Coupled plasma source... Matrix effects were found to be dependent on the coupling geometry of the rf power to the torch, observation height, emitting Ca species and EIEs ma-trix nature but independent from Al as regards its salt origin....
Solar physics doi: 10.1007/•••••-•••-•••-••••-• properties of high-frequency wave power halos around active regions: an analysis of multi-height data from hmi and aia onboard sdo.... Here we study in detail, in comparison with HMI Doppler data, properties of the power maps, especially the so called “acoustic halos ” seen around active regions, as a function of wave frequencies, inclination, and strength of magnetic field (derived from the vector-field observations by HMI) and observation height....
Turbulence regimes and turbulence intermittency in the stable boundary layer during cases-99...http://www.ametsoc.org/.An investigation of nocturnal intermittent turbulence during the Cooperative Atmosphere Surface Exchange Study in 1999 (CASES-99) revealed three turbulence regimes at each observation height: 1) regime 1, a weak turbulence regime when the wind speed is less than a threshold value; 2) regime 2, a strong turbulence regime when the wind speed exceeds...
The effect of the carrier gas flow rate and observation height on analyte emission in an argon icpThis paper reports on the influence of the carrier gas flow rate and observation height on electron number density, excitation temperature, and the departure from LTE in an argon ICP....
