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.

Collapse Features on Hrad Vallis Mudflow:   ESP_016467_2155   ESP_016533_2155   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
35.13

141.

0.42

-15.9

41.1

42.4

Layered Walls of Impact Crater in Mawrth Vallis Outcrops:   ESP_016895_2045   ESP_017040_2045   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
23.95

339.

-3.5

8.322

41.6

41.0

Source Region for Branch of Auqakuh Vallis:   ESP_016826_2080   ESP_016971_2080   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
27.47

62.7

-7.7

5.246

41.4

40.6

Small Volcano in Northern Syria Planum:   ESP_016318_1710   ESP_016951_1710   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.76

254.

6.70

-9.92

48.9

55.9

Large-Scale Slumping in Moreux Crater:   ESP_016642_2215   ESP_017710_2215   (Interval in Earth days: 83)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
41.13

44.1

-7.3

6.121

42.8

41.2

Aureum Chaos:   ESP_016803_1770   ESP_088144_1770   (Interval in Earth days: 5559)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-3.11

334.

-3.6

-16.2

51.1

57.8

Pits along the Claritas Rupes:   ESP_016450_1570   ESP_016516_1570   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-22.5

252.

7.58

-14.9

58.8

60.8

Gordii Dorsum:   ESP_016847_1910   ESP_017559_1910   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
10.61

211.

-2.9

6.107

44.9

47.3

Candidate MSL Landing Site in Northeast Syrtis Major:   ESP_016720_1980   ESP_016786_1980   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.78

76.9

2.08

-17.9

41.7

43.6

Very Recent Small Impact Crater:   ESP_016630_1720   ESP_030291_1720   (Interval in Earth days: 1064)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.08

17.6

-3.5

8.058

52.4

48.4


  


Page 692 of 878 (8,772 images)