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.

Small Lava Flows Emanating From the Cerberus Fossae:   PSP_007197_1910   PSP_008199_1910   (Interval in Earth days: 78)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
10.63

156.

5.84

-4.05

39.2

46.5

Dark Dunes Over Light-Toned Mega-Ripples Seen in MOC Image SP1-26004:   PSP_007532_1905   PSP_008679_1905   (Interval in Earth days: 89)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
10.61

9.06

2.36

-9.87

41.8

49.2

Recent Crater:   PSP_007750_1900   ESP_051001_1895   (Interval in Earth days: 3370)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.637

176.

5.67

-4.50

43.3

35.5

Upper Section of Northern Olympus Mons Basal Scarp:   PSP_007445_2035   PSP_008447_2035   (Interval in Earth days: 78)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
22.90

223.

-1.4

-13.8

40.1

44.4

Fresh 10-Kilometer Diameter Unnamed Crater in Terra Sabaea:   PSP_007966_1615   ESP_025055_1615   (Interval in Earth days: 1331)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-18.1

41.5

5.02

25.73

59.9

51.0

Ridges and Mounds Near Hecates Tholus:   PSP_007672_2155   PSP_007883_2155   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
34.92

142.

6.64

-7.98

40.8

42.0

Gullies:   PSP_007456_2140   ESP_016040_2140   (Interval in Earth days: 669)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
33.74

281.

-4.6

-22.7

41.7

43.6

Lobate Debris Aprons with Ridge-Like Structures:   PSP_007693_2300   PSP_008550_2300   (Interval in Earth days: 67)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
49.57

286.

6.42

-7.47

45.2

44.0

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

Central Peak of Large 40-Kilometer Diameter Crater:   PSP_007592_1995   ESP_045595_1995   (Interval in Earth days: 2961)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
19.25

169.

-0.9

19.06

40.8

43.5


  


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