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 Flows in Crater in Southwestern Daedalia Planum :   ESP_028886_1560   ESP_029031_1560   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-23.9

220.

-6.7

8.729

59.9

57.6

Depositional Fan on Northern Rim of Hargraves Crater :   ESP_028746_2010   ESP_033427_2010   (Interval in Earth days: 365)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
21.00

75.5

8.50

-7.28

53.5

38.7

Small Fresh Crater :   ESP_028795_2305   ESP_037155_2305   (Interval in Earth days: 651)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
50.08

174.

-1.2

-20.5

63.8

59.6

Troughs and Small Cones in Cydonia Region :   ESP_028670_2225   ESP_037465_2225   (Interval in Earth days: 685)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
42.35

349.

-6.3

4.464

59.2

59.5

Chevrons on Lava Surface in Marte Vallis :   ESP_028716_1880   ESP_053704_1875   (Interval in Earth days: 1947)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.810

177.

0

12.89

53.4

47.2

Layering in Crater in Mawrth Vallis :   ESP_028855_2045   ESP_020297_2045   (Interval in Earth days: 666)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
24.23

341.

-13.

-25.2

57.0

61.1

Light-Toned Deposits in Ladon Valles Basin :   ESP_028816_1605   ESP_029594_1605   (Interval in Earth days: 61)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-19.2

329.

6.81

-3.96

57.8

53.2

Well-Preserved Double Crater :   ESP_028631_1965   ESP_028776_1965   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
16.16

336.

-1.4

11.21

53.0

53.0

Lava Flow Through Breached Crater Rim in Tartarus Montes :   ESP_028637_2040   ESP_029072_2040   (Interval in Earth days: 34)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
23.67

172.

-8.4

27.76

54.3

55.5

Crater Filled with Mantling Deposit in Far Eastern Acidalia Planitia :   ESP_028628_2315   ESP_028694_2315   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
51.20

54.1

-4.9

-17.8

61.8

64.0


  


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