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.

Valleys and Channels in Parana Valles:   ESP_082632_1560   ESP_082922_1560   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-23.6

349.

-5.8

5.35

55.6

51.4

Possible Spatter Cones East of Arsia Mons:   ESP_082873_1715   ESP_083440_1715   (Interval in Earth days: 44)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.45

246.

-0.0

0.453

54.6

49.4

Resistant Layer in Medusae Fossae Formation:   ESP_082729_1830   ESP_083230_1830   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.727

217.

-6.6

0.505

58.9

56.0

Intracrater Landslide South of Pyrrhae Chaos:   ESP_082646_1485   ESP_082936_1485   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-31.3

328.

-2.5

8.715

55.7

51.0

Layered Deposits in Liais Crater:   ESP_082694_1045   ESP_082681_1045   (Interval in Earth days: 1)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-75.4

106.

8.06

-8.39

68.8

70.2

Crater in Galle Crater:   ESP_082712_1290   ESP_082778_1290   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-50.5

329.

-5.6

-23.2

59.1

59.4

Graben-Crater Intersection at Tantalus Fossae:   ESP_082648_2260   ESP_082727_2260   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
45.90

262.

7.49

26.08

77.2

76.6

Small Scale Channels near Central Pit in Terra Cimmeria:   ESP_082521_1440   ESP_083444_1440   (Interval in Earth days: 72)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-35.9

142.

-6.0

-22.2

58.3

46.5

Flow Features on Ice-Rich Plateau on Malea Patera:   ESP_082854_1165   ESP_082775_1165   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-63.1

53.2

5.61

-11.0

60.5

63.1

Exposed Crater Floor Materials in Western Arabia Terra:   ESP_082552_1835   ESP_090648_1835   (Interval in Earth days: 631)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
3.618

10.1

7.89

-24.4

58.3

59.1


  


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