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.

Well-Preserved 8-Kilometer Diameter Impact Crater:   ESP_034987_2020   ESP_035620_2020   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
21.60

324.

-2.8

-21.0

43.4

46.9

Athabasca Valles Distributary Channel:   ESP_035191_1880   ESP_036457_1880   (Interval in Earth days: 99)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.051

155.

6.56

-7.04

48.6

52.4

Discontinuous Sinuous Ridge North of Hellas Region:   ESP_035036_1560   ESP_035880_1560   (Interval in Earth days: 66)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-23.8

72.0

-0.6

-22.0

68.1

71.1

Ridge Changing into Trough in Utopia Planitia:   ESP_035153_2085   ESP_053825_2085   (Interval in Earth days: 1455)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
28.26

111.

-5.7

4.001

42.7

42.3

Candidate Future Landing Site:   ESP_035052_1795   ESP_037241_1795   (Interval in Earth days: 171)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-0.62

351.

7.41

-14.3

52.7

57.2

Crater with Steep Slopes:   ESP_035246_2105   ESP_035879_2105   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
30.23

91.0

6.44

-5.33

41.5

44.5

Northern Plains Crater Morphology:   ESP_035017_2315   ESP_035096_2315   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
51.06

220.

-0.2

20.09

43.4

41.5

Domoni Crater Secondaries:   ESP_035056_2310   ESP_035188_2310   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
50.65

235.

-0.7

-25.8

43.2

45.6

Flow Feature West of Meridiani Planum:   ESP_034973_1780   ESP_035118_1780   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.95

349.

-5.9

8.914

53.9

53.6

Young 10-Kilometer Diameter Crater:   ESP_035075_2010   ESP_035365_2010   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
20.77

82.2

-6.8

20.14

44.2

42.9


  


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