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.

Sublimation Process and Spider Evolution:   PSP_003490_0930   PSP_003846_0930   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-86.9

274.

0.41

0.79

73.5

68.7

Cerberus Fossae with Fluvial/Volcanic Features Near Athabasca Vallis Head:   PSP_003650_1900   PSP_004283_1900   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
10.01

157.

-3.5

-20.4

58.7

56.3

Layered Sinuous Ridge in Argyre Planitia:   PSP_003816_1245   PSP_004106_1245   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-55.1

314.

3.82

21.86

51.2

46.0

Craters with Valley on Both Ends - South End:   PSP_003402_1795   PSP_003547_1795   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-0.40

89.6

-0.6

14.47

55.1

53.4

South Polar Layered Deposit Comparison with Higher Latitude Scarps:   PSP_003868_0940   PSP_003896_0940   (Interval in Earth days: 3)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-85.7

13.2

-0.6

-19.9

67.4

70.0

Light-Toned Layering in Ius Chasma:   PSP_003593_1725   ESP_058000_1725   (Interval in Earth days: 4239)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.48

275.

4.77

-11.1

51.7

34.5

Gullies with Tributary Channels in Gorgonum Chaos Crater:   PSP_003649_1435   PSP_003794_1435   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-36.3

190.

3.51

18.06

48.9

45.7

Mangala Source:   PSP_003635_1615   PSP_005613_1615   (Interval in Earth days: 154)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-18.2

210.

-1.4

-22.8

49.5

34.9

Fresh Crater:   PSP_003942_1585   ESP_058138_1585   (Interval in Earth days: 4223)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-21.1

109.

1.8

-11.9

45.4

31.0

Breached Impact Crater in Elysium Planitia:   PSP_004151_1810   ESP_020963_1810   (Interval in Earth days: 1310)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
0.869

160.

1.37

-21.1

50.9

56.5


  


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