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.

Central Peak and Pit of Large Impact Crater:   PSP_007027_1570   ESP_023905_1570   (Interval in Earth days: 1315)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-22.9

122.

4.75

-19.6

51.3

40.6

Granicus Valles Subchannel Breakout From Main Channel:   PSP_007725_2075   PSP_007936_2075   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
27.11

136.

7.86

-8.35

40.0

41.8

Well-Exposed Scarp of Noachian Phyllosilicates Along Nili Fossae:   PSP_007200_2005   ESP_016153_2005   (Interval in Earth days: 698)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
20.03

73.6

1.53

26.79

39.1

37.1

Nili Fossae Crater Rim:   PSP_007438_2000   ESP_069113_2000   (Interval in Earth days: 4805)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
19.95

55.0

-1.8

15.09

40.2

45.7

Alluvial Fan Apex in Saheki Crater:   PSP_007543_1580   PSP_007899_1580   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-21.7

72.5

3.97

-8.11

57.6

62.4

Layered Bedrock Exposed in Central Uplift of Crater in Thaumasia Planum:   PSP_007113_1595   PSP_007469_1595   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-20.3

293.

4.00

-7.61

50.9

56.5

Possible Sulfates in Ius Chasma:   PSP_007509_1720   ESP_050839_1720   (Interval in Earth days: 3376)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.70

279.

-2.3

13.43

49.3

36.5

Terraced Fan Deposit in Tyras Vallis:   PSP_008167_1885   PSP_008602_1885   (Interval in Earth days: 34)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.358

310.

-1.6

10.76

47.1

48.3

Putative Salt Deposits Detected by THEMIS West of Meridiani Region:   PSP_007981_1770   PSP_008851_1770   (Interval in Earth days: 68)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-3.06

350.

-5.6

23.21

51.6

54.5

Ganges Mensa:   PSP_007521_1725   PSP_007877_1725   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.23

311.

7.88

-4.81

48.5

53.0


  


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