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.

Enigmatic Pits in Southern Elysium Planitia:   ESP_017284_1790   ESP_017429_1790   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.07

160.

5.24

19.21

52.3

52.0

Well-Preserved 4-Kilometer Diameter Impact Crater in Elysium Region:   ESP_017153_1830   ESP_017298_1830   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.912

138.

-13.

1.198

50.8

50.5

Possible Cone Field in Phlegra Dorsa:   ESP_017178_2065   ESP_017679_2065   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
26.35

172.

-7.6

8.46

42.3

42.0

Gullies with Bright Deposits in Poynting Crater:   ESP_017149_1890   ESP_017294_1890   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.768

246.

-12.

2.349

47.9

47.5

Nili Patera:   ESP_016905_1890   ESP_035181_1890   (Interval in Earth days: 1424)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.910

67.6

0

17.66

45.7

47.4

Rocky Hill:   ESP_016922_1615   ESP_017423_1615   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-18.5

326.

5.41

22.56

61.0

63.1

Distal Edge of Flow from Galaxias Fossae:   ESP_017179_2175   ESP_017245_2175   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
37.16

142.

6.93

-10.3

40.5

42.0

Well-Preserved Mid-Latitude Crater:   ESP_016981_2210   ESP_017482_2210   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
40.75

149.

-6.3

6.555

42.1

40.9

Intersecting Graben in Ulysses Fossae:   ESP_017268_1915   ESP_017413_1915   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
11.38

237.

-11.

3.258

47.2

46.7

Possible Al-Clay near Columbus Crater:   ESP_017138_1525   ESP_053585_1520   (Interval in Earth days: 2840)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.2

191.

-6.9

3.289

69.4

69.5


  


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