Tenders are invited for globe valves for hydrogen lines
On the first commissioning flight, EXES observed emissions from Jupiter's atmosphere in two molecular hydrogen lines
AM CVn stars differ from most other cataclysmic variables (CVs) in the lack of hydrogen lines
from their spectra.
A minor objection to the use of Stark broadening to explain the width of the hydrogen lines in the gaseous models rests on the fact that the appropriate experiments on hydrogen plasma do not exist.
Hydrogen lines were known to be extremely broad from the days of Henry Norris Russell and Donald H.
The central questions are three fold: 1) Why are the hydrogen lines broad?
1, concerning hydrogen line emission in the chromosphere, is completely unlike that currently postulated to exist within the gaseous Sun .
A sampling of topics: the microstructure of a sunspot penumbra, penumbral moving magnetic features, SOLIS-VSM solar vector magnetograms, multigrid methods for polarized radiative transfer, tunable narrow-band filter for imaging polarimetry, the diffraction limited spectro-polarimeter, a brief overview of the Second Solar Spectrum, polarizability factors for molecular bands, spectro-polarimetry of cool stars, molecular diagnostics of the internal structure of starspots and sunspots, and the effect of turbulent electric fields on the scattering polarization of hydrogen lines
Tenders are invited for Supply of lobe valves for hydrogen lines
The hydrogen lines ofthe Balmer series, and, as Babcock has recently shown, ofthe Paschen series as well, are very strong in the Sun, though the energy required to put an atom into condition to absorb these series is, respectively, 10.
Today, the quest to link helium abundances and primordial nucleosynthesis has continued [26-30] using two lines of reasoning: 1) the analysis of anisotropy in the microwave background [132,133] and 2) the observation of helium and hydrogen lines from low-metallicity extragalactic HII regions [26,134-137].
The ramps were on the tank to protect a cable tray and two pressurization oxygen and hydrogen lines
during the dynamic portion of launch, which includes liftoff through about the first three minutes of the climb to orbit.