Zobrazeno 1 - 10
of 17
pro vyhledávání: '"Amir Ouyed"'
Publikováno v:
Atmospheric Science Letters, Vol 24, Iss 5, Pp n/a-n/a (2023)
Abstract Mesoscale convective systems (MCSs) in the tropics play an integral role in the water cycle, are associated with local hazardous weather conditions, and have significant remote impacts on the midlatitude jet stream. Although it is known that
Externí odkaz:
https://doaj.org/article/00c4bf62280947019a871bfc3bc2e8b1
Publikováno v:
Geophysical Research Letters, Vol 50, Iss 7, Pp n/a-n/a (2023)
Abstract The lack of measurements of three‐dimensional (3D) distribution of horizontal wind vectors is a major challenge in atmospheric science. Here, we develop an algorithm to retrieve winds for nine pressure levels at 1° grid spacing from 70°N
Externí odkaz:
https://doaj.org/article/b2e1d2ba01b74c2ca89317f52b3eddc2
Publikováno v:
Remote Sensing, Vol 14, Iss 18, p 4557 (2022)
The weather and climate over the coastal regions have received increasing attention because of substantial population growth, the rising sea level, and extreme weather. Satellite remote sensing provides global precipitation estimates (including coast
Externí odkaz:
https://doaj.org/article/6283b9bb31ba40759b8746d0cefb7d39
Publikováno v:
Physics Letters B, Vol 777, Iss , Pp 184-190 (2018)
We simulate and study the microphysics of combustion (flame burning) of two flavored quark matter (u,d) to three flavored quark matter (u,d,s) in a trapped neutrino regime applicable to conditions prevailing in a hot proto-neutron star. The reaction
Externí odkaz:
https://doaj.org/article/27b3d975b03e4cbfb463bd04eb1e14ea
Publikováno v:
Universe, Vol 5, Iss 6, p 136 (2019)
Hadron-quark combustion in dense matter is a central topic in the study of phases in compact stars and their high-energy astrophysics. We critically reviewed the literature on hadron-quark combustion, dividing them into a “first wave” that treats
Externí odkaz:
https://doaj.org/article/8f667e416ada4f4783a291b5ad90dd8f
Publikováno v:
Universe, Vol 4, Iss 3, p 51 (2018)
The hadron–quark combustion front is a system that couples various processes, such as chemical reactions, hydrodynamics, diffusion, and neutrino transport. Previous numerical work has shown that this system is very nonlinear, and can be very sensit
Externí odkaz:
https://doaj.org/article/2e3ecfd7d91e4aa5aed8f0a4e16e14fc
Publikováno v:
Journal of Applied Meteorology and Climatology. 60:1671-1684
Much of the errors of atmospheric motion vectors (AMV) may be a consequence of algorithms not incorporating dynamical information. A physics-informed, artificial intelligence algorithm was developed that corrects errors of moisture tracking AMV (from
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::7e5702539e3c6569e4d9614d3e883943
https://doi.org/10.1175/jamc-d-21-0070.1
https://doi.org/10.1175/jamc-d-21-0070.1
Publikováno v:
Physics Letters
Physics Letters B, Vol 777, Iss, Pp 184-190 (2018)
Physics Letters B, Vol 777, Iss, Pp 184-190 (2018)
We simulate and study the microphysics of combustion (flame burning) of two flavored quark matter (u, d) to three flavoured quark matter (u,d,s) in a trapped neutrino regime applicable to conditions prevailing in a hot proto-neutron star. The reactio
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c27e59c96f6b9d0ef4c4fdb48cd354d1
http://repo.scoap3.org/api
http://repo.scoap3.org/api
Publikováno v:
Nuclear Physics A. 941:241-254
This paper shows that the collision of the ejecta of an exploding neutron star (the Quark-Nova or QN) with the preceding Type II Supernova (SNII) ejecta synthesizes p-nuclei, r-process-like and s-process-like isotopes. The QN ejecta, rich in A > 130
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b153519897dd0107abb6fdcb1351e73a
https://doi.org/10.1016/j.nuclphysa.2015.07.005
https://doi.org/10.1016/j.nuclphysa.2015.07.005
FRBs are puzzling, millisecond, energetic radio transients with no discernible source; observations show no counterparts in other frequency bands. The birth of a quark star from a parent neutron star experiencing a quark nova - previously thought und
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c352ae8a0f2f4b504c9d7f341e76c705
http://arxiv.org/abs/1505.08147
http://arxiv.org/abs/1505.08147
