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.

Channels near Osuga Valles:   ESP_089041_1635   ESP_089463_1635   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-16.2

319.

29.7

15.43

63.4

63.3

Chryse Chaos:   ESP_089120_1850   ESP_089265_1850   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
5.033

322.

3.73

17.70

53.5

52.6

Kasei Valles Alluvial Fans and Terraced Scarps:   ESP_089042_2025   ESP_088765_2025   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
22.38

291.

-8.7

22.53

48.3

44.7

Test for Inverted Channel near Intersection with Crater:   ESP_088921_1875   ESP_089066_1875   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.249

356.

-5.0

8.307

53.0

52.2

Terrain Features around Crater in Arabia Terra:   ESP_088875_2215   ESP_088585_2215   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
41.06

167.

2.85

-12.9

44.9

45.1

Gypsum Dunes and Basal Unit Contact:   ESP_089030_2605   ESP_088911_2605   (Interval in Earth days: 9)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
80.49

242.

-7.7

7.217

60.3

58.6

Alluvial Fan and Light-Toned Deposits in Coprates Catena Trough:   ESP_089187_1655   ESP_089121_1655   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.1

297.

-21.

2.298

65.3

63.9

Depression in Nepenthes Mensae:   ESP_088956_1935   ESP_089167_1935   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
13.27

119.

1.73

-7.93

50.0

51.2

Ismenius Cavus Channel:   ESP_088986_2140   ESP_089131_2140   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
33.50

17.7

2.34

12.95

45.5

45.3

Flow Entering Fretted Terrain Valley:   ESP_089025_2170   ESP_089091_2170   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
36.42

31.9

6.73

-11.0

45.2

47.2


  


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