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.

Pitted Mounds in Aurorae Chaos :   ESP_058196_1700   ESP_057774_1700   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-10.0

323.

2.01

-6.81

31.1

35.5

Gusev Crater Mesas :   ESP_058096_1645   ESP_058030_1645   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.1

175.

-12.

14.44

31.7

30.0

Dissected Fan or Delta in Terby Crater :   ESP_058192_1510   ESP_059405_1510   (Interval in Earth days: 95)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-28.6

75.2

-4.3

8.821

31.6

44.4

Stratigraphy in Ius Chasma Region :   ESP_058079_1720   ESP_058725_1720   (Interval in Earth days: 51)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.95

278.

-4.7

6.876

33.2

29.8

Ancient Bedforms on Gordii Dorsum :   ESP_058055_1895   ESP_058767_1895   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.255

210.

3.71

-10.2

42.0

35.8

Possible Olivine-Rich Terrain :   ESP_057902_1570   ESP_058680_1570   (Interval in Earth days: 60)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-22.7

70.6

4.04

-15.5

30.8

33.4

Crescentic Feature on South Polar Layered Deposits :   ESP_057951_0925   ESP_057831_0925   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-87.6

240.

7.09

20.50

68.9

66.4

Exposed Bedrock in Terrace of 44-Kilometer Diameter Crater in Margaritifer Terra :   ESP_057932_1670   ESP_057866_1670   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-12.9

331.

-4.7

9.629

32.8

32.4

Candidate Landing Site for 2020 Mission Near Jezero Crater :   ESP_058139_1985   ESP_058429_1985   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.17

76.9

-8.4

6.967

47.9

43.3

Well-Preserved Ejecta of 20-Kilometer Crater Northeast of Ascraeus Mons :   ESP_058040_1995   ESP_058831_1995   (Interval in Earth days: 62)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
19.19

259.

-6.3

14.41

49.8

39.1


  


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