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.

Well-Preserved 7-Kilometer Impact Crater :   ESP_046334_2075   ESP_050883_2075   (Interval in Earth days: 355)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
27.00

154.

-7.3

5.524

52.7

37.9

Fracture in Utopia Planitia:   ESP_046296_2130   ESP_046006_2130   (Interval in Earth days: 22)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
32.86

109.

7.91

-14.7

52.5

50.8

Alluvial Fans in Southwestern Mojave Crater:   ESP_046275_1870   ESP_051958_1870   (Interval in Earth days: 443)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
7.160

326.

5.60

25.31

49.5

40.4

Crater in Corinto Crater Secondary Field :   ESP_046440_1965   ESP_047152_1965   (Interval in Earth days: 55)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
16.29

140.

5.52

18.67

50.8

55.2

Crater with Steep Slopes:   ESP_046262_2095   ESP_051866_2095   (Interval in Earth days: 436)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
29.21

320.

-8.3

-22.4

52.5

39.9

Landforms at West End of Her Desher Vallis :   ESP_046579_1550   ESP_047423_1550   (Interval in Earth days: 66)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-24.5

311.

5.67

-27.2

56.1

51.0

Floor of East Candor Chasma :   ESP_046395_1730   ESP_046250_1730   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-6.84

292.

3.09

-12.7

52.0

53.4

Braided Channel System in Eastern Hellas Region :   ESP_046323_1405   ESP_051149_1405   (Interval in Earth days: 377)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-38.9

102.

6.20

-8.76

65.1

61.5

Sharply Stratified Wind Eroded Crater Fill Deposit :   ESP_046498_1430   ESP_046854_1430   (Interval in Earth days: 28)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-36.4

5.63

-9.7

1.604

63.0

58.0

Protonilus Mensae Debris Apron :   ESP_046430_2260   ESP_046496_2260   (Interval in Earth days: 5)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
45.90

48.9

8.77

-5.59

59.3

61.5


  


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