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.

Possible Hematite and Kieserite in Capri Chasma:   ESP_023753_1660   ESP_024320_1660   (Interval in Earth days: 44)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.8

309.

-4.7

8.069

34.3

39.8

Small Floral-Shaped Volcano on a Cerberus Fossa:   ESP_023811_1880   ESP_024378_1880   (Interval in Earth days: 45)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.076

162.

7.71

21.56

34.0

33.7

Basal Exposure of South Polar Layered Deposits:   ESP_023773_1025   ESP_023615_1025   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-77.2

129.

25.3

8.468

75.0

73.1

Crater with Surrounding Bench in Sinus Meridiani:   ESP_023382_1845   ESP_023593_1845   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
4.381

356.

-2.8

-14.6

35.3

35.2

Aeolis Planum:   ESP_023785_1745   ESP_067671_1745   (Interval in Earth days: 3420)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.55

154.

0

-21.5

32.9

41.2

Rugged Banded Material in Crater in Northwest Hellas Planitia:   ESP_023789_1420   ESP_024066_1420   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-37.7

47.4

21.8

0.082

44.7

50.6

Possible Exposures of Polar Layered Deposits in Area Not Well Observed:   ESP_023793_0895   ESP_023673_0905   (Interval in Earth days: 9)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-89.2

49.1

24.5

24.15

86.2

83.8

Libya Montes Layered Cliffs:   ESP_023827_1835   ESP_024671_1835   (Interval in Earth days: 65)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
3.427

85.9

11.0

-9.63

32.7

38.9

Gullies on Eastern Side of Crater in Newton Crater:   ESP_023612_1375   ESP_023546_1375   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-42.2

202.

5.08

22.97

46.0

43.8

South Polar Residual Cap in Late Summer:   ESP_023677_0920   ESP_023781_0920   (Interval in Earth days: 8)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-88.0

298.

11.1

22.62

84.1

84.5


  


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