
14.52

98.3

21.7

6.703

34.1

36.4

Possible Future Landing Site at Edge of Libya Montes:   ESP_024038_1835   ESP_023405_1835   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
3.516

86

5.65

27.23

33.6

32.4

MSL Rover Landing Site in Gale Crater:   ESP_024234_1755   ESP_024300_1755   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.64

137.

-5.2

-24.4

36.6

38.8

Possible Bedform Changes in Medusae Fossae:   ESP_024047_1895   ESP_024113_1895   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.508

197.

25.0

5.939

32.7

34.4

Massif in Reull Vallis:   ESP_024051_1365   ESP_024407_1365   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-43.2

97.0

7.01

22.35

53.8

59.0

MSL Landing Site in Gale Crater:   ESP_023957_1755   ESP_024023_1755   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.55

137.

15.1

-6.86

32.6

34.9

Small Mounds in Chryse Planitia:   ESP_024082_1995   ESP_023581_1995   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
19.07

322.

7.16

-17.0

37.1

42.1

Dunes:   ESP_024060_1205   ESP_023928_1205   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-59.1

218.

-18.

5.39

67.4

63.9


  


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