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.

Collapsed Terrain in Osuga Valles Depression and Part of Relict Channel:   ESP_067678_1650   ESP_068008_1650   (Interval in Earth days: 26)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.8

322.

4.26

-24.2

39.6

45.2

Crater Fill Materials:   ESP_067663_1360   ESP_076631_1360   (Interval in Earth days: 699)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-43.7

15.7

4.85

-5.40

50.8

51.6

Searching for Slope Features:   ESP_067410_1515   ESP_076853_1515   (Interval in Earth days: 735)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-28.1

76.1

5.88

-23.1

40.2

47.0

Gullies Mantling and Glaciers near Dao Vallis:   ESP_067581_1440   ESP_067713_1440   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-35.6

91.8

4.62

-9.42

45.3

48.1

Outcrops of Fluvial Deposits in Mesa Flank:   ESP_067605_1760   ESP_066510_1760   (Interval in Earth days: 86)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-3.80

152.

5.52

-6.48

38.9

45.6

Layering in Arabia Terra:   ESP_067505_1845   ESP_067637_1845   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
4.307

-0.0

8.59

-8.44

40.6

41.6

A Technicolor Mound near Oxia Planum:   ESP_066622_2000   ESP_074430_2000   (Interval in Earth days: 608)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
19.88

332.

5.69

22.84

57.4

63.3

Crater near Dao Vallis:   ESP_067040_1440   ESP_066209_1440   (Interval in Earth days: 65)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-35.8

93.1

3.28

-19.1

40.0

43.0

Valleys in Crater Northeast of Argyre Region:   ESP_067229_1500   ESP_067361_1500   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-29.7

334.

7.83

-10.6

39.0

41.4

South Polar Layered Deposits:   ESP_067270_0910   ESP_067124_0910   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-89.0

-2.7

24.9

27.39

75.7

73.1


  


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