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.

Bright Layers in Hale Crater Ejecta:   PSP_006756_1465   ESP_023779_1465   (Interval in Earth days: 1327)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-33.2

322.

4.57

-11.2

53.6

43.7

Alluvial Fans in Unnamed Crater:   PSP_006528_1585   PSP_007095_1585   (Interval in Earth days: 44)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-21.4

67.1

0

-14.3

43.3

52.6

Gullies Within Central Pit of Bamberg Crater:   PSP_006794_2200   PSP_010301_2200   (Interval in Earth days: 274)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
39.66

356.

-3.9

21.59

46.9

48.7

Crater in Tyrrhena Terra:   PSP_006830_1745   ESP_069692_1740   (Interval in Earth days: 4898)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.58

99.6

-3.9

-21.0

40.7

61.4

Juventae Chasma Layered Kieserite Deposit:   PSP_006915_1760   PSP_007060_1760   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-3.96

298.

2.79

14.99

40.6

41.3

Fresh Double-Layered Crater with Possible Ponded Materials:   PSP_006945_2350   PSP_007235_2350   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
54.57

190.

1.13

12.28

54.1

50.5

Seasonal Monitoring:   PSP_005455_0975   PSP_005547_0975   (Interval in Earth days: 7)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-82.1

225.

1.30

15.98

69.4

69.9

Floor of Ares Vallis:   PSP_006940_1900   PSP_007876_1900   (Interval in Earth days: 73)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
10.11

334.

-1.8

20.02

38.4

42.9

Exposure of High-Latitude Polar Layered Deposits Not Well Observed:   PSP_005157_0875   PSP_005577_0925   (Interval in Earth days: 32)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-87.2

152.

0

14.21

71.5

75.0

Longitudinally-Aligned Rings and Cones in the Phlegra Dorsa Region:   PSP_006748_2060   PSP_006959_2060   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
25.91

173.

5.71

-5.32

40.1

40.5


  


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