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.

Mound with Linear Depression at Summit in Center of Crater:   ESP_026042_2020   ESP_028574_2020   (Interval in Earth days: 198)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
21.91

93.1

2.80

-9.54

41.2

53.6

Small Fresh Crater on Northern Plains:   ESP_026076_2320   ESP_026419_2320   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
51.66

236.

24.6

-3.11

40.7

42.9

Newton Crater Valleys and Alluvial Fans:   ESP_026012_1410   ESP_026078_1410   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-38.7

199.

4.09

-15.0

76.7

78.1

Layered Light-Toned Rounded Blocks in Melas Chasma:   ESP_025811_1700   ESP_026312_1700   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-10.2

284.

-7.9

16.99

55.8

57.1

Valleys on Northern Flank of Hecates Tholus:   ESP_026119_2135   ESP_026185_2135   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
32.93

150.

-2.5

-20.0

40.2

41.9

Well-Preserved Impact Crater on Floor of Coprates Chasma:   ESP_025982_1675   ESP_025626_1675   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-12.3

294.

14.8

0

56.9

55.1

Streamlined Forms in Elysium Planitia:   ESP_025802_1960   ESP_026435_1960   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
15.72

165.

7.87

-11.1

41.7

45.6

Flow Margin Visible in Viking Image 731A38:   ESP_026077_1770   ESP_027554_1770   (Interval in Earth days: 115)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-2.80

221.

-3.8

-24.4

52.7

56.8

Fresh Crater:   ESP_025888_2365   ESP_025664_2365   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
56.40

327.

28.0

1.477

42.8

46.0

Streamlined Layered Forms in Athabasca Valles:   ESP_026198_1895   ESP_027042_1895   (Interval in Earth days: 66)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.217

156.

-0.7

-17.9

46.7

50.2


  


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