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.

Valley along Noctis Labrynthus Floor:   ESP_017465_1730   ESP_017966_1730   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.16

261.

-10.

10.24

57.8

57.8

Pit Craters in North Polar Layered Deposit:   ESP_017376_2645   ESP_018918_2645   (Interval in Earth days: 120)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
84.39

134.

0.70

16.29

60.4

65.5

Possible Kieserite Deposit on Flanks of Hebes Mensa:   ESP_017319_1785   ESP_017385_1785   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.24

284.

10.7

-13.0

52.2

54.2

Well-Preserved 1-Kilometer Diameter Impact Crater on Northern Plains:   ESP_017480_2355   ESP_017968_2355   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
55.21

200.

6.86

-14.0

44.1

46.3

Central Uplift of a Northern Plains Impact Crater:   ESP_017453_2315   ESP_024969_2315   (Interval in Earth days: 586)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
51

220.

-6.6

9.417

43.9

46.9

Southern Gale Crater Strata with Possible Sulfates and Clays:   ESP_017364_1745   ESP_017509_1745   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.59

138.

-8.2

6.376

56.3

55.9

Cone with Lobate Flows in Hydraotes Chaos:   ESP_017634_1800   ESP_025493_1800   (Interval in Earth days: 612)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-0.10

326.

-12.

-26.9

54.3

49.1

Western Half of Fresh Crater on Alba Patera:   ESP_017571_2235   ESP_017861_2235   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
43.05

240.

-9.5

10.32

42.5

41.3

Thermally-Anomalous Crater on Hrad Vallis Flow:   ESP_017601_2145   ESP_018023_2145   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
34.20

141.

6.74

-6.84

40.9

43.0

Western Rim Well-Preserved 25-Kilometer Diameter Crater in Acidalia Region:   ESP_017370_2170   ESP_017871_2170   (Interval in Earth days: 40)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
36.52

329.

-8.4

6.007

41.9

41.5


  


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