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.

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

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

A Snow Plow Landslide :   ESP_058960_1800   ESP_058894_1800   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-0.05

341.

-2.6

20.52

31.7

29.8

Gullied Crater Wall :   ESP_059242_1335   ESP_066983_1335   (Interval in Earth days: 603)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-46.1

208.

1.75

17.62

54.3

42.8

Layer Orientations Within Nia Tholus :   ESP_059384_1735   ESP_058883_1735   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.51

285.

15.9

-6.45

33.1

31.3

Well-Preserved Small Impact Crater on Hellas Planitia Floor :   ESP_059261_1380   ESP_067886_1380   (Interval in Earth days: 672)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-41.7

49.7

-4.4

21.24

51.7

52.2

Topographical Characterization of Russell Crater Dunes :   ESP_059302_1255   ESP_059236_1255   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-54.2

12.9

-6.3

8.33

62.0

60.1

Small Crater Northeast of Hellas Planitia :   ESP_059352_1515   ESP_059286_1515   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-28.3

83.6

-7.9

13.60

44.4

42.0

Impact Crater with Central Pit :   ESP_059263_1840   ESP_059408_1840   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
4.060

349.

-8.6

7.628

33.4

32.6


  


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