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.

Lava and Streamlined Forms in Athabasca Valles:   ESP_042167_1890   ESP_052294_1890   (Interval in Earth days: 789)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
9.141

156.

7.63

-5.94

37.4

44.1

East Endeavour Crater Dune Field:   ESP_042674_1775   ESP_042740_1775   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-2.32

354.

7.30

-16.8

44.2

46.5

USGS Dune Database Number 0380-426 Changes:   ESP_042343_1370   ESP_033811_1370   (Interval in Earth days: 664)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-42.6

38.0

0.13

15.08

65.4

68.7

Inverted Channels on Fan in Saheki Crater:   ESP_042368_1580   ESP_042869_1580   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-21.9

72.7

-2.1

12.98

51.9

57.0

Fresh Impact with Many Secondary Craters in Acidalia Planitia:   ESP_042292_2195   ESP_042793_2195   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
39.29

340.

-7.9

2.101

45.4

41.8

Candidate Landing Site for 2020 Mission:   ESP_042430_1510   ESP_042364_1510   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-28.6

181.

-9.5

13.55

57.4

55.1

Fan on Crater Floor:   ESP_042661_1505   ESP_046327_1505   (Interval in Earth days: 286)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-29.1

353.

3.01

-13.7

60.0

61.5

Cerberus Fossae:   ESP_042457_1915   ESP_045912_1915   (Interval in Earth days: 269)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
11.14

157.

8.06

-3.60

38.5

48.2

Oxia Palus Region:   ESP_042134_1985   ESP_053962_1985   (Interval in Earth days: 922)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.04

335.

7.47

-28.4

37.8

47.7

Terrain Contacts in Argyre Region:   ESP_042359_1295   ESP_050996_1295   (Interval in Earth days: 673)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-50.1

322.

-3.6

-19.7

71.4

68.2


  


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