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.

Pavonis Mons:   ESP_039131_1830   ESP_039342_1830   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.876

244.

6.87

-5.46

55.0

54.2

Seeing Beneath the Surface in Morava Valles:   ESP_038798_1665   ESP_039497_1665   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.2

335.

0

-13.8

52.6

46.3

Candidate ExoMars Landing Site:   ESP_038428_1880   ESP_047461_1880   (Interval in Earth days: 704)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.816

348.

-1.7

-18.0

59.1

55.8

Channels Emanating from Flow Deposit:   ESP_038629_1750   ESP_039328_1750   (Interval in Earth days: 54)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.03

266.

-15.

5.479

56.6

49.9

Outflow Channel Landforms in CTX Image:   ESP_038490_1430   ESP_064771_1430   (Interval in Earth days: 2048)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-36.9

102.

0.95

-18.7

56.4

60.8

Fractured Mesa in Elysium Planitia:   ESP_038659_1815   ESP_038184_1815   (Interval in Earth days: 37)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
1.316

168.

-28.

-7.09

59.3

57.8

Deposits in Libya Montes:   ESP_038530_1830   ESP_038398_1830   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.712

85.9

-0.0

21.69

57.6

55.8

Well-Preserved Impact Crater:   ESP_038345_1925   ESP_065470_1925   (Interval in Earth days: 2113)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
12.18

93.3

-5.2

4.187

60.4

61.4

Crater in Isidis Planitia:   ESP_038319_1860   ESP_046284_1860   (Interval in Earth days: 620)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
6.136

83.4

-3.9

-20.7

58.6

51.8

Pollack Crater Bedform Changes Near Formation Dubbed White Rock:   ESP_038308_1720   ESP_037675_1720   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.01

24.9

2.08

-16.1

56.0

58.8


  


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