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.

Melas Chasma:   ESP_076489_1675   ESP_076977_1675   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-12.2

286.

0

15.90

35.7

38.9

Layering in Western Arabia Terra:   ESP_076447_1900   ESP_075959_1900   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.843

351.

-19.

-5.22

40.8

43.7

Dusty Terraced Impact Crater:   ESP_076372_1875   ESP_079181_1870   (Interval in Earth days: 219)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.279

237.

-2.6

-13.5

38.9

52.4

Dark Layers in Arabia Crater:   ESP_076460_1910   ESP_076671_1910   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
10.61

355.

-2.3

9.977

39.8

37.9

Valleys and Inverted Channels in Melas Chasma:   ESP_076621_1710   ESP_076476_1710   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-9.11

282.

15.2

-14.2

35.0

36.6

Small Delta or Fan:   ESP_076539_2150   ESP_077027_2150   (Interval in Earth days: 38)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
34.76

356.

-6.0

7.624

53.1

47.2

Inverted Channel and Possible Lake Deposits:   ESP_076462_1725   ESP_084242_1725   (Interval in Earth days: 606)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.56

303.

-5.5

29.60

35.8

38.1

Small Candidate Lake Deposit Downstream of Alluvial Fan:   ESP_076629_1675   ESP_076972_1675   (Interval in Earth days: 26)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-12.5

66.0

-6.2

-19.7

37.3

41.7

Crater in Arabia Terra:   ESP_076631_2175   ESP_077462_2175   (Interval in Earth days: 65)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
37.29

5.51

-8.7

7.098

53.9

45.4

Expanded Crater and Scalloped Depressions:   ESP_076524_1220   ESP_076880_1220   (Interval in Earth days: 27)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-57.4

58.6

-1.2

24.75

59.2

63.9


  


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