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.

Central Uplift of a Large Impact Crater:   PSP_010534_1620   ESP_051992_1620   (Interval in Earth days: 3230)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-17.8

125.

-4.5

-24.2

63.7

58.4

Section of Wall Rock on the South Rim of Coprates Chasma:   PSP_010501_1645   ESP_016026_1645   (Interval in Earth days: 431)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-15.4

305.

5.32

23.12

62.0

48.0

Mesas with Circumferential Depressions Near Kasei Valles:   ESP_011319_2100   ESP_011464_2100   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
29.64

289.

-20.

-7.41

62.3

62.9

Light-Toned Layering South of Ius Chasma with Unusual Morphology:   PSP_010423_1720   ESP_016726_1720   (Interval in Earth days: 491)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-8.01

275.

-10.

7.863

60.0

52.5

Possible MSL Landing Site in Holden Crater:   ESP_011397_1535   ESP_011898_1535   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-26.3

324.

3.35

27.36

61.3

54.6

Arandas Crater in Northern Plains:   PSP_010407_2230   ESP_019123_2230   (Interval in Earth days: 679)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
42.43

345.

0

17.14

52.3

48.4

Channels on North Rim of Cerulli Crater:   PSP_010498_2135   ESP_045574_2135   (Interval in Earth days: 2733)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
32.99

21.7

4.01

14.18

51.5

43.7

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

Eastern Rim of Heimdal Crater:   PSP_010648_2485   PSP_010846_2485   (Interval in Earth days: 15)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
68.34

235.

11.9

-10.7

63.8

68.8

Distributary Channel South of Ascraeus Mons:   PSP_010872_1865   ESP_011373_1865   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
6.197

254.

-2.2

20.12

55.7

55.8


  


Page 735 of 862 (8,618 images)