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.

Channel in Maadim Vallis :   ESP_045951_1560   ESP_046162_1560   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-23.5

176.

7.72

-1.89

60.0

59.2

Valley with Flows in Noachis Terra :   ESP_045853_1525   ESP_046565_1525   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-27.2

333.

-6.9

5.379

63.7

57.2

Basin with Lava Fill in Southern Elysium Planitia :   ESP_045938_1775   ESP_046149_1775   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-2.57

167.

18.6

9.184

49.8

50.6

Crater with Blocky Interior in Marte Vallis :   ESP_045977_1920   ESP_046267_1920   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
11.83

183.

-6.5

20.42

48.6

48.0

Candidate Landing Site for 2020 Mission in Jezero Crater :   ESP_045994_1985   ESP_046060_1985   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.42

77.4

3.48

-18.2

47.5

49.9

Syria Planum Bedform and Albedo Changes :   ESP_046080_1655   ESP_046502_1655   (Interval in Earth days: 32)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.2

252.

22.2

7.064

53.8

53.2

1-Kilometer Diameter Crater :   ESP_046065_2260   ESP_046355_2260   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
45.84

295.

-5.3

13.65

54.8

57.7

East Coprates Montes Dark Fans :   ESP_045907_1665   ESP_046619_1665   (Interval in Earth days: 56)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.3

297.

-2.1

12.58

55.8

52.1

Thin Layers in Eroded Crater Southwest of Bamberg Crater :   ESP_046142_2165   ESP_046643_2165   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
36.34

355.

-6.1

12.42

52.7

58.2

Light-Toned Surface in Valley in CTX Image :   ESP_046011_1620   ESP_046723_1620   (Interval in Earth days: 56)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-17.8

338.

-6.0

11.19

57.7

52.7


  


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