First detection of the O III 495.8911 and 500.6843 nm lines in the Earth’s upper atmosphere

work has been realized previously and allows characterizing nitrogen or oxygen incorporation in tholins produced in various gaseous mixtures. This would allow characterizing

Indeed in the case of a 10 nm diameter sphere, the electrostatic interaction is mostly covered by Brownian motion noise and makes it difficult to perform a precise force

The noise properties of the stabilized laser emission are investigated in order to evaluate the contribution of the dual frequency OP-VECSEL to the performance

Regardless of the sources and geochemical cycle of lithium in hydrogeological systems, an understanding of its thermodynamic properties and its geochemical behavior is

Pyrroloindolizine structures with a Lewis base substituent at C8 are predisposed to generate azafulvenium ions upon electrophilic activation (Scheme 1). This reactivity enables a

During a planetary transit, atoms with high atomic number absorb short-wavelength radiation in the upper atmosphere, and the planet should appear larger during a primary

The subdivision of the Schumann-Runge spectral range adopted in the preceding sections is based on the physical structure (individual bands) of the ab- sorption

For daytime conditions (see Fig. 5) a small cooling, previously unnoticed, appears below this heating zone. Since atomic oxygen disappears very quickly below 80 km