Sulphur compounds in the atmosphere of Venus. 1 - An upper limit for the abundance of sulphur dioxide
Sulfur dioxide abundance in Venus atmosphere determined from infrared spectra
SEARCH · Engineering Papers
Search indexed NASA NTRS and DOE OSTI research on propulsion, heat transfer, battery materials and energy systems. Follow report and document links to the original sources.
Quote a phrase for an exact phrase match. Source license links do not imply unrestricted reuse.
Sulfur dioxide abundance in Venus atmosphere determined from infrared spectra
Carbonyl and hydrogen sulfide abundance in Venus atmosphere determined from infrared spectra
Satellite data evaluated for relative helium abundance and plasma properties in solar wind
Age and initial helium abundance of stars in M15 globular clusters estimated from stellar evolution lifetime ratio
Solar coronal ion abundance analyses from extreme UV emission lines
Spectra of close binary systems, analyzing abundance anomalies, noting metallicity results
Cosmic ray nuclei energy spectra and abundances above 20 Mev/nucleon determined by OGO-1 satellite experiment, considering He, B, C, N, O, Ne, Mg, Si, Mn, Fe, Co and Ni
Solar photosphere abundances of various heavy elements from photoelectric spectrometer measurements of equivalent width of known Fraunhofer lines
Solar system elements abundance compilation based on carbonaceous chondrites and nucleosynthesis in stars
Indium abundances in chondritic and achondritic meteorites and terrestrial rocks determined by radiochemical neutron activation analysis
Chemical abundances in planetary atmospheres based on spectroscopic determinations, considering terrestrial and Jovian planets
Continental diabases and oceanic tholeiites in light of rare earth and barium abundances and partition coefficients indicating fusion process
Element abundances of sharp lined field early A stars using model atmosphere
Carbon dioxide abundance in Mars atmosphere measured with three etalon Fabry-Perot spectrometer
Aluminum abundances in stony meteorites measured using nondestructive instrumental neutron activation analysis
Light ion abundance measurements of OGO satellites and field aligned diffusive equilibrium theory with temperature and concentration latitudinal variations
Ionization stratification and chemical abundances in planetary nebula NGC 7662, discussing density fluctuations effect on N II and O II lines