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.

Ridges and Alcoves:   ESP_060238_1820   ESP_060805_1820   (Interval in Earth days: 44)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.070

11.2

-1.5

16.93

40.6

44.5

Osuga Valles Depression Transect:   ESP_060108_1650   ESP_060174_1650   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.8

322.

-4.6

-24.7

47.4

49.7

Dunes and Steep Slopes in Coprates Chasma:   ESP_060188_1660   ESP_060333_1660   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.7

298.

-3.5

16.22

47.8

48.4

Tilted Layers in Electris Region:   ESP_059955_1435   ESP_060232_1435   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-36.0

181.

7.57

-13.5

58.5

63.9

Candidate Recent Impact Site:   ESP_060062_1840   ESP_060128_1840   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
3.862

135.

-0.6

-21.4

38.3

40.6

Aeolis Dorsa Deltaic Lobes:   ESP_060035_1735   ESP_059402_1735   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.38

154.

-6.4

7.766

42.2

33.8

Smooth Region in Phlegra Montes:   ESP_060140_2170   ESP_060430_2170   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
36.42

162.

-1.9

25.22

40.8

37.6

Small Crater in Light Mantle:   ESP_060135_2350   ESP_059647_2350   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
54.53

298.

-20.

-5.52

51.5

55.6

Northwestern Rim of Roddy Crater:   ESP_060029_1585   ESP_059963_1585   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-21.3

320.

-10.

11.28

50.6

48.3

Apollinaris Sulci Ancient Dunes:   ESP_060166_1675   ESP_060443_1675   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-12.5

177.

6.46

-16.4

46.1

51.1


  


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