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.

Ius Chasma Hydrated Mineralogy:   PSP_010792_1715   ESP_046501_1715   (Interval in Earth days: 2782)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.55

280.

4.74

-11.7

58.6

53.3

High-Latitude Exposure of North Polar Layered Deposits:   PSP_010555_2720   PSP_010583_2680   (Interval in Earth days: 3)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
87.91

156.

-8

-8.54

75.6

75.2

Distributary Channel South of Ascraeus Mons:   PSP_010872_1865   ESP_011373_1865   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
6.197

254.

-2.2

20.12

55.7

55.8

Crater in Icaria Fossae Region with Intersecting Graben:   ESP_011440_1335   ESP_011941_1335   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-45.9

234.

-5.1

15.24

68.4

59.6

Very Fresh 1-Kilometer Crater:   PSP_010571_2205   ESP_016083_2205   (Interval in Earth days: 429)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
40.22

187.

0.52

-26.3

53.7

46.1

Distinctive Small Rayed Crater in Terra Cimmeria:   PSP_010863_1720   ESP_020133_1720   (Interval in Earth days: 723)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.92

142.

-1.8

-20.3

58.8

57.3

Central Uplift of an Impact Crater:   PSP_010745_1465   ESP_028006_1465   (Interval in Earth days: 1345)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-33.2

126.

5.23

-17.2

69.4

71.8

Western Half of Very Fresh Crater in Utopia Region:   PSP_010402_2050   ESP_053495_2050   (Interval in Earth days: 3357)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
24.57

124.

-2.7

-23.1

51.1

44.1

Possible MSL Rover Landing Site Eberswalde Crater:   ESP_011265_1560   ESP_011331_1560   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-23.8

326.

20.4

-1.11

60.2

61.4

Cone at the Source of Athabasca Valles:   PSP_010770_1905   ESP_011403_1905   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
10.15

157.

16.7

-7.00

53.1

58.4


  


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