Results 51 to 60 of about 1,078,179 (287)
, 2012 We study effects of the fully ionized initial state, or pre-ionization, on the subsequent thermal evolution of low-metallicity clouds under various intensities of the external far-ultraviolet(FUV) and cosmic-ray(CR) fields.
Omukai, Kazuyuki
core +1 more source
Mars thermal history based on its tectonic and structural systems [PDF]
Geofísica Internacional, 2002 We suggest an interpretation of the thermal history of Mars base on crustal deformations. Local deformations are associated with an increase of the thermal gradient with time and indicate tensional stresses in eruptive centers such as Alba Patera ...
J. Urrutia-Fucugauchi +2 more
doaj
Present‐Day Mars' Seismicity Predicted From 3‐D Thermal Evolution Models of Interior Dynamics
Geophysical Research Letters, 2018 The Interior Exploration using Seismic Investigations, Geodesy and Heat Transport mission, to be launched in 2018, will perform a comprehensive geophysical investigation of Mars in situ.
A.‐C. Plesa +8 more
doaj +1 more source
Геодинамика и тектонофизика, 2020 We present the first results of fission-track dating of apatite monofractions from two rock samples taken from the Southern carbonatite massif of the world’s largest alkaline ultrabasic Guli pluton (~250 Ma), located within the Maymecha-Kotuy region of ...
M. S. Myshenkova +6 more
doaj +1 more source
Quiescent thermal emission from neutron stars in LMXBs [PDF]
, 2015 We monitored the quiescent thermal emission from neutron stars in low-mass X-ray binaries after active periods of intense activity in x-rays (outbursts).
Aguilera, Deborah N. +2 more
core +3 more sources
Thermal evolution of lava planets
Monthly Notices of the Royal Astronomical SocietyABSTRACT Rocky planets typically form with a transient magma ocean. Lava planets, however, maintain a permanent day-side magma ocean. The extent of this magma ocean depends on the planet’s thermal history. We present numerical simulations of the thermal history of tidally locked lava planets over 10 billion years, starting from a ...
Mahesh Herath +2 more
openaire +2 more sources
RHESSI images and spectra of two small flares
, 2005 We studied the evolution of two small flares (GOES class C2 and C1) that developed in the same active region with different morphological characteristics: one is extended and the other is compact. We analyzed the accuracy and the consistency of different
A. Falchi +25 more
core +2 more sources
Hardness, grainsize and porosity formation prediction on the Laser Metal Deposition of AISI 304 stainless steel [PDF]
, 2018 The presented numerical model solves the heat and mass transfer equations in the Laser Metal Deposition process and based on the evolution of the thermal field predicts the grainsize, the resulting hardness and evaluates the pores formation probability ...
Alberdi, Amaia +4 more
core +3 more sources
Pediatric Blood &Cancer, EarlyView.ABSTRACT Background Survivors of childhood acute lymphoblastic leukemia (ALL) often exhibit early deficits in muscle and movement competence, which can compromise long‐term health. Integrative neuromuscular training (INT), a multifaceted approach combining fundamental movement activities with strength exercises, may help address these deficits during ...
Anna Maria Markarian +7 more
wiley +1 more source
Time Evolution of an Infinite Projected Entangled Pair State: an Efficient Algorithm [PDF]
, 2019 An infinite projected entangled pair state (iPEPS) is a tensor network ansatz to represent a quantum state on an infinite 2D lattice whose accuracy is controlled by the bond dimension $D$.
Corboz, Philippe +2 more
core +2 more sources