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.

Distinctive Small Rayed Crater in Terra Cimmeria:   PSP_010863_1720   ESP_020133_1720   (Interval in Earth days: 723)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.92

142.

-1.8

-20.3

58.8

57.3

Central Uplift of an Impact Crater:   PSP_010745_1465   ESP_028006_1465   (Interval in Earth days: 1345)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-33.2

126.

5.23

-17.2

69.4

71.8

Possible Source for a Small Outburst along the Cerberus Fossae:   PSP_010480_1910   ESP_053362_1910   (Interval in Earth days: 3341)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
10.70

155.

7.33

-7.40

52.6

47.0

Noachis Region Clays:   ESP_011592_1595   ESP_011658_1595   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-20.3

40.3

4.94

-17.2

58.3

59.6

Knobs and Thermokarst:   ESP_011365_1365   ESP_011642_1365   (Interval in Earth days: 21)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-43.3

120.

5.79

-16.4

67.6

65.5

Ithaca Region Plumes:   ESP_011350_0945   ESP_011351_0945   (Interval in Earth days: 0)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-85.2

181.

22.8

-3.81

87.6

89.8

Light-Toned Layering in Ladon Valles:   PSP_010632_1595   ESP_028394_1595   (Interval in Earth days: 1384)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-20.5

330.

3.21

13.98

64.0

60.3

Odd Craters North of Bacolor Crater:   PSP_010890_2150   ESP_045531_2150   (Interval in Earth days: 2699)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
34.58

119.

-3.7

-23.4

56.9

46.9

Apron of Material in Columbus Crater:   PSP_010492_1510   ESP_045278_1510   (Interval in Earth days: 2710)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-28.8

194.

-5.8

-28.5

69.7

69.7

Very Fresh 1-Kilometer Crater:   PSP_010571_2205   ESP_016083_2205   (Interval in Earth days: 429)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
40.22

187.

0.52

-26.3

53.7

46.1


  


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