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.

Valleys in Crater Northeast of Argyre Region:   ESP_067704_1500   ESP_073784_1500   (Interval in Earth days: 474)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-29.6

334.

7.13

20.86

44.0

53.7

Inverted Channel in Cusus Valles:   ESP_067833_1960   ESP_067965_1960   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
16.05

49.8

5.88

-3.77

43.8

44.2

Mounds in Acidalia Planitia:   ESP_068074_2280   ESP_068483_2280   (Interval in Earth days: 32)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
47.47

312.

-7.6

26.38

59.5

53.0

Two Notches near Lowest Elevation Point of Crater Rim:   ESP_067821_1465   ESP_067689_1465   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-33.2

24.7

-7.3

6.887

48.4

45.5

Gullies Eroding Thick Mantling Deposits:   ESP_067903_1370   ESP_073574_1370   (Interval in Earth days: 442)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-42.6

308.

-5.4

22.27

54.7

59.3

Terrain in Cydonia Region:   ESP_067848_2205   ESP_068970_2200   (Interval in Earth days: 87)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
40.15

358.

-1.9

-16.2

57.0

50.7

Landforms on Floor of Wahoo Crater:   ESP_067902_2040   ESP_067493_2040   (Interval in Earth days: 32)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
23.50

326.

8.19

-6.89

46.5

50.7

Eroded Crater with Eroded Floor in Hellas Region:   ESP_067435_1385   ESP_076680_1385   (Interval in Earth days: 721)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-40.9

116.

-2.8

6.995

46.5

49.9

Crater near Uranius Mons:   ESP_067495_2080   ESP_067363_2080   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
27.80

271.

-7.2

8.657

53.2

53.7

Small Impact Crater Exposed by Erosion:   ESP_067455_1755   ESP_067930_1755   (Interval in Earth days: 37)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.48

286.

-3.2

8.213

39.3

40.2


  


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