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.

Bedrock in Northeast Syrtis Major Region:   ESP_078712_1980   ESP_087494_1975   (Interval in Earth days: 684)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.48

77.2

26.2

-10.1

43.1

45.3

Overprinting Rampart Crater Ejecta:   ESP_078678_1875   ESP_077465_1875   (Interval in Earth days: 94)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.652

287.

17.3

6.161

47.5

39.7

Well-Preserved 9-Kilometer Impact Crater:   ESP_078821_1740   ESP_079243_1740   (Interval in Earth days: 32)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.81

346.

5.18

-7.41

56.3

59.3

Bright and Round Deposit in Eos Chasma:   ESP_078888_1665   ESP_079244_1665   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.1

319.

-8.5

2.452

62.1

63.3

Partial Icy Fill of Impact Crater onto Graben:   ESP_078679_2170   ESP_078824_2170   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
36.46

258.

-6.1

5.368

43.4

42.5

Hydrae Cavus:   ESP_078625_1720   ESP_079337_1720   (Interval in Earth days: 56)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.03

298.

-4.1

16.02

56.8

59.5

Terra Cimmeria Dune Monitoring :   ESP_078934_1655   ESP_078868_1655   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.4

142.

2.23

24.21

62.5

60.7

Dune Monitoring in Northern Mid-Latitude Crater:   ESP_078674_2295   ESP_078595_2295   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
49.27

30.2

16.0

-5.49

43.8

45.8

Sedimentary Layers in Hebes Chasma:   ESP_078942_1795   ESP_079298_1795   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-0.55

282.

4.64

16.17

54.0

54.8

Terrain Sample near Jezero Crater:   ESP_078844_1980   ESP_078989_1980   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.61

76.4

-6.5

8.294

46.4

45.7


  


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