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.

Arsia Mons Reticulate Bedform Change Detection:   ESP_025760_1705   ESP_025483_1705   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-9.50

237.

-14.

10

55.4

51.5

Well Preserved 7-Kilometer Impact Crater in Utopia Planitia:   ESP_025791_1945   ESP_025646_1945   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
14.46

104.

24.6

6.969

40.6

41.4

Flow Draped over Crater Rim Visible in CTX Image :   ESP_025563_1975   ESP_025207_1975   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.48

209.

15.2

2.131

39.4

38.8

Light-Toned Material along Coprates Chasma Wallrock:   ESP_025718_1645   ESP_027696_1645   (Interval in Earth days: 154)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.5

303.

-0.2

13.09

58.0

60.8

Pit on Crater Floor with Layered Material:   ESP_025767_1515   ESP_034549_1515   (Interval in Earth days: 684)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-28.1

47.3

2.05

20.55

67.1

66.5

Coimbra Crater Interior Layering:   ESP_025571_1840   ESP_060410_1840   (Interval in Earth days: 2714)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
3.988

354.

-7.4

8.63

46.1

40.8

Crater and Fans Embayed by Flow Material in Kasei Valles:   ESP_025481_2025   ESP_033340_2025   (Interval in Earth days: 612)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
22.14

290.

-14.

-0.15

40.8

38.4

Channel in Tharsis Region:   ESP_025417_1965   ESP_024916_1965   (Interval in Earth days: 40)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
16.19

235.

17.6

-8.13

38.8

38.5

Crater Rim:   ESP_025631_1825   ESP_035969_1825   (Interval in Earth days: 806)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.346

156.

-6.2

5.312

47.2

53.4

Ring-Shaped Feature in Northeastern Acidalia Region:   ESP_025663_2280   ESP_026362_2280   (Interval in Earth days: 54)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
47.84

355.

4.36

-18.8

42.2

43.4


  


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