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.

Inverted Channel in Noachis Terra:   ESP_086639_1610   ESP_086850_1610   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-18.8

22.5

7.49

-2.17

53.4

56.7

Layering in Arabia Terra:   ESP_086653_1825   ESP_087286_1825   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.399

358.

-5.2

-24.6

44.3

51.0

Sulfate-Rich Terrain in Aureum Chaos:   ESP_086799_1760   ESP_086654_1760   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-3.91

332.

2.44

-11.8

47.6

47.2

Area near Viking 1 Landing Site:   ESP_086681_2025   ESP_087182_2025   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
22.26

311.

-7.0

14.31

41.5

41.1

North-Pole-Facing Deposit in Crater Associated with Headwall Erosion:   ESP_086671_2205   ESP_087093_2205   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
40.33

220.

6.96

-3.98

44.2

43.7

Alluvial Fans in Kasei Valles:   ESP_086774_2035   ESP_085851_2035   (Interval in Earth days: 72)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
23.07

294.

-22.

4.013

43.1

41.4

Fissure and Channel near Pavonis Mons:   ESP_086723_1775   ESP_086868_1775   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-2.46

247.

-0.2

15.12

46.4

46.7

North Mid-Latitude Dune Field Topography:   ESP_086760_2420   ESP_087195_2420   (Interval in Earth days: 34)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
61.54

308.

-2.2

17.53

54.7

49.8

Small Impact Craters in Aeolis Dorsa:   ESP_086766_1740   ESP_085975_1740   (Interval in Earth days: 62)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.04

153.

2.85

-21.3

48.2

41.6

North-Pole-Facing Deposit in Crater:   ESP_086710_2235   ESP_086789_2235   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
42.99

237.

-6.3

18.84

46.0

43.6


  


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