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.

Boulders inside of Pits on a Mesa:   ESP_037747_1810   ESP_073986_1810   (Interval in Earth days: 2824)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
1.014

217.

-6.3

20.01

57.1

55.5

Possible Yardangs:   ESP_037683_1570   ESP_046637_1570   (Interval in Earth days: 698)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-22.6

167.

0

11.53

61.1

54.5

InSight Mission Candidate Landing Site:   ESP_037961_1845   ESP_038449_1845   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
4.572

135.

-11.

0.843

58.1

58.0

Candidate Landing Site for 2020 Mission Near Nili Fossae:   ESP_037673_2015   ESP_037739_2015   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
21.14

74.1

4.25

-14.2

56.9

59.0

Extensive Raised Ridges in Eridania Region:   ESP_037788_1495   ESP_046109_1495   (Interval in Earth days: 649)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-30.3

181.

4.59

28.59

62.4

60.9

Crater Adjacent to Lunae Mensa Scarp:   ESP_037678_2045   ESP_037823_2045   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
24.07

298.

-8.1

11.1

58.5

58.4

Daedalia Planum Lava Flow:   ESP_037615_1455   ESP_046002_1455   (Interval in Earth days: 653)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-34.3

224.

6.44

18.30

65.6

65.0

Herschel Crater Dunes Change Detection:   ESP_037948_1645   ESP_038291_1645   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.1

131.

3.51

-24.6

57.5

58.0

Meridiani Planum Stratigraphy:   ESP_037676_1840   ESP_037953_1840   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
4.078

354.

7.34

-10.4

55.7

57.9

Candidate ExoMars Landing Site Near Hypanis Valles:   ESP_037717_1920   ESP_037651_1920   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
11.73

314.

2.17

21.01

56.4

54.4


  


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