✦ LIBER ✦

Absolute ages of the lunar maria and large craters

✍ Scribed by Ralph B. Baldwin

Publisher: Elsevier Science
Year: 1969
Tongue: English
Weight: 786 KB
Volume: 11
Category: Article
ISSN: 0019-1035
DOI: 10.1016/0019-1035(69)90065-7

No coin nor oath required. For personal study only.

📜 SIMILAR VOLUMES

A stochastic model of the formation and

A stochastic model of the formation and survival of lunar craters: III. Filling and disappearance of craters

✍ A.H. Marcus 📂 Article 📅 1966 🏛 Elsevier Science 🌐 English ⚖ 817 KB

A stochastic model of the formation and

A stochastic model of the formation and survival of lunar craters: IV. On the nonrandomness of crater centers

✍ A.H. Marcus 📂 Article 📅 1966 🏛 Elsevier Science 🌐 English ⚖ 648 KB

A stochastic model of the formation and

A stochastic model of the formation and survival of lunar craters: V. Approximate diameter distribution of primary and secondary craters

✍ Allan H. Marcus 📂 Article 📅 1966 🏛 Elsevier Science 🌐 English ⚖ 914 KB

The absolute photographic brightness of

The absolute photographic brightness of details of the lunar surface

✍ A. Markov 📂 Article 📅 1927 🏛 John Wiley and Sons 🌐 English ⚖ 462 KB

Terrestrial and lunar flux of large mete

Terrestrial and lunar flux of large meteorites in the last two billion years

✍ William K. Hartmann 📂 Article 📅 1965 🏛 Elsevier Science 🌐 English ⚖ 592 KB

Pulsed ENDOR Spectroscopy at Large Therm

Pulsed ENDOR Spectroscopy at Large Thermal Spin Polarizations and the Absolute Sign of the Hyperfine Interaction

✍ M.T. Bennebroek; J. Schmidt 📂 Article 📅 1997 🏛 Elsevier Science 🌐 English ⚖ 194 KB

It is shown that in pulsed Mims-type ENDOR experiments perthe conventional range of 9-35 GHz. The main advantages formed at 95 GHz and 1.2 K the sign of the ENDOR signal can are the high spectral resolution and the high absolute sensibe positive, corresponding to an increase of the stimulated echo t