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.

Region adjacent to Zhurong Rover Landing Site:   ESP_080201_2055   ESP_080346_2055   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
25.18

109.

-0.3

20.25

48.1

46.9

Dune Ice Interaction West of Olympia Region:   ESP_080570_2605   ESP_080333_2605   (Interval in Earth days: 19)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
80.45

96.7

2.25

-15.3

63.1

62.0

Light-Toned Exposures near Voeykov Crater:   ESP_080340_1465   ESP_080274_1465   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-33.0

283.

-1.3

15.81

77.0

76.2

Lava Filling Craters in Elysium Planitia:   ESP_080529_1895   ESP_080674_1895   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.230

159.

-7.8

3.279

54.3

53.7

Ares Vallis:   ESP_080549_1910   ESP_080760_1910   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
10.87

332.

2.57

-10.1

53.0

54.5

Frost-Free Dunes in Viking 2 Image 544B05:   ESP_080437_2570   ESP_080490_2570   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
76.66

130.

7.66

-7.69

59.3

61.0

Dune Monitoring in Northern Mid-Latitude Crater:   ESP_080539_2425   ESP_080618_2425   (Interval in Earth days: 7)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
62.07

238.

-7.6

7.316

55.0

54.6

Dune Monitoring in Northern Mid-Latitude Crater:   ESP_080576_2395   ESP_080286_2395   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
59.33

302.

24.5

7.497

51.7

50.5

Landslide near Kasei Valles:   ESP_080273_2085   ESP_079996_2085   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
28.13

303.

5.79

17.72

47.4

45.1

Athabasca Valles:   ESP_080450_1890   ESP_080951_1890   (Interval in Earth days: 40)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.124

155.

-7.0

8.08

54.1

54.1


  


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