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.

Small Feature on South Polar Layered Deposits:   ESP_041111_0925   ESP_041004_0925   (Interval in Earth days: 8)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-87.2

244.

7.47

28.48

80.0

76.6

Ridges and Light-Toned Outcrops North of Atlantis Chaos:   ESP_041151_1500   ESP_047309_1500   (Interval in Earth days: 480)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-29.7

181.

-8.0

2.323

39.6

50.5

Light-Toned Hydrated Materials Inside Ius Chasma:   ESP_041121_1725   ESP_048136_1725   (Interval in Earth days: 547)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.24

276.

1.18

20.39

33.8

43.6

Candidate Landing Site for 2020 Mission in Hypanis Valles Delta:   ESP_041436_1920   ESP_041858_1920   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
12.02

314.

-0.1

-24.4

37.7

39.3

Possible Degraded Crater on South Polar Layered Deposits:   ESP_041218_0925   ESP_041309_0925   (Interval in Earth days: 7)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-87.6

243.

3.20

9.973

83.4

83.5

Protonilus Region Terraces:   ESP_041129_2210   ESP_041406_2210   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
40.73

51.7

5.59

-14.1

57.6

55.0

Gigas Sulci:   ESP_040661_1890   ESP_041149_1890   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.091

233.

7.06

-29.4

41.8

40.3

Icy Scarp:   ESP_040772_1215   ESP_041062_1215   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-58.0

93.6

-4.8

13.05

51.8

55.0

Well-Preserved Gullied 15-Kilometer Impact Crater:   ESP_040964_1305   ESP_057856_1305   (Interval in Earth days: 1316)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-49.1

249.

-4.2

5.903

48.2

38.7

Layering on Floor of Orson Welles Crater:   ESP_040790_1805   ESP_056996_1805   (Interval in Earth days: 1263)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
0.309

314.

-20.

5.758

38.3

48.2


  


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