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.

Light-Toned Outcrops in Iani Chaos:   ESP_016328_1760   ESP_016473_1760   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-3.82

341.

1.72

18.56

46.9

47.0

Cratered Mounds in Galaxias Colles:   ESP_016691_2175   ESP_018260_2175   (Interval in Earth days: 122)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
37.23

146.

0

27.19

41.3

40.5

Geologic Contact Between Landslides and Blocky Deposit on Floor of Melas Ch:   ESP_016739_1715   ESP_018941_1715   (Interval in Earth days: 172)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.58

282.

-8.3

8.612

54.0

57.9

Ridges and Fill Material Among Knobs on West Flank of Arsia Mons:   ESP_016833_1715   ESP_019035_1715   (Interval in Earth days: 171)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.53

235.

-1.7

13.23

54.3

57.3

Aram Chaos Mineralogical Variability:   ESP_016605_1830   ESP_086812_1830   (Interval in Earth days: 5470)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.889

339.

-8.3

-23.3

46.9

47.0

Olivine-Rich Terrain in Yuty Crater:   ESP_016579_2025   ESP_017647_2025   (Interval in Earth days: 83)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
22.08

325.

1.00

18.99

40.6

42.1

Crater with Lineated Material on Floor:   ESP_016824_1465   ESP_016969_1465   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-33.2

124.

-2.9

10.86

71.0

71.5

Terrain South of Newcomb Crater:   ESP_016736_1520   ESP_068970_1525   (Interval in Earth days: 4070)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.6

5.59

4.65

-7.50

65.7

63.9

25-Kilometer Diameter Gullied Impact Crater in Acidalia Planitia:   ESP_016592_2170   ESP_016737_2170   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
36.54

329.

-3.7

9.38

41.6

40.3

Pits along the Claritas Rupes:   ESP_016450_1570   ESP_016516_1570   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-22.5

252.

7.58

-14.9

58.8

60.8


  


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