Zobrazeno 1 - 10
of 115
pro vyhledávání: '"M G, Evans"'
Autor:
J P, Ritson, O, Kennedy-Blundell, J, Croft, M R, Templeton, C E, Hawkins, J M, Clark, M G, Evans, R E, Brazier, D, Smith, N J D, Graham
Publikováno v:
Environmental monitoring and assessment. 194(11)
High frequency ultraviolet - visible (UV-VIS) sensors offer a way of improving dissolved organic carbon (DOC) load estimates in rivers as they can be calibrated to DOC concentration. This is an improvement on periodic grab sampling, or the use of pum
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=pmid________::c42ece19872a672a4de04d56e4458a1c
https://pubmed.ncbi.nlm.nih.gov/36163406
https://pubmed.ncbi.nlm.nih.gov/36163406
Fibrocyte degeneration in the cochlear lateral wall is one possible pathology of age-related metabolic hearing loss (presbycusis). Within the lateral wall fibrocytes play a role in potassium recycling and maintenance of the endocochlear potential. It
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fa1642893b2e219ebffe52b76e192685
https://eprints.keele.ac.uk/10469/7/Osborn2022_Article_ElectricalAndImmunohistochemic.pdf
https://eprints.keele.ac.uk/10469/7/Osborn2022_Article_ElectricalAndImmunohistochemic.pdf
Publikováno v:
Hydrology and Earth System Sciences, Vol 12, Iss 2, Pp 625-634 (2008)
This study investigates for the first time the relative importance of dissolved organic carbon (DOC) and particulate organic carbon (POC) in the fluvial carbon flux from an actively eroding peatland catchment in the southern Pennines, UK. Event scale
Externí odkaz:
https://doaj.org/article/1859a4e9e9684ed8853e41ae5dfa614c
Publikováno v:
Journal of Literature and Art Studies. 11
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::19bf5235e8cef41eff5b53a487b5e520
https://doi.org/10.17265/2159-5836/2021.04.008
https://doi.org/10.17265/2159-5836/2021.04.008
Autor:
Frederick M. G. Evans, James Shumpert
Publikováno v:
Journal of Literature and Art Studies. 10
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::66a6e11cd54b96213cc9c5b5e78098cf
https://doi.org/10.17265/2159-5836/2020.02.011
https://doi.org/10.17265/2159-5836/2020.02.011
Publikováno v:
HardwareX. 8
Understanding the spatial variability of gaseous carbon flux at a landscape scale requires intensive monitoring campaigns necessitating significant and perhaps prohibitive financial investment. Commercially available CO
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=pmid________::85c0dbe23bd74490469ad50a1ed64042
https://pubmed.ncbi.nlm.nih.gov/35498252
https://pubmed.ncbi.nlm.nih.gov/35498252
Autor:
A. C. Boley, Paola Caselli, T. W. Hartquist, Cassandra Hall, Catherine Clarke, Richard A. Booth, John D. Ilee, J. M. C. Rawlings, M. G. Evans, Duncan Forgan, Wkm Rice
Publikováno v:
Monthly Notices of the Royal Astronomical Society
NASA Astrophysics Data System
NASA Astrophysics Data System
In this paper, we model the chemical evolution of a 0.25 M$_{\odot}$ protoplanetary disc surrounding a 1 M$_{\odot}$ star that undergoes fragmentation due to self-gravity. We use Smoothed Particle Hydrodynamics including a radiative transfer scheme,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::dfec81fbff77daf2a74f6528b194ac0f
https://doi.org/10.1093/mnras/stx1966
https://doi.org/10.1093/mnras/stx1966
At the time of formation, protoplanetary discs likely contain a comparable mass to their host protostars. As a result, gravitational instabilities (GIs) are expected to play a pivotal role in the early phases of disc evolution. However, as these youn
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::07ff27eafebf1981b64fe5bf78a17d55
http://arxiv.org/abs/1810.04537
http://arxiv.org/abs/1810.04537
Publikováno v:
Journal of Literature and Art Studies. 7
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::139f3cae352717711d515af0ab03175b
https://doi.org/10.17265/2159-5836/2017.09.012
https://doi.org/10.17265/2159-5836/2017.09.012
Autor:
J. M. C. Rawlings, Richard H. Durisen, Paola Caselli, M. G. Evans, A. C. Boley, T. W. Hartquist, John D. Ilee
To date, most simulations of the chemistry in protoplanetary discs have used 1+1D or 2D axisymmetric $\alpha$-disc models to determine chemical compositions within young systems. This assumption is inappropriate for non-axisymmetric, gravitationally
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5aa097fc8db34cec3852de08cc67e96a
http://arxiv.org/abs/1508.00773
http://arxiv.org/abs/1508.00773