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.

Exposure of North Polar Layered Deposits:   ESP_035568_2655   ESP_036306_2655   (Interval in Earth days: 57)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
85.31

268.

-3.7

5.673

60.5

64.0

Faulted Layered Deposits in West Candor Chasma:   ESP_035582_1745   ESP_036070_1745   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.66

283.

-3.0

-27.7

58.0

60.2

Impact Monitoring Site in Phlegra Montes:   ESP_035362_2190   ESP_060984_2190   (Interval in Earth days: 1997)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
38.72

163.

-3.3

-21.8

42.2

41.7

Candidate Landing Site for 2020 Mission:   ESP_035304_1950   ESP_036148_1950   (Interval in Earth days: 66)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
14.70

309.

8.61

-3.59

45.9

49.1

Xanthe Terra Region:   ESP_035528_1920   ESP_036873_1920   (Interval in Earth days: 105)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
11.66

315.

0.16

11.08

48.5

51.2

Crater with Steep Slopes:   ESP_035246_2105   ESP_035879_2105   (Interval in Earth days: 50)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
30.23

91.0

6.44

-5.33

41.5

44.5

Light-Toned Deposits along Coprates Chasma Wallrock Slopes:   ESP_035199_1655   ESP_035555_1655   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.1

300.

-5.2

4.733

62.5

62.8

Young 10-Kilometer Diameter Crater:   ESP_035075_2010   ESP_035365_2010   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
20.77

82.2

-6.8

20.14

44.2

42.9

Gully in Crater Wall in Acidalia Planitia:   ESP_035118_2330   ESP_035408_2330   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
52.71

344.

-8.1

8.764

44.5

43.3

Aram Chaos:   ESP_034947_1830   ESP_036503_1830   (Interval in Earth days: 121)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.803

338.

2.06

16.03

50.6

52.8


  


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