Results 71 to 80 of about 927 (171)
Characterization of Shallow Sedimentary Layers in the Oran Region Using Ambient Vibration Data
This study investigates the structure of shear-wave velocities (Vs) in the shallow layers of the Oran region, north-west of Algeria, using non-invasive techniques based on ambient vibration arrays. The region has experienced several moderate earthquakes,
Ahmed Saadi +4 more
doaj +1 more source
Author Correction: In situ recording of Mars soundscape. [PDF]
Maurice S +42 more
europepmc +1 more source
Multiplatform Computing of Transition Probabilities in Os V
Osmium is an element of the Periodic Table with an atomic number Z equal to 76. In Tokamaks with divertors made of tungsten (Z=74), it is produced in the neutron-induced transmutation of the latter.
Patrick Palmeri +5 more
doaj +1 more source
Using the Multiconfiguration Dirac–Hartree–Fock method as implemented in the General Relativistic Atomic Structure Package, the magnetic dipole and electric quadrupole hyperfine structure constants were determined for the ground and first excited levels ...
Lorenzo Nezosi +4 more
doaj +1 more source
Ground magnetic field measurements are an important tool to determine the strength of space weather events in the terrestrial environment on local and global scales. For that purpose, geomagnetic baselines play a vital role as they describe typical quiet
Veronika Haberle +3 more
doaj +1 more source
Far-infrared to centimeter emission of very nearby galaxies with archival data
Compared to the well-studied infrared and radio domains, galaxy emission in the range from a few millimeters (mm) to centimeters (cm) (300−30 GHz) has been observed less frequently.
Correia L. +11 more
doaj +1 more source
The new gravimetric network of the north-eastern part of Algeria. [PDF]
Bayou Y +3 more
europepmc +1 more source
Color dichotomy and gradients in the bulges and disks of EFIGI galaxies along the Hubble sequence
Context. One of the most outstanding questions in contemporary astrophysics is: What is the significance of galaxy morphology? What physical processes underlie the morphologies we observe and is a galaxy’s internal structure shaping its evolution (nature)
Quilley L. +2 more
doaj +1 more source
Les réactions nucléaires importantes en astrophysique
On examine les réactions nucléaires importantes pour la compréhension de la production d'énergie et de la composition chimique des étoiles. Nous donnons les énergies dans le système du centre de gravité. (a) Les réactions des étoiles de la séquence principale ont lieu vers quelques keV ; (b) les réactions avec les particules α dans les géantes ont lieu
openaire +2 more sources
On Restrictions of Current Warp Drive Spacetimes and Immediate Possibilities of Improvement
Looking at current proposals of so-called ‘warp drive spacetimes’, they appear to employ General Relativity only at an elementary level. A number of strong restrictions are imposed such as flow-orthogonality of the spacetime foliation, vanishing spatial ...
Hamed Barzegar, Thomas Buchert
doaj +1 more source

