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 on North Rim of Baldet Crater :   ESP_029498_2045   ESP_031845_2045   (Interval in Earth days: 182)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
24.22

65.7

-9.2

4.698

62.7

50.9

Well Preserved 2-Kilometer Impact Crater :   ESP_029418_1600   ESP_030130_1600   (Interval in Earth days: 56)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-19.9

94.4

3.58

14.65

54.1

46.6

Well-Preserved 15-Kilometer Diameter Crater Near Alba Mons :   ESP_029729_2195   ESP_020894_2195   (Interval in Earth days: 689)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
39.07

238.

-22.

-9.47

73.1

72.1

Dunes on Slope in CTX :   ESP_029504_1745   ESP_046963_1745   (Interval in Earth days: 1360)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.26

265.

-6.8

4.182

54.4

51.1

Sub-Chryse Planitia Layering in Cairns Crater Near Viking 1 Site :   ESP_029634_2040   ESP_030412_2040   (Interval in Earth days: 61)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
23.55

312.

-7.6

-20.0

63.3

66.0

Distal End of Lobe on Floor of Unnamed Crater in Northern Terra Sabaea :   ESP_029406_2060   ESP_030118_2060   (Interval in Earth days: 56)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
25.84

56.8

-2.5

7.181

62.0

65.7

Gullies on Two Sides of Mound in Nereidum Montes :   ESP_029436_1355   ESP_047528_1355   (Interval in Earth days: 1409)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-44.1

326.

4.50

-13.2

59.8

52.2

Streamlined Forms in Shalbatana Vallis :   ESP_029502_1945   ESP_029647_1945   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
14.57

317.

-7.8

5.518

59.0

58.7

Fan at Terminus of Meandered Ridge in Reuyl Crater :   ESP_029679_1700   ESP_030101_1700   (Interval in Earth days: 32)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-9.84

166.

8.05

-7.77

52.1

50.5

Merging Channels in Harmakhis Vallis :   ESP_029471_1375   ESP_030104_1375   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-41.9

90.1

6.19

-13.6

58.4

50.4


  


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