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.

Test Erosion Mechanisms at Exit Channel Upstream of Jezero Crater :   ESP_059563_1995   ESP_067687_1995   (Interval in Earth days: 633)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
19.20

75.7

7.00

-27.8

35.5

48.5

Well-Preserved Impact Crater :   ESP_059565_1375   ESP_076393_1375   (Interval in Earth days: 1311)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-42.1

30.0

-2.2

8.829

57.1

46.1

Terrain in Utopia Planitia :   ESP_059760_2120   ESP_060182_2120   (Interval in Earth days: 32)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
31.46

96.8

-2.6

-7.88

40.3

39.4

Eastern Rim of Noord Crater :   ESP_059751_1605   ESP_060107_1605   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-19.3

348.

-1.0

13.60

44.7

49.0

Valleys in Crater Northeast of Argyre Planitia :   ESP_059501_1500   ESP_060134_1500   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-29.6

335.

1.19

-10.1

47.0

57.7

Noachis Terra Sand Dune Topography :   ESP_059619_1400   ESP_059975_1400   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-39.5

355.

-2.5

8.852

56.1

61.3

Mass Wasting Feature on Southern Wall of Crater Near Amazonis Mensa :   ESP_059611_1860   ESP_060244_1860   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
5.755

207.

5.84

-4.61

33.9

39.7

Small Gullies and Fans along Ridge in Nereidum Montes :   ESP_059647_1360   ESP_059502_1360   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-43.9

309.

20.8

8.562

58.6

56.8

Scarps in Icaria Region :   ESP_059716_1425   ESP_059993_1425   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-37.1

227.

-3.5

-24.4

56.1

61.8

Possible Phyllosilicate-Rich Stratigraphy in Western Mawrth Vallis:   ESP_059738_2050   ESP_060094_2050   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
24.53

338.

-7.4

5.422

38.1

36.8


  


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