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.

Dark Materials on Block in Olympus Mons Aureole:   PSP_008935_1975   ESP_016372_1975   (Interval in Earth days: 580)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
17.33

217.

-8.1

5.979

47.1

40.0

Characterize Surface Hazards and Science of MSL Rover Landing Site:   PSP_008218_1815   PSP_008719_1815   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
1.522

357.

13.4

-4.22

49.6

53.4

Central Peak and Floor of Large Crater West of Schiaparelli Crater:   PSP_008613_1760   PSP_008969_1760   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-3.93

12.2

1.91

-18.6

55.6

58.3

Stratigraphy in Aureum Chaos:   PSP_008443_1760   PSP_008944_1760   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-3.72

334.

9.28

-8.46

54.2

57.4

Crater Floor and Central Mound in Gale Crater (MSL):   PSP_009505_1755   PSP_009571_1755   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-4.47

137.

-7.4

-28.4

58.6

60.2

Deposits Layered at Several Scales:   PSP_009038_1745   PSP_010027_1745   (Interval in Earth days: 77)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-5.54

286.

2.43

-12.1

58.0

59.4

Drainage Off Ponded Materials in Mojave Crater:   PSP_008496_1880   PSP_009076_1880   (Interval in Earth days: 45)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.741

326.

-8.6

13.58

49.6

50.0

Polygons and Spots on Defrosting Dunes:   PSP_008867_2640   PSP_009105_2640   (Interval in Earth days: 18)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
83.99

233.

8.23

-9.68

59.0

59.9

Flows on the Northeastern Flank of Arsia Mons:   PSP_008565_1720   PSP_009844_1720   (Interval in Earth days: 100)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-7.68

242.

9.15

-10.2

57.2

60.4

Impact Crater Amid the Deuteronilus Mensae:   PSP_009021_2245   PSP_009654_2245   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
44.21

23.3

8.73

-7.10

42.2

46.4


  


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