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.

Channel in Tharsis Region:   ESP_025417_1965   ESP_024916_1965   (Interval in Earth days: 40)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
16.19

235.

17.6

-8.13

38.8

38.5

Proposed Future Landing Site in Ladon Valles:   ESP_025295_1595   ESP_025783_1595   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-20.4

329.

22.4

-2.40

55.6

62.0

Strange Features in Hellas Basin:   ESP_025160_1445   ESP_042395_1445   (Interval in Earth days: 1343)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-35.2

58.5

10.2

-13.7

65.2

61.7

Stratified Material in Pit as Seen in CTX Image :   ESP_025259_1825   ESP_026881_1825   (Interval in Earth days: 127)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.450

231.

6.43

-8.79

43.3

52.6

Impact Crater with Central Pit on Floor of Larger Crater:   ESP_025240_1690   ESP_025728_1690   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-10.6

31.9

2.87

-23.9

50.1

56.6

Erosional Features Near Head of Grjota Valles:   ESP_025156_1965   ESP_025011_1965   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
16.14

161.

12.4

-2.60

37.9

38.5

Fluvial Fan on Crater Floor as Seen in THEMIS Image I03235002:   ESP_025309_2155   ESP_024887_2155   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
35.15

304.

-17.

-8.15

41.4

41.4

Exposed Bedrock on Western Side of 42-Kilometer Crater Central Uplift:   ESP_025304_1560   ESP_025027_1560   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-23.5

88.5

-22.

4.349

60.6

55.5

Mawrth Region Crater with Possible Sedimentary Features:   ESP_025123_2045   ESP_026811_2045   (Interval in Earth days: 131)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
24.24

340.

12.4

-19.9

37.4

44.7

Rampart of Flow Ejecta:   ESP_025260_1475   ESP_028293_1475   (Interval in Earth days: 237)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-32.3

209.

-5.1

5.684

65.2

67.7


  


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