Results 71 to 80 of about 173,010 (211)
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
This study identified that antler bone peptide‐calcium chelate promotes MC3T3‐E1 cell differentiation and mineralization. Two novel calcium‐chelating peptides were identified from antler bone hydrolysate with high chelation rates. Oxygen and nitrogen in the peptides' carboxyl and amino groups are involved in calcium binding, with a preference for ...
Zhaoguo Wang +7 more
wiley +1 more source
Abstract It was recently suggested that the Sun could switch to a high‐activity regime which would lead to a rise of ultraviolet radiation with an amplitude of about four times larger than the amplitude of an average solar activity cycle and a simultaneous drop in total solar irradiance.
Anna V. Shapiro +5 more
wiley +1 more source
Investigating the Temperature Sensitivity of UV Line Ratios in the 280 nm Region of Solar-like Stars
Stellar UV spectra are fundamental diagnostics of physical and magnetic properties of stars. For instance, lines like Mg ii at 280 nm serve as valuable indicators of stellar activity, providing insights into the activity levels of Sun-like stars and ...
Valentina Penza +9 more
doaj +1 more source
China's Ground‐Based Space Environment Monitoring Network—Chinese Meridian Project (CMP)
Abstract Monitoring and investigation of the solar‐terrestrial space environment is a huge challenge for humans in space age. To this end, China has established the Ground‐based Space Environment Monitoring Network, namely Chinese Meridian Project (CMP).
Chi Wang +6 more
wiley +1 more source
Double-edged Sword: The Influence of Tidal Interaction on Stellar Activity in Binaries
Using the LAMOST DR7 low-resolution spectra, we carried out a systematic study of stellar chromospheric activity in both single and binary stars. We constructed a binary sample and a single-star sample, mainly using the binary belt and the main sequence ...
Yuedan Ding +6 more
doaj +1 more source
Abstract The primary external energy input to planetary atmospheres comes from solar radiation. Accurate estimates of solar irradiance are needed in order to understand atmospheric conditions at other planets. Many studies have interpolated Earth‐based irradiance measurements at other planets, disregarding the evolution of solar features, which are ...
I. de Oliveira +3 more
wiley +1 more source
X-Shooter spectroscopy of young stellar objects in Lupus. Atmospheric parameters, membership and activity diagnostics [PDF]
A homogeneous determination of basic stellar parameters of young stellar object (YSO) candidates is needed to confirm their evolutionary stage, membership to star forming regions (SFRs), and to get reliable values of the quantities related to ...
Alcalà, J. M. +6 more
core +2 more sources
Nowcasting Solar EUV Irradiance With Photospheric Magnetic Fields and the Mg II Index
Abstract A new method to nowcast spectral irradiance in extreme ultraviolet (EUV) and far ultraviolet (FUV) bands is presented here, utilizing only solar photospheric magnetograms and the Mg II index (i.e., the core‐to‐wing ratio). The EUV and FUV modeling outlined here is a direct extension of the SIFT (Solar Indices Forecasting Tool) model, based on ...
Kara L. Kniezewski +2 more
wiley +1 more source
We report on intriguing photometric properties of Galactic stars observed in the GALEX satellite's far-UV and near-UV bandbasses as well as from the SDSS survey and the Kepler Input Catalog.
Bianchi, Luciana +2 more
core +1 more source

