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 Rocks of Ophir Mensa:   ESP_034738_1760   ESP_034949_1760   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-3.81

285.

-3.5

-14.7

53.5

55.5

Lava-Ejecta Interaction in Cerberus Region:   ESP_034664_1865   ESP_034954_1865   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
6.328

144.

7.04

29.64

46.9

46.6

Domoni Crater Secondaries:   ESP_034845_2305   ESP_035280_2305   (Interval in Earth days: 34)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
50.02

236.

-1.8

22.27

43.3

41.1

Fan-Shaped Landform at Valley Terminus in Lyot Crater:   ESP_034813_2315   ESP_061912_2315   (Interval in Earth days: 2111)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
50.94

31.0

-5.0

-24.6

43.9

45.0

Tributary of Mamers Valles:   ESP_034695_2175   ESP_034972_2175   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
37.10

15.0

-5.1

-28.5

41.4

43.9

Crater within Kasei Valles:   ESP_034830_2025   ESP_036241_2025   (Interval in Earth days: 110)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
22.14

290.

3.80

-7.00

42.2

47.6

Fan and Channel Forms in Memnonia Sulci Region:   ESP_034768_1695   ESP_035757_1695   (Interval in Earth days: 77)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-10.5

186.

6.76

-7.65

57.1

61.5

Crater with Light and Dark Layers Exposed in Walls:   ESP_034733_1675   ESP_035023_1675   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-12.4

63.9

-7.9

19.17

59.0

59.1

Change Detection in Chain of Small Pits North of Alba Patera:   ESP_034699_2310   ESP_034831_2310   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
50.52

263.

-1.2

-27.3

43.6

45.8

Lava Flow North of Ascraeus Mons:   ESP_034739_1975   ESP_035240_1975   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.37

255.

-1.0

16.11

43.6

44.0


  


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