This extended conference abstract describes new crater size-frequency distribution measurements around the Apollo 14 landing site
The size-frequency distribution (SFD) of craters on the Moon, Mars, and Mercury turns up at very sma...
The distribution of impact craters on the ejecta of Giordano Bruno, a recent (<10 Ma) 22-km ...
In September 1977, a crater studies workshop was held for the purpose of developing standard data an...
This extended conference abstract describes a new geological map and crater size-frequency distribut...
This extended conference abstract describes geological mapping of the Apollo 17 landing site in the ...
The shape of the size-frequency distribution for small (<= 1 km diameter) primary craters coul...
This journal article describes geological mapping of the Apollo 12 landing site in the context of ne...
This extended conference abstract discusses the age and origin of the lunar northern light plains ba...
The threat of destructive impact events on Earth is mirrored in more than 160 proven impact structur...
This extended conference abstract describes progress being made on new geological maps of the Apollo...
Boulders represent a landing hazard that must be addressed in the planning of future landings on the...
It is shown that the size-frequency distribution (SFD) of a time-averaged projectile population deri...
The log normal frequency distribution law was used to analyze the crater population on the surface o...
By using high-resolution altimetric measurements of the Moon, we produced a catalog of all impact cr...
Recently it could be shown (Scholkmann, Prog. in Phys. , 2016, v. 12(1), 26-29) that the impact c...
The size-frequency distribution (SFD) of craters on the Moon, Mars, and Mercury turns up at very sma...
The distribution of impact craters on the ejecta of Giordano Bruno, a recent (<10 Ma) 22-km ...
In September 1977, a crater studies workshop was held for the purpose of developing standard data an...
This extended conference abstract describes a new geological map and crater size-frequency distribut...
This extended conference abstract describes geological mapping of the Apollo 17 landing site in the ...
The shape of the size-frequency distribution for small (<= 1 km diameter) primary craters coul...
This journal article describes geological mapping of the Apollo 12 landing site in the context of ne...
This extended conference abstract discusses the age and origin of the lunar northern light plains ba...
The threat of destructive impact events on Earth is mirrored in more than 160 proven impact structur...
This extended conference abstract describes progress being made on new geological maps of the Apollo...
Boulders represent a landing hazard that must be addressed in the planning of future landings on the...
It is shown that the size-frequency distribution (SFD) of a time-averaged projectile population deri...
The log normal frequency distribution law was used to analyze the crater population on the surface o...
By using high-resolution altimetric measurements of the Moon, we produced a catalog of all impact cr...
Recently it could be shown (Scholkmann, Prog. in Phys. , 2016, v. 12(1), 26-29) that the impact c...
The size-frequency distribution (SFD) of craters on the Moon, Mars, and Mercury turns up at very sma...
The distribution of impact craters on the ejecta of Giordano Bruno, a recent (<10 Ma) 22-km ...
In September 1977, a crater studies workshop was held for the purpose of developing standard data an...
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