RESUMO
For most materials science oriented applications incoherent cathodoluminescence (CL) is of main interest, for which the recombination of electron-hole pairs yields the emission of light. However, the incoherent signal is superimposed by coherently excited photons, similar to the situation for X-rays in Energy-Dispersive X-ray spectra (EDX). In EDX two very different processes superimpose in each spectrum: Bremsstrahlung and characteristic X-ray radiation. Both processes yield X-rays, however, their origin is substantially different. Therefore, in the present CL study we focus on the coherent emission of light, in particular Cerenkov radiation. We use a 200µm thick GaAs sample, not electron transparent and therefore not acting as a light guide, and investigate the radiation emitted from the top surface of the sample generated by back-scattered electrons on their way out of the specimen. The CL spectra revealed a pronounced peak corresponding to the expected interband transition. This peak was at 892 nm at room temperature and shifted to 845 nm at 80 K. The coherent light emission significantly modifies the shape of CL spectra at elevated beam energies. For the first time, by the systematic variation of current and energy of primary electrons we could distinguish the coherent and incoherent light superimposed in CL spectra. These findings are essential for the correct interpretation of CL spectra in STEM. The Cerenkov intensity as well as the total intensity in a spectrum scales linearly with the beam current. Additionally, we investigate the influence of asymmetric mirrors on the spectral shapes, collecting roughly only half of the whole solid angle. Different emission behaviour of different physical causes thus lead to changes in the overall spectral shape.
RESUMO
We launched a cryptoendolithic habitat, made of a gneissic impactite inoculated with Chroococcidiopsis sp., into Earth orbit. After orbiting the Earth for 16 days, the rock entered the Earth's atmosphere and was recovered in Kazakhstan. The heat of entry ablated and heated the rock to a temperature well above the upper temperature limit for life to below the depth at which light levels are insufficient for photosynthetic organisms ( approximately 5 mm), thus killing all of its photosynthetic inhabitants. This experiment shows that atmospheric transit acts as a strong biogeographical dispersal filter to the interplanetary transfer of photosynthesis. Following atmospheric entry we found that a transparent, glassy fusion crust had formed on the outside of the rock. Re-inoculated Chroococcidiopsis grew preferentially under the fusion crust in the relatively unaltered gneiss beneath. Organisms under the fusion grew approximately twice as fast as the organisms on the control rock. Thus, the biologically destructive effects of atmospheric transit can generate entirely novel and improved endolithic habitats for organisms on the destination planetary body that survive the dispersal filter. The experiment advances our understanding of how island biogeography works on the interplanetary scale.
