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.

Candidate Recent Impact Site :   ESP_050129_2055   ESP_050696_2055   (Interval in Earth days: 44)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
25.45

222.

-2.3

-15.1

43.1

39.6

Wrinkle Ridge in Sacra Sulci Region :   ESP_050430_2000   ESP_050720_2000   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
19.63

283.

8.44

28.67

36.6

33.7

Gully Monitoring :   ESP_050125_1480   ESP_050046_1480   (Interval in Earth days: 6)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-31.4

337.

16.6

-14.6

38.5

39.5

Possible Dike Associated with Aromatum Chaos :   ESP_050363_1785   ESP_050429_1785   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.26

316.

-0.5

-24.5

32.2

34.6

Dark-Toned Disks in Light-Toned Layer along Samara Valles :   ESP_050415_1565   ESP_050626_1565   (Interval in Earth days: 17)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-23.4

339.

-6.5

-17.9

39.6

43.5

Floor of Ius Chasma:   ESP_050338_1720   ESP_050483_1720   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.81

279.

0.96

12.74

32.5

32.8

Monitor Small Fresh Impact Crater in Meridiani Planum :   ESP_050322_1740   ESP_059566_1740   (Interval in Earth days: 720)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.09

356.

4.50

19.72

31.9

34.6

Smaller Deposit of Hargraves Crater Ejecta in Nili Fossae Trough :   ESP_050319_2020   ESP_050385_2020   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
21.64

74.9

-1.4

-23.0

39.0

40.2

Clays Exposed in Electris Region Deposit :   ESP_050236_1445   ESP_050170_1445   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-35.0

188.

-1.1

20.77

43.5

41.1

Search for Active Glacial Flow:   ESP_050279_1420   ESP_050490_1420   (Interval in Earth days: 16)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-37.8

95.4

-8.5

-19.1

46.5

50.6


  


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