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.

West Melas Chasma:   ESP_041991_1715   ESP_042136_1715   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.57

284.

-5.4

10.07

40.8

41.3

Candidate ExoMars Landing Site in Hypanis Valles:   ESP_041937_1920   ESP_042003_1920   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
11.88

314.

16.7

-5.73

35.9

37.9

Channel Containing Streamlined Forms Near Anseris Mons:   ESP_041972_1490   ESP_042117_1490   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-30.7

86.3

-8.6

5.165

52.1

53.5

Hydrated Materials within Orson Welles Crater:   ESP_041924_1790   ESP_052130_1790   (Interval in Earth days: 795)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-0.97

313.

-19.

7.429

39.3

47.1

Daedalia Planum Lava Flows:   ESP_041940_1570   ESP_042006_1570   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-22.7

237.

4.90

-18.3

46.0

48.4

Convoluted Folds in Light-Toned Deposits along Ius Chasma Floor:   ESP_041899_1725   ESP_042321_1725   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.47

275.

-0.2

-19.6

39.0

45.0

Winding Valley in Sinus Sabaeus Region:   ESP_041974_1740   ESP_042119_1740   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.17

27.5

3.38

18.36

39.2

39.5

Candidate Landing Site for 2020 Mission in Oxia Palus Region:   ESP_041989_1980   ESP_055175_1980   (Interval in Earth days: 1027)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.81

335.

-6.6

20.39

38.9

50.2

Daedalia Planum Lava Flows:   ESP_041861_1575   ESP_049509_1575   (Interval in Earth days: 596)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-22.3

234.

7.61

-4.70

44.4

30.8

Geologic Contact between Fluvial Deposits in Aeolis Dorsa:   ESP_041943_1745   ESP_050303_1745   (Interval in Earth days: 652)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.30

154.

-6.0

6.611

39.3

31.5


  


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