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.

Polar Layered Deposits Unconformity:   PSP_010048_2615   PSP_010509_2615   (Interval in Earth days: 36)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
81.49

49.1

-3.5

16.55

63.8

68.5

Exposure of North Polar Layered Deposits:   PSP_009967_2660   PSP_009980_2660   (Interval in Earth days: 1)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
85.86

102.

-16.

-13.4

66.5

66.4

High-Latitude Exposure of North Polar Layered Deposits:   PSP_010130_2675   PSP_010263_2675   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
87.47

297.

-7.6

-19.1

68.9

70.9

Stratigraphy Exposed in Ausonia Cavus:   PSP_009889_1480   ESP_079872_1480   (Interval in Earth days: 5452)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-31.7

96.8

-1.5

12.44

74.4

76.4

Rayed Crater on Southeast Flank of Elysium Mons:   PSP_009333_2025   PSP_009834_2025   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
22.46

151.

-21.

-0.87

47.7

47.8

Fluvial and Alluvial Features on North Wall of Eos Chasma:   PSP_009894_1665   PSP_010606_1665   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.3

317.

3.44

21.18

62.6

59.5

Sapping Features East of Tooting Crater:   PSP_010333_2025   PSP_010689_2025   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
22.14

208.

-3.9

0.754

50.8

53.1

Mounds in Ulysses Fossae:   PSP_009409_1860   PSP_009554_1860   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
5.804

237.

-7.2

8.646

53.1

52.1

Look for Change Due to Mass Wasting on Scarps of Different Slopes:   PSP_009408_2640   PSP_009882_2640   (Interval in Earth days: 37)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
84.00

230.

0.72

16.89

60.3

62.9

Gullies in North Mid-Latitude Crater:   PSP_009744_2305   PSP_010245_2305   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
50.11

84.3

-0.6

14.78

47.4

50.9


  


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