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 Cone East of Pavonis Mons:   ESP_064673_1810   ESP_064818_1810   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
1.079

250.

8.69

27.00

57.2

55.9

Flow-Like Feature within Chryse Planitia:   ESP_064868_2005   ESP_064156_2005   (Interval in Earth days: 56)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
20.24

324.

13.0

-11.5

62.9

58.6

Sinuous Ridge Feature in CTX D21_035468_1545_XN_25S202W:   ESP_064716_1535   ESP_047534_1535   (Interval in Earth days: 1339)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-26.2

158.

26.4

2.235

55.6

47.5

Landform in CTX Image G03_019466_2032_XN_23N014W:   ESP_064709_2035   ESP_072979_2035   (Interval in Earth days: 644)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
23.38

345.

-4.9

6.945

64.2

58.2

Channels with Tributaries on Rocky Plains Northwest of Argyre Region:   ESP_064645_1320   ESP_082568_1320   (Interval in Earth days: 1397)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-47.5

301.

5.97

-6.62

63.9

60.6

Valleys in Central Pit of Crater:   ESP_064630_1525   ESP_073599_1525   (Interval in Earth days: 699)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.4

347.

8.33

-13.2

58.2

58.2

Nilosyrtis Mensae Dunes:   ESP_064495_2150   ESP_064561_2150   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
34.49

65.8

1.20

-15.4

65.4

67.6

Crater in Arabia Terra:   ESP_064207_2205   ESP_064062_2205   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
40.17

7.50

2.90

-7.96

63.3

62.0

Peace Vallis Channel in Gale Crater:   ESP_064453_1760   ESP_064730_1760   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.06

137.

3.20

-21.6

57.1

59.1

Intersecting Ridges on Fan-Shaped Deposit North of Arsia Mons:   ESP_064212_1765   ESP_064634_1765   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-3.59

237.

1.45

-9.52

57.1

58.1


  


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