Temperature emission spectrum of exoelectrons of lunar regolith

Details Temperature emission spectrum of exoelectrons of lunar regolith Temperature emission spectrum of exoelectrons of lunar regolith

Oct 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974lssf.nasa..528m&link_type=abstract

"In its Lunar Soil from the Sea of Fertility (NASA-TT-F-15881) p 528-537 (SEE N75-11814 02-91) Transl. into ENGLISH from the bo

Computer Science

Electron Emission, Emission Spectra, Heat Treatment, Lunar Soil, Anorthosite, Breccia, Gabbro, Glass, Lunar Rocks, Lunar Surface, Lunik 16 Lunar Probe, Olivine, Spherules

Scientific paper

Thermostimulated exoelectronic emission of eight fragments of regolith returned by the Soviet Luna 16 automatic station was studied. The nature of the exoemission glove-curves was determined by particle type. Fragments of breccia, sinter, slag, anorthosite, glass plate, and leucocratic gabbro after the first heating disclosed a single exoemission maximum, whose temperature position is in the range 115 to 200 C. The data obtained indicate the complex and inhomogeneous energy structure of some regolith fragments. The presence of surface states capable of forming sorptive bonds can be assumed for most particles. The exoemission of anorthosite, olivine, and the glass spherule is due to the presence of formation defects at their surfaces.

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