Surface Density of Large Lunar Craters View Full Text


Ontology type: schema:ScholarlyArticle     


Article Info

DATE

1968-06

AUTHORS

L. B. RONCA, R. R. GREEN

ABSTRACT

So that variations in cratering parameters on the lunar surface can be determined, the front face of the Moon has been divided into a grid of equiareal blocks. Various crater parameters can be measured for each block, and variations of the parameter can be shown diagrammatically by assigning the values of the parameter to the co-ordinates of the centre of the blocks and then constructing contours over the lunar disk. More... »

PAGES

1147-1149

References to SciGraph publications

Identifiers

URI

http://scigraph.springernature.com/pub.10.1038/2181147a0

DOI

http://dx.doi.org/10.1038/2181147a0

DIMENSIONS

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