Results 181 to 190 of about 697,282 (295)
Everyone wants something better than ΛCDM. [PDF]
Turner MS.
europepmc +1 more source
Cosmic Ray Anisotropy Generated by the June 22nd 2015 Interplanetary Events
Abstract On 22 June 2015, the near Earth interplanetary space was perturbed by a series of high‐speed streamers and interplanetary coronal mass ejections associated with an active region and two low‐latitude coronal holes. The interaction of these disturbances gave rise to the complex solar wind structure observed at 1 au.
A. Lara, K. P. Arunbabu, T. Niembro
wiley +1 more source
f(Q) gravity as a possible resolution of the H<sub>0</sub> and S<sub>8</sub> tensions with DESI DR2. [PDF]
Kavya NS, Swagat Mishra S, Sahoo PK.
europepmc +1 more source
Intra‐Tessera Plains: Implications of Their Radar Properties for Surface Processes on Venus
Abstract Intra‐tessera plains are radar‐dark plains deposits that occur within tesserae. Their emplacement mechanism(s) and composition are poorly constrained, though they are hypothesized to be basaltic lava flows. Here, we map intra‐tessera plains within 16 different tesserae spanning various latitudes and elevations.
E. N. Haas, J. L. Whitten
wiley +1 more source
Black hole information turbulence and the Hubble tension. [PDF]
Cabrera Fernández JL.
europepmc +1 more source
The Role of Chlorate‐Driven Oxidative Weathering in Shaping Clay Deposits on Mars
Abstract Oxidized clays and the widespread Al/Si‐over‐Fe/Mg stratigraphy on Mars imply prolonged water‐rock interactions and efficient oxidative weathering despite the largely anoxic conditions of Early Mars when most deposits formed during the climate optimum.
Jiawei Wang, Nicole M. Fernandez
wiley +1 more source
Generating solutions for charged compact configurations in f(R) gravity. [PDF]
Noureen I, Mardan SA, Zahra A, Anwar I.
europepmc +1 more source
Ferric Chloride: The Venusian Unknown UV Absorber?
Abstract Near‐ultraviolet imaging of the planet Venus reveals inhomogeneous absorption features in the otherwise bright clouds. This absorption has been studied for nearly 100 years, but identification of the near‐UV absorber remains one of the largest open questions in Venusian research.
Joanna V. Egan +8 more
wiley +1 more source
The abundance and radial distribution of faint and ultra-faint dwarfs in galaxy clusters. [PDF]
Sadhu P +5 more
europepmc +1 more source

