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.

Candidate Landing Site for 2020 Mission in Jezero Crater:   ESP_060130_1985   ESP_060275_1985   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.27

77.2

1.32

18.72

36.6

35.7

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

Exit Breach in Small Crater:   ESP_059976_1600   ESP_060121_1600   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-19.5

326.

-4.1

14.60

48.4

49.3

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

Candidate Landing Site for 2020 Mission Near Jezero Crater:   ESP_060196_1985   ESP_060486_1985   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.26

77.1

-17.

18.20

38.5

36.7

Troughs on North Polar Layered Deposits:   ESP_060011_2615   ESP_059985_2615   (Interval in Earth days: 2)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
81.33

58.2

8.35

-7.35

70.8

71.7

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 Channels Converging above Large Crater:   ESP_060180_1410   ESP_077470_1410   (Interval in Earth days: 1347)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-38.5

158.

8.70

-10.6

63.8

62.3

Outlet Breach in Crater:   ESP_060028_1460   ESP_060305_1460   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-33.7

347.

6.53

-14.5

58.0

63.3

Trough on North Polar Layered Deposits:   ESP_060102_2640   ESP_060063_2640   (Interval in Earth days: 3)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
84.06

80.7

9.00

-5.71

72.0

72.8


  


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