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.

Mamers Valles:   PSP_009773_2165   ESP_053789_2165   (Interval in Earth days: 3429)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
36.13

14.3

5.21

-4.42

45.5

42.7

Fresh Santa Fe Crater in Chryse Planitia:   PSP_009749_1995   PSP_010382_1995   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
19.36

312.

3.75

-11.7

47.9

52.2

Well-Preserved Crater on a Steep Slope in Tyrrhena Terra:   PSP_009824_1610   PSP_010246_1610   (Interval in Earth days: 33)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-18.5

69.0

6.12

-5.57

65.8

65.3

High-Latitude Exposure of North Polar Layered Deposits:   PSP_010080_2680   PSP_010856_2720   (Interval in Earth days: 61)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
87.79

209.

-8.2

-6.88

68.7

80.5

Rayed Thila Crater in Elysium Planitia:   PSP_009346_1985   PSP_009491_1985   (Interval in Earth days: 12)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.08

155.

-5.4

8.677

47.7

47.0

Sapping Features East of Tooting Crater:   PSP_010333_2025   PSP_010689_2025   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
22.14

208.

-3.9

0.754

50.8

53.1

Central Pit of Large But Well-Preserved Crater:   PSP_009585_1660   PSP_010429_1660   (Interval in Earth days: 66)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-13.7

113.

5.01

-19.0

63.2

63.2

Small Crater on the North Polar Deposits:   PSP_009773_2675   PSP_010500_2675   (Interval in Earth days: 56)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
87.25

297.

0.08

-14.1

65.4

73.7

Southern Highlands High Thermal Inertia and Spectrally Distinct Materials:   PSP_010326_1560   PSP_010471_1560   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-23.7

44.9

4.00

18.94

67.2

65.4

Phyllosilicates in Acidalia Region:   PSP_009538_2220   PSP_010039_2220   (Interval in Earth days: 39)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
41.78

309.

0.48

17.37

44.8

46.8


  


Page 778 of 896 (8,955 images)