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.

Light-Toned Possible Fans at Base of Crater Wall:   ESP_031127_1500   ESP_075647_1500   (Interval in Earth days: 3469)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-29.6

236.

2.27

-8.59

35.1

36.3

Possible Fluvial Features in Golden Crater:   ESP_031005_1575   ESP_039405_1575   (Interval in Earth days: 654)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-22.0

326.

-5.8

8.33

37.4

43.5

Reull Vallis and Tongue-Shaped Landform in the Centauri Montes:   ESP_031119_1405   ESP_031264_1405   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-39.0

97.1

-11.

2.562

37.6

35.9

Flows Associated with Mojave Crater Secondaries:   ESP_031229_1895   ESP_040196_1895   (Interval in Earth days: 699)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.550

326.

1.62

22.38

48.5

46.8

Possible Preserved Impact Melt Flow on the Ejecta of Bakhuysen Crater:   ESP_031201_1555   ESP_031056_1555   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-24.3

13.8

17.1

1.41

33.5

36.1

Northern Hellas Planitia Layered Bedrock:   ESP_031120_1505   ESP_031898_1505   (Interval in Earth days: 61)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-28.9

67.3

0

-13.4

35.4

34.8

Impact Crater with Central Peak:   ESP_031226_1820   ESP_067015_1820   (Interval in Earth days: 2789)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.009

50.0

-5.7

8.953

44.3

42.4

South Polar Layered Deposit Spiral Troughs during Katabatic Wind Season:   ESP_031048_0945   ESP_031100_0945   (Interval in Earth days: 4)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-85.4

289.

-13.

2.826

65.5

64.1

Light-Toned Stratified Materials in Melas Chasma:   ESP_031125_1670   ESP_031903_1670   (Interval in Earth days: 61)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.0

289.

-4.6

-18.9

38.4

33.6

USGS Dune Database Entry Number 2226-767:   ESP_031260_1030   ESP_031062_1030   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-76.6

223.

-13.

3.747

58.8

57.0


  


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