Results 61 to 70 of about 151,165 (141)
Deriving the Coronal Separatrix‐Web With the WSA Model
Abstract We demonstrate a new capability of the Wang‐Sheeley‐Arge (WSA) model to routinely derive the coronal separatrix web (S‐web) as a standard data product. We describe our methodology for deriving the squashing factor (Q $Q$) and we use Carrington rotation (CR) 2109 to illustrate the validation of our output with that derived from the POT3D model.
Samantha Wallace +5 more
wiley +1 more source
The energy input mechanism into the lower transition regions between stellar chromospheres and coronae [PDF]
The ratio of the emission line fluxes for the C II and C IV lines in the lower transition regions (T = 30,000 to 100,000 K) between stellar chromospheres and transition layers is shown to depend mainly on the temperature gradient in the line emitting ...
Boehm-Vitense, Erika
core
Abstract Working toward the goal of understanding solar wind (SW) entry to the Earth's magnetosphere, this study examines solar‐origin ion composition in the magnetotail. During its trajectory, Wind spent a significant amount of time in the Earth's magnetotail, where its SupraThermal Ion Composition Spectrometer (STICS) measured the mass and mass per ...
S. Colón‐Rodríguez +3 more
wiley +1 more source
Studies of the local interstellar medium [PDF]
The existing ultraviolet and optical data concerning late-type stars are discussed along with the acquisition and reduction of additional ultraviolet and simultaneous ground-based observation.
Dupree, A. K.
core
In vitro analysis of noradrenaline, adrenaline and dopamine release in chromospheres and CC.
(a-b) Adrenaline, noradrenaline and dopamine release under basal conditions was determined by HPLC-ED in 3- and 9- days cultured-CC and 9 days cultured-chromospheres. 3 days CC and 9 days chromospheres were obtained from 8 independently processed adrenal
René Drucker-Colín (2950836) +4 more
core +1 more source
The Stagger Code for Accurate and Efficient, Radiation-coupled Magnetohydrodynamic Simulations
We describe the Stagger code for simulations of magnetohydrodynamic (MHD) systems. This is a modular code with a variety of physics modules that will let the user run simulations of deep stellar atmospheres, sunspot formation, stellar chromospheres and ...
Robert F. Stein +3 more
doaj +1 more source
Slow Solar Wind: Origin in an Independent Small‐Scale Solar Dynamo
Abstract Separation of the solar wind (SW) into three flow types (coronal mass ejections (CMEs), high speed streams (HSSs), and slow solar wind (SSW)) reveals an inverse relationship between the percentage of time Earth spends in SSW during a year and its annually averaged magnetic field strength (B).
E. W. Cliver +2 more
wiley +1 more source
Disentangling planetary orbits from stellar activity in radial-velocity surveys [PDF]
The majority of extra-solar planets have been discovered (or confirmed after follow-up) through radial-velocity (RV) surveys. Using ground-based spectrographs such as High Accuracy Radial Velocity Planetary Search (HARPS) and HARPS-North, it is now ...
Segransan, Damien +42 more
core +1 more source
Robust Statistical Techniques for Operational Maintenance of the 10.7 cm Solar Radio Flux
Abstract The F10.7 solar radio flux is a critical quantity for operational space weather nowcasting and forecasting, where it is routinely used as a driver for coupled atmospheric models to estimate a variety of important quantities such as the neutral atmospheric density.
Daniel A. Brandt +2 more
wiley +1 more source
In vitro analysis of the number of TH+ cells in chromospheres and CC.
(a-b) Confocal microscopy photographs showing double-immunofluorescence staining for TH (green, top right panel) and DBH (red, bottom left panel) in freshly isolated cells (a) and 9 days-chromospheres (b).
René Drucker-Colín (2950836) +4 more
core +1 more source

