Abalos Undae

Abalos Undae ( Latin for "Abalos Waves") is a dune field on Mars in the periphery of Planum Boreum , the Martian North pole. It is one of the officially named northern circumpolar dune fields, along with Olympia , Hyperboreae , and Siton Undae , and also one of the densest of the region. [1] [2] Its northernmost boundary is located in the southwest channel that separates the Abalos Colles formation from the main polar ice cap, and from there the dune field extends southwest all the way to the lowlands of Vastitas Borealis . [2] [3] [4]

Page Revisions

Year Metadata Sections Top Words First Paragraph
2018

107217 characters

5 sections

22 paragraphs

18 images

665 internal links

13 external links

1. Location and formation characteristics

2. Images by HiRISE and THEMIS

3. See also

4. References

5. External links

abalos 0.695

undae 0.528

dunes 0.192

dune 0.138

scarp 0.133

colour 0.118

hyperboreae 0.112

gypsum 0.111

periphery 0.105

olympia 0.098

basal 0.091

siton 0.090

irb 0.087

fields 0.068

tenuis 0.067

Abalos Undae ( Latin for "Abalos Waves") is a dune field on Mars in the periphery of Planum Boreum , the Martian North pole. It is one of the officially named northern circumpolar dune fields, along with Olympia , Hyperboreae , and Siton Undae , and also one of the densest of the region. [1] [2] Its northernmost boundary is located in the southwest channel that separates the Abalos Colles formation from the main polar ice cap, and from there the dune field extends southwest all the way to the lowlands of Vastitas Borealis . [2] [3] [4]

2017

65095 characters

5 sections

22 paragraphs

21 images

176 internal links

10 external links

1. Location and formation characteristics

2. Images by HiRISE and THEMIS

3. See also

4. References

5. External links

abalos 0.695

undae 0.528

dunes 0.192

dune 0.138

scarp 0.133

colour 0.118

hyperboreae 0.112

gypsum 0.111

periphery 0.105

olympia 0.098

basal 0.091

siton 0.090

irb 0.087

fields 0.068

tenuis 0.067

Abalos Undae ( Latin for "Abalos Waves") is a dune field on Mars in the periphery of Planum Boreum , the Martian North pole. It is one of the officially named northern circumpolar dune fields, along with Olympia , Hyperboreae , and Siton Undae , and also one of the densest of the region. [1] [2] Its northernmost boundary is located in the southwest channel that separates the Abalos Colles formation from the main polar ice cap, and from there the dune field extends southwest all the way to the lowlands of Vastitas Borealis . [2] [3] [4]