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.

Northern Mid-Latitude Crater:   ESP_062806_2150   ESP_062740_2150   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
34.80

100.

-3.6

15.57

45.8

43.6

Terraced Fan in East Candor Chasma:   ESP_062786_1730   ESP_062997_1730   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.84

292.

-3.2

-17.8

58.1

59.1

Sinuous Inverted Channel in Large Basin in East Arabia Terra:   ESP_062808_2085   ESP_062874_2085   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
28.26

45.7

8.60

-12.7

45.0

47.3

Flow Deposits in Eastern Ladon Valles Basin:   ESP_062745_1615   ESP_062956_1615   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-18.2

332.

8.06

-7.02

64.1

64.6

Dark Sediments in Medusae Fossae Formation:   ESP_062791_1800   ESP_035679_1800   (Interval in Earth days: 2113)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
0.052

153.

5.36

4.584

54.0

54.3

Candidate Landing Site for 2020 and Sample Return Missions at Jezero Crater:   ESP_062662_1990   ESP_062952_1990   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.61

77.2

-29.

-12.5

49.4

49.2

Lyot Crater Peak Ring:   ESP_062703_2295   ESP_062769_2295   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
49.32

29.0

8.48

-6.30

45.9

47.7

Central Peak of a Large Crater:   ESP_014361_1585   ESP_021587_1585   (Interval in Earth days: 563)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-21.5

44.7

-14.

6.137

35.0

43.9

The Life of a Glacier on Mars:   PSP_008809_2215   PSP_009455_2215   (Interval in Earth days: 51)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
41.27

54.7

-6.7

10.01

42.9

43.4

An Impact North of Valles Marineris:   ESP_011425_1775   ESP_012282_1775   (Interval in Earth days: 67)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-2.35

278.

-7.2

29.98

58.0

53.4


  


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