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.

Lobate Margin of Impact Ejecta:   PSP_006835_2085   PSP_007481_2085   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
28.13

319.

-5.9

4.424

41.5

40.0

Eastern Side of Hale Crater Ridge with Gullies on Both Sides:   PSP_005833_1445   ESP_011753_1445   (Interval in Earth days: 462)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-35.1

324.

0.11

25.34

40.8

58.2

Basal Exposure of South Polar Layered Deposits:   PSP_005379_1060   PSP_005893_1060   (Interval in Earth days: 40)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-74.0

131.

-5.2

20.22

62.0

68.6

Small Shield Volcanoes on Syria Planum:   PSP_005031_1680   PSP_005453_1680   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-11.7

257.

-5.2

-22.1

36.1

34.9

Pair of Small Pits in the Arsia Chasmata:   PSP_005203_1730   PSP_005625_1730   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.71

240.

5.13

-11.8

35.6

34.4

Central Uplift of Large Crater in Syrtis Major:   PSP_006607_1985   PSP_007108_1985   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.47

65.1

0

9.813

38.4

38.1

Pitted Layers Northeast of Hellas Region:   PSP_006198_1525   ESP_032702_1525   (Interval in Earth days: 2065)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.3

78.0

0

-26.6

41.6

43.7

Gullies in Southwest Noachis Ring Trough:   PSP_006003_1320   PSP_006926_1320   (Interval in Earth days: 72)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-47.5

4.56

7.00

-4.62

50.7

67.0

Breached and Flooded Crater:   PSP_006511_1935   PSP_007078_1935   (Interval in Earth days: 44)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
13.33

167.

0

-14.1

37.2

40.0

Unnamed Well-Preserved Crater in Cimmeria Terra:   PSP_005286_1480   PSP_005576_1480   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-31.5

140.

-27.

-1.66

36.8

36.4


  


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