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.

Fresh 3-Kilometer Diameter Crater Near Hellas Planitia:   ESP_016681_1575   ESP_017393_1575   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-22.1

67.3

-6.1

7.478

62.0

66.5

Field of Small Volcanoes Northeast of Ascraeus Mons:   ESP_016832_1885   ESP_017254_1885   (Interval in Earth days: 32)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
8.580

259.

8.08

-10.9

44.8

48.3

Very Well-Preserved 9-Kilometer Diameter Impact Crater:   ESP_016490_2315   ESP_016780_2315   (Interval in Earth days: 23)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
51.39

234.

-21.

-2.88

48.2

45.3

Aram Chaos:   ESP_016750_1830   ESP_017172_1830   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
2.769

339.

3.01

-13.3

47.2

51.0

Remnant Mantiling Deposit in Millochau Crater:   ESP_016377_1585   ESP_017010_1585   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-21.2

85.4

7.40

-9.53

57.1

64.5

Source Region for Branch of Auqakuh Vallis:   ESP_016826_2080   ESP_016971_2080   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
27.47

62.7

-7.7

5.246

41.4

40.6

Northern Plains West of Erebus Montes:   ESP_016650_2205   ESP_035427_2205   (Interval in Earth days: 1464)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
40.26

185.

-1.2

27.98

42.1

39.3

Well-Preserved Crater in Margaritifer Terra:   ESP_016407_1675   ESP_016763_1675   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-12.5

345.

-0.5

12.61

52.5

55.3

Possible Phyllosilicates in Her Desher Vallis:   ESP_016527_1550   ESP_025032_1550   (Interval in Earth days: 663)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-24.8

311.

-6.8

7.004

62.1

56.3

Layered Deposits along Floor of Melas Chasma:   ESP_016673_1700   ESP_017952_1700   (Interval in Earth days: 100)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-9.67

284.

-5.2

5.092

53.8

59.7


  


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