Zobrazeno 1 - 10
of 14
pro vyhledávání: '"S. P. Good"'
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://doaj.org/article/ccc9ecb9ae2542208853dcab5b61acce
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
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
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
Publikováno v:
Canadian Journal of Fisheries and Aquatic Sciences. 58:1187-1195
We investigated the size-selective mortality of Atlantic salmon (Salmo salar) fry during two consecutive summers that differed markedly in weather conditions. We sampled fry shortly after emergence in June and at the end of August to compare the dist
Publikováno v:
Canadian Journal of Fisheries and Aquatic Sciences. 55:1663-1673
The development of the relationship between otolith and body size in Atlantic salmon (Salmo salar) between hatching and emergence was examined by repeatedly measuring individually identified fish. Otolith growth increments were deposited daily in the
Publikováno v:
Canadian Journal of Fisheries and Aquatic Sciences. 55:1674-1681
There is conflicting evidence on the role of size-selective mortality in the demography of populations of young sockeye salmon (Oncorhynchus nerka). A previous field study suggested that increases in mean fork length and otolith size at emergence obs
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