Zobrazeno 1 - 10
of 55
pro vyhledávání: '"S. A. Good"'
Autor:
J. R. Siddorn, S. A. Good, C. M. Harris, H. W. Lewis, J. Maksymczuk, M. J. Martin, A. Saulter
Publikováno v:
Ocean Science, Vol 12, Iss 1, Pp 217-231 (2016)
Ocean monitoring and forecasting services are increasingly being used by a diverse community of public and commercial organizations. The Met Office, as the body responsible for severe weather prediction, has for many years been involved in providing
Externí odkaz:
https://doaj.org/article/292f300ff39c4f07acea1de495478b12
Publikováno v:
The Astrophysical Journal Letters, Vol 956, Iss 1, p L30 (2023)
Interplanetary coronal mass ejections (ICMEs) have low proton beta across a broad range of heliocentric distances and a magnetic flux rope structure at large scales, making them a unique environment for studying solar wind fluctuations. Power spectra
Externí odkaz:
https://doaj.org/article/e6b9f6ac310e4bc984b9753fb1b1754b
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 9 (2022)
Sheath regions of interplanetary coronal mass ejections (ICMEs) are formed when the upstream solar wind is deflected and compressed due to the propagation and expansion of the ICME. Small-scale flux ropes found in the solar wind can thus be swept int
Externí odkaz:
https://doaj.org/article/1a656ff6b165488598917518c4e8c76e
Autor:
E. K. J. Kilpua, D. Fontaine, S. W. Good, M. Ala-Lahti, A. Osmane, E. Palmerio, E. Yordanova, C. Moissard, L. Z. Hadid, M. Janvier
Publikováno v:
Annales Geophysicae, Vol 38, Pp 999-1017 (2020)
In this work, we investigate magnetic field fluctuations in three coronal mass ejection (CME)-driven sheath regions at 1 AU, with their speeds ranging from slow to fast. The data set we use consists primarily of high-resolution (0.092 s) magnetic
Externí odkaz:
https://doaj.org/article/d924c28382cf47a0819eb633cedea544
Autor:
P. C. Stoy, T. S. El-Madany, J. B. Fisher, P. Gentine, T. Gerken, S. P. Good, A. Klosterhalfen, S. Liu, D. G. Miralles, O. Perez-Priego, A. J. Rigden, T. H. Skaggs, G. Wohlfahrt, R. G. Anderson, A. M. J. Coenders-Gerrits, M. Jung, W. H. Maes, I. Mammarella, M. Mauder, M. Migliavacca, J. A. Nelson, R. Poyatos, M. Reichstein, R. L. Scott, S. Wolf
Publikováno v:
Biogeosciences, Vol 16, Pp 3747-3775 (2019)
Evaporation (E) and transpiration (T) respond differently to ongoing changes in climate, atmospheric composition, and land use. It is difficult to partition ecosystem-scale evapotranspiration (ET) measurements into E and T, which makes it difficult t
Externí odkaz:
https://doaj.org/article/e29a5322b10c4e0088c414eb119ee725
Publikováno v:
Hydrology and Earth System Sciences, Vol 22, Pp 3229-3243 (2018)
Vegetation controls on soil moisture dynamics are challenging to measure and translate into scale- and site-specific ecohydrological parameters for simple soil water balance models. We hypothesize that empirical probability density functions (pdfs
Externí odkaz:
https://doaj.org/article/ae04e3716a604261b8e06ffa84ce843c
Autor:
B. Li, S. P. Good
Publikováno v:
Hydrology and Earth System Sciences, Vol 25, Pp 5029-5045 (2021)
The National Aeronautics and Space Administration (NASA) Soil Moisture Active-Passive (SMAP) mission characterizes global spatiotemporal patterns in surface soil moisture using dual L-band microwave retrievals of horizontal (TBh) and vertical (TBv) p
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bb66aa22efd0e64562e95485ecdbfe58
https://hess.copernicus.org/articles/25/5029/2021/hess-25-5029-2021.pdf
https://hess.copernicus.org/articles/25/5029/2021/hess-25-5029-2021.pdf
Publikováno v:
Biogeosciences, Vol 11, Iss 23, Pp 6939-6954 (2014)
Climate change is expected to modify intra-seasonal rainfall variability, arising from shifts in rainfall frequency, intensity and seasonality. These intra-seasonal changes are likely to have important ecological impacts on terrestrial ecosystems. Ye
Externí odkaz:
https://doaj.org/article/1d3825e704ec471cbe5468741c33bf3b
Interplanetary coronal mass ejections (ICMEs) contain magnetic field and velocity fluctuations across a wide range of scales. These fluctuations may be interpreted as Alfv\'enic wave packets propagating parallel or anti-parallel to the background mag
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b7ed425b092823d4d113fe6abcf4c443
http://arxiv.org/abs/2205.07751
http://arxiv.org/abs/2205.07751
Publikováno v:
Astronomy & Astrophysics
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=r3c4b2081b22::dbbd0477fc8b54def9e5313524dbd91e