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.

Layered Mound near Mawrth Vallis:   ESP_090359_2045   ESP_090425_2045   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
24.02

335.

8.76

-7.68

55.6

57.6

Morphologically Fresh Incision in Potentially Ice-Rich Mantling Deposit:   ESP_090370_2225   ESP_090436_2225   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
41.91

34.0

-3.7

-16.2

60.6

62.6

Flow Obstacle in Lobate Debris Apron:   ESP_090608_2215   ESP_090107_2215   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
40.89

11.8

27.4

9.221

61.0

55.7

Vent East of Ascraeus Mons:   ESP_090375_1925   ESP_090520_1925   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
12.13

261.

-5.8

10.07

56.2

55.7

Monitor Changes in Intracrater Mounds:   ESP_090444_2195   ESP_090378_2195   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
39.18

175.

-8.2

5.181

61.3

59.2

Terrain around Crater in Terra Sabaea:   ESP_090409_2165   ESP_090132_2165   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
36.18

50.6

-6.7

5.045

59.7

55.3

An Inverted Channel in Flammarion Crater:   ESP_089631_2065   ESP_090330_2065   (Interval in Earth days: 54)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
26.02

48.9

5.65

-12.0

49.6

57.2

Deep in Valles Marineris:   ESP_089134_1655   ESP_088633_1655   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.3

303.

-5.3

-18.1

64.4

65.7

Terrain Northeast of Chryse Planitia:   ESP_090214_2200   ESP_090491_2200   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
39.48

332.

-3.6

-16.1

57.8

62.7

Mottled Ridged Terrain:   ESP_090266_1840   ESP_090688_1840   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
3.703

357.

-1.8

-24.6

56.2

59.2


  


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