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.

Inverted Terrain in the Mawrth Vallis Region:   ESP_013084_2060   ESP_013361_2060   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
25.90

341.

0.94

-25.7

66.4

65.7

Central Uplift of an Impact Crater in Hesperia Planum:   ESP_013211_1675   ESP_013633_1675   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-12.4

118.

8.88

-5.92

42.9

39.0

South Polar Layered Deposits Exposed in Promethei Lingula:   ESP_013714_0970   ESP_013687_0970   (Interval in Earth days: 3)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-82.8

116.

-28.

-8.52

66.4

64.2

Layers in Crater Near West Rim of Gale Crater:   ESP_013329_1745   ESP_031025_1745   (Interval in Earth days: 1378)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.44

136.

2.91

20.54

44.8

40.9

Incipient Scalloped Terrain in Mid-Latitude Mantle at Peneus Patera:   ESP_013029_1235   ESP_013306_1235   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-56.1

54.6

-0.3

-19.2

47.7

46.9

Lava Flow Margin in Echus Chasma:   ESP_013271_1810   ESP_013693_1810   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
1.211

279.

2.08

-12.7

48.9

44.8

Gullies in Gorgonum Chaos Mesas:   ESP_012747_1425   ESP_013024_1425   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-37.0

189.

2.86

-20.5

46.1

44.2

Terby Crater Surroundings:   ESP_013885_1520   ESP_020465_1520   (Interval in Earth days: 513)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.9

79.1

4.84

-7.13

34.3

58.0

Gullies and Lobate Material in a Crater in the Nereidum Montes:   ESP_014127_1420   ESP_020786_1420   (Interval in Earth days: 519)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-37.5

314.

-2.1

19.93

37.6

54.3

Light-Toned Outcrop in Lower Coprates Chasma Wall:   ESP_013231_1690   ESP_013732_1690   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-10.9

292.

1.57

23.81

43.7

36.2


  


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