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.

Possible Fan in Crater :   ESP_029490_1565   ESP_029912_1565   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-23.3

288.

3.81

-10.5

53.9

50.7

Layered Material in Melas Chasma :   ESP_029411_1690   ESP_055599_1690   (Interval in Earth days: 2040)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-10.6

284.

-1.8

24.60

54.1

51.0

Possible Phyllosilicate Deposit in Valles Marineris :   ESP_029569_1675   ESP_056720_1675   (Interval in Earth days: 2116)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-12.5

290.

5.53

-4.17

52.7

46.2

Interesting Young Flow Features in Nereidum Montes :   ESP_029634_1430   ESP_041001_1430   (Interval in Earth days: 886)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-36.5

319.

4.54

-22.6

54.6

42.3

Impacts from MSL Tungsten Blocks and Cruise Stage:   ESP_029245_1755   ESP_031869_1755   (Interval in Earth days: 204)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.40

136.

1.29

-18.0

54.3

35.6

Columnar Jointing on Mars and Earth:   ESP_029286_1885   ESP_030143_1885   (Interval in Earth days: 67)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.599

95.5

-3.4

18.28

56.1

55.5

Colorful Fractured Bedrock in Ritchey Crater:   ESP_029542_1510   ESP_029964_1510   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-28.5

308.

14.3

3.043

53.3

49.1

20-Kilometer Crater in Meridiani Planum Exposing Layers :   ESP_029092_1770   ESP_029804_1770   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-2.96

353.

-8.5

3.934

55.2

53.2

Multiple Geologic and Geomorphic Units in Contact :   ESP_029151_1695   ESP_029296_1695   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-10.4

182.

4.21

20.99

54.6

52.7

Ridges and Valley and Flow Fronts in CTX Image D03_028235_1829_XN_02N011W:   ESP_029013_1830   ESP_031215_1830   (Interval in Earth days: 171)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.723

348.

3.34

11.42

54.2

43.8


  


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