Zobrazeno 1 - 10
of 114
pro vyhledávání: '"E, Wiik"'
Autor:
M J, Whelan, C, Linstead, F, Worrall, S J, Ormerod, I, Durance, A C, Johnson, D, Johnson, M, Owen, E, Wiik, N J K, Howden, T P, Burt, A, Boxall, C D, Brown, D M, Oliver, D, Tickner
Publikováno v:
Science of The Total Environment, 2022, Vol.843 [Peer Reviewed Journal]
We explore the oft-repeated claim that river water quality in Great Britain is "better now than at any time since the Industrial Revolution". We review available data and ancillary evidence for seven different categories of water pollutants: (i) bioc
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::800e3c1d4bb0d1f3133b9f31a1ca7ced
http://dro.dur.ac.uk/36962/
http://dro.dur.ac.uk/36962/
Publikováno v:
Value in Health. 23:S450-S451
Publikováno v:
Value in Health. 20:A498-A499
Publikováno v:
Value in Health. 20:A499
Publikováno v:
Value in Health. 20:A499
Publikováno v:
Solar Physics. 227:283-297
The locations of barbs of quiescent solar filaments are compared with the photospheric/chromospheric network, which thereby serves as a proxy of regions with enhanced concentrations of magnetic flux. The study covers quiet regions, where also the pho
Publikováno v:
Solar Physics. 226:239-254
High-resolution images obtained in Hα with the new Swedish Solar Telescope at La Palma, Spain, have been used for studies of fine-scale threads in solar filaments. The widths of the thin threads are ≤0.3 arcsec. The fact that the width of the thin
Publikováno v:
Solar Physics. 216:109-120
The motion of small-scale structures is well resolved in high-resolution filament images that were observed on 19 June 1998 with the Swedish Vacuum Solar Telescope, La Palma. The filament was between 80 000 and 100 000 km high. The study is based on
Publikováno v:
Symposium - International Astronomical Union. 203:310-313
We have studied the temporal relationship between three selected prominence eruptions and their associated coronal mass ejections (CME). For these three events it is not possible to predict from the CME time history when the prominence would erupt. H
Publikováno v:
Solar Physics. 187:405-426
A quiescent polar crown prominence was observed at Meudon in Hα and Ca ii lines, and by EIT and SUMER on board SOHO in UV lines from 9 to 10 March 1996. SUMER observed the prominence continuously in a scanning mode between 21:40 UT on 9 March, and 1