Results 171 to 180 of about 697,282 (295)
The image shows a black, white and red illustrated panel. Barbed wire loops above a sign reading ‘STATE CARE’ in the upper left, and a fist tattooed with ‘HATE’ appears in the upper right. Two smaller figures at left, one with a hand over her mouth and one crouched with her face hidden, sit in muted red and black tones.
Paora Moyle
wiley +1 more source
Modified Gravity: From Black Holes Entropy to Current Cosmology, 4th Edition. [PDF]
Bamba K.
europepmc +1 more source
ABSTRACT This scoping review maps how spirituality is operationalised within trauma care for adult refugees and asylum seekers. Following Arksey and O'Malley's (2005) five‐stage framework with PRISMA‐ScR reporting, 5 databases were searched, and 12 studies were included.
Ruying Shi +2 more
wiley +1 more source
Numerical Investigations of Low‐Latitude Ground Magnetic Fields Due To Cavity Mode Oscillations
Abstract Pi2 oscillations are known to be associated with cavity mode oscillations (CMOs) in the inner magnetosphere at low latitudes. CMOs can also be excited by interplanetary shocks on the dayside. We present results from a global linear MHD wave model in spherical coordinates that allows us to analyze these waves at equatorial latitudes.
K. Majmudar, R. L. Lysak, K. Takahashi
wiley +1 more source
The quintom theory of dark energy after DESI DR2. [PDF]
Cai Y, Ren X, Qiu T, Li M, Zhang X.
europepmc +1 more source
The Daily Atmospheric Ionospheric Limb Imager (DAILI) CubeSat Experiment
Abstract The Daily Atmospheric Ionospheric Limb Imager (DAILI) (Daily Atmospheric and Ionospheric Limb Imager) mission utilized a 6U CubeSat, deployed at about 410 km altitude in a 51‐degree orbit, to make simultaneous daytime limb measurements in two colors; at 630 nm to measure the OI (630 nm) redline and at 765 nm to measure the O2 ${\mathrm{O}}_{2}$
James H. Hecht +15 more
wiley +1 more source
The era of precision cosmology with voids. [PDF]
Contarini S, Verza G, Pisani A.
europepmc +1 more source
Abstract Variations in the solar wind, particularly those associated with interplanetary coronal mass ejections (ICMEs) and high‐speed streams (HSSs), drive geomagnetic disturbances that produce rapid changes in the ground magnetic field. These variations, commonly quantified by the time derivative of the horizontal magnetic field dBH/dt $\left({\text ...
José P. Marchezi +8 more
wiley +1 more source

