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.

Jezero Crater Outflow Channel:   ESP_076879_1980   ESP_076945_1980   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.01

77.8

9.06

-4.89

39.9

40.7

Xanthe Dorsa:   ESP_076870_2225   ESP_077081_2225   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
42.17

320.

-0.1

13.43

53.8

50.7

Channels in Nereidum Montes:   ESP_076765_1435   ESP_076132_1435   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-36.4

316.

7.45

-16.9

48.3

41.4

Terrain Sample near Zhurong Rover Landing Site:   ESP_076957_2055   ESP_077168_2055   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
25.33

109.

-7.7

10.93

43.9

41.5

Gullies on Massif in Argyre Region:   ESP_076923_1345   ESP_076224_1345   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-45.0

325.

7.99

-7.78

56.6

46.5

Traverse Ramp in East Coprates Chasma:   ESP_076818_1640   ESP_076752_1640   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.6

306.

9.47

23.67

38.7

36.8

USGS Dune Database Entry Number 3525-631:   ESP_076909_1165   ESP_076988_1165   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-63.1

352.

-2.8

20.78

70.2

70.3

Deposits in Aeolis Dorsa:   ESP_076995_1735   ESP_076784_1735   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.26

154.

19.6

0.949

37.1

36.9

Downwind Hellespontus Regional Barchan Dunes:   ESP_076841_1380   ESP_076221_1380   (Interval in Earth days: 48)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-41.4

44.5

-10.

12.82

53.9

43.1

Floor of East Candor Chasma:   ESP_077056_1730   ESP_078045_1730   (Interval in Earth days: 77)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.86

291.

-7.9

23.88

40.0

48.6


  


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