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.

Yardangs in Aeolis Region:   ESP_082204_1800   ESP_082336_1800   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-0.07

151.

6.30

-25.1

57.9

60.5

Lava Interactions with Landscape:   ESP_082228_1545   ESP_082663_1545   (Interval in Earth days: 34)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-25.2

221.

-7.6

21.04

60.0

53.2

Chryse Chaos:   ESP_082290_1885   ESP_082356_1885   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.575

323.

8.00

-7.61

59.2

60.6

Cones:   ESP_082416_2015   ESP_082139_2015   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
21.13

123.

-4.7

6.682

64.5

61.5

Ridges in Meridiani Planum:   ESP_082289_1805   ESP_082355_1805   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
0.516

351.

8.46

-7.68

57.8

59.0

Lava-Coated Crater near Kasei Valles:   ESP_082265_1960   ESP_082555_1960   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
15.66

285.

1.99

21.45

61.3

61.1

Volcanic Vent East of Pavonis Mons:   ESP_082174_1795   ESP_082240_1795   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-0.46

251.

-3.3

-20.3

58.6

60.0

Hillslope Morphologies in Crater:   ESP_082342_1655   ESP_090372_1655   (Interval in Earth days: 626)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.4

347.

3.30

-13.1

57.2

61.3

Lava-Topography Interactions:   ESP_082294_1535   ESP_082162_1535   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-26.4

221.

-23.

8.101

60.8

59.7

Partly-Filled Impact Crater near Nicholson Crater:   ESP_082176_1830   ESP_082242_1830   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.848

196.

-7.6

-23.2

59.3

60.7


  


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