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.

Contact between Wallrock and Light-Toned Deposits in Hebes Chasma:   ESP_013772_1795   ESP_022910_1795   (Interval in Earth days: 712)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-0.51

283.

-21.

-5.7

43.5

37.1

Alcove in East Candor Chasma Layered Deposits:   ESP_012809_1725   ESP_013310_1725   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.44

293.

-2.1

22.37

50.2

42.7

Possible Blocky Deposit in Melas Chasma:   ESP_013508_1665   ESP_014141_1665   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.2

289.

6.08

-18.0

39.2

35.6

Distal Rampart of Crater in Chryse Planitia:   ESP_014140_1975   ESP_014417_1975   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.17

311.

4.17

-20.1

48.0

46.2

Basal Exposure of South Polar Layered Deposits:   ESP_013145_1070   ESP_013277_1070   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-73.0

133.

0.46

-14.5

55.6

56.1

Bright Gully Deposits in Western Hale Crater:   ESP_012874_1450   ESP_013019_1450   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-34.8

322.

-1.8

13.78

44.6

41.4

Putative Paleolake:   ESP_013780_1630   ESP_058667_1630   (Interval in Earth days: 3497)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-16.7

64.7

1.57

-15.2

35.8

31.8

Crater in the Sirenum Fossae Region:   ESP_012918_1450   ESP_013340_1450   (Interval in Earth days: 32)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-34.4

201.

-7.6

-20.0

44.4

40.3

Light-Toned Material in a Crater in Iani Chaos:   ESP_013572_1795   ESP_022710_1795   (Interval in Earth days: 712)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-0.54

341.

-3.2

13.82

44.7

37.9

Remnant of Unusual Looking Material on Plains:   ESP_012675_1565   ESP_013743_1565   (Interval in Earth days: 83)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-23.0

353.

-1.3

22.39

47.7

33.5


  


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