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.

Flow Boundary in Elysium Planitia:   ESP_036127_1970   ESP_036760_1970   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
16.56

161.

3.64

-12.2

47.8

51.6

Exposed Crater-Fill Megabreccias and Pitted Materials:   ESP_036176_1700   ESP_036110_1700   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-9.88

268.

-7.0

14.44

61.0

59.7

Candidate Future Landing Site in Ladon Valles:   ESP_036398_1595   ESP_036121_1595   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-20.1

329.

-6.5

11.53

66.6

66.2

Ridges Associated with Medusae Fossae:   ESP_036270_1840   ESP_037048_1840   (Interval in Earth days: 61)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
3.835

219.

6.35

-7.03

52.9

55.1

Pits in North Polar Layered Deposits:   ESP_036043_2645   ESP_036004_2645   (Interval in Earth days: 4)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
84.33

254.

7.23

-6.70

61.2

61.6

East Rim of Well-Preserved Impact Crater:   ESP_036335_2270   ESP_036757_2270   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
46.55

239.

6.41

-5.27

46.7

51.9

The Busy Flank of Arsia Mons :   ESP_031944_1790   ESP_030876_1790   (Interval in Earth days: 83)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.11

246.

7.53

-9.11

34.4

46.9

New Impact Site:   ESP_036336_1835   ESP_036481_1835   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
3.325

219.

-8.5

12.73

54.3

52.9

Changing Dunes and Ripples in Olympia Undae:   ESP_036099_2615   ESP_036073_2615   (Interval in Earth days: 2)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
81.63

178.

7.29

-7.01

59.7

60.4

Northwest of Crommelin Crater:   ESP_035962_1880   ESP_036529_1880   (Interval in Earth days: 44)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.851

348.

-10.

7.94

52.0

51.5


  


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