Does canopy wetness matter? Evapotranspiration from a subtropical montane cloud forest in Taiwan          下载免费PDF全文

Hou‐Sen Chu  Shih‐Chieh Chang  Otto Klemm  Cheng‐Wei Lai  You‐Zhu Lin  Chi‐Chen Wu  Ji‐Yu Lin  Jhia‐Ying Jiang  Jiquan Chen  Johan F. Gottgens  Yue‐Joe Hsia 《水文研究》2014,28(3):1190-1214

Evapotranspiration (ET) and canopy wetness were measured over a 2‐year intensive field campaign at the Chi‐Lan Mountain cloud forest site in Taiwan. Eddy covariance and sap flow methods were applied to measure ET and tree sap flow of the endemic yellow cypress (Chamaecyparis obtusa var. formosana). ET was 553 mm yr^?1 over the study period with an annual rainfall and fog deposition of 4893 and 288 mm yr^–1, respectively. The duration of canopy wetness exceeded actual fog or rain events (mostly in the afternoon), and the intercepted water was evaporated later in the following dry morning. The cumulative wet duration accounted for 52% of time over the study period, which was longer than the duration of rainfall and fog altogether (41%). As it adapted to the extremely moist environment, the yellow cypress behaved in a wet‐enhanced/dry‐reduced water use strategy and was sensitive to short periods of dry atmosphere with high evaporation potential. During dry days, the sap flow rate rose quickly after dawn and led to conservative water use through midday and the afternoon. During periodically wet days, the canopy was mostly wetted in the morning, and the interception evaporation contributed largely to the morning ET. The initiation of morning sap flow was postponed 1–3 h, and the sap flow rate tended to peak later at midday. The midday canopy conductance was higher in the periodically wet days (10.6 mm s^–1) as compared with 7.6 mm s^?1 in the dry days. Consequently, the dry‐reduced water use strategy led to much lower annual ET with respect to the available energy (~46%) and high precipitation input (~11%). The moist‐adapted ecohydrology we report reveals the vulnerability of montane cloud forests to prolonged fog‐free periods. More research is urgently needed to better understand the resilience of these ecosystems and formulate adaptive management plans. Copyright © 2012 John Wiley & Sons, Ltd.  相似文献   

Larval Pacific Herring (Clupea pallasi) Survival in Suspended Sediment     

Frederick J. Griffin  Theresa DiMarco  Karl L. Menard  Joe A. Newman  Edmund H. Smith  Carol A. Vines  Gary N. Cherr 《Estuaries and Coasts》2012,35(5):1229-1236

Pacific herring early life stages provide good model systems for studying effects of suspended sediments on estuarine organisms. To investigate effects on the herring larval stage, we used environmentally relevant particle concentrations for San Francisco Bay (200?C400?mg/L of particles <50???m in size) and exposure times of 16?h in a novel two-pump sediment suspension mesocosm. There were no mortalities during the 16-h suspended sediment incubation. Following sediment exposure, larvae were cultured in sediment-free water for up to 10?days during which survival and condition were measured. None were affected by previous sediment treatment. Four criteria for larval condition included growth, heart rate, prey capture, and critical swimming velocity. These results provide a framework for implementing regulatory decisions on anthropogenic activities such as dredging.  相似文献   

Giant sandstone pipes record basin-scale liquefaction of buried dune sands in the Middle Jurassic of SE Utah     

Mads Huuse  Simon J. Shoulders  Dennis I. Netoff  Joe Cartwright 《地学学报》2005,17(1):80-85

Giant sandstone pipes crop out over a 20 000 km² area of SE Utah. They range from metres to decametres in diameter and crosscut more than 100 m of continental sediments. New and published observations, encompassing all known pipe localities in SE Utah, suggest that the pipes formed by upward movement of groundwater, sand and sediment blocks in response to liquefaction of buried dune sands. Pipe formation was most likely triggered by seismicity during a phase of Cordilleran shortening and regional tectonic reorganization in the late Middle Jurassic. The depth of liquefaction recorded by the pipes far exceeds depths usually considered in earthquake engineering.  相似文献   

Practical Corrosion and Incrustation Guide Lines for Water Wells     

Joe L. Mogg 《Ground water》1972,10(2):6-11

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The three-dimensional clustering of radio galaxies in the Texas–Oxford NVSS structure survey     

Kate Brand  Steve Rawlings  Gary J. Hill  Joseph R. Tufts 《Monthly notices of the Royal Astronomical Society》2005,357(4):1231-1254

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Deep Impact photometry of Comet 9P/Tempel 1     

Jian-Yang Li  Michael F. A'Hearn  Christopher J. Crockett  Carey M. Lisse  Lucy A. McFadden  Jessica M. Sunshine  Joe Veverka 《Icarus》2007,187(1):41-55

The photometric properties of the nucleus of Comet 9P/Tempel 1 are studied from the disk-resolved color images obtained by Deep Impact (DI). Comet Tempel 1 has typical photometric properties for comets and dark asteroids. The disk-integrated spectrum of the nucleus of Tempel 1 between 309 and 950 nm is linear without any features at the spectral resolution of the filtered images. At V-band, the red slope of the nucleus is 12.5±1% per 100 nm at 63° phase angle, translating to B-V=0.84±0.01, V-R=0.50±0.01, and R-I=0.49±0.02. No phase reddening is confirmed. The phase function of the nucleus of Tempel 1 is constructed from DI images and earlier ground-based observations found from the literature. The phase coefficient is determined to be β=0.046±0.007 mag/deg between 4° and 117° phase angle. Hapke's theoretical scattering model was used to model the photometric properties of this comet. Assuming a single Henyey-Greenstein function for the single-particle phase function, the asymmetry factor of Tempel 1 was fitted to be g=−0.49±0.02, and the corresponding single-scattering albedo (SSA) was modeled to be 0.039±0.005 at 550 nm wavelength. The SSA spectrum shows a similar linear slope to that of the disk-integrated spectrum. The roughness parameter is found to be 16°±8°, and independent of wavelength. The Minnaert k parameter is modeled to be 0.680±0.014. The photometric variations on Tempel 1 are relatively small compared to other comets and asteroids, with a ∼20% full width at half maximum of albedo variation histogram, and ∼3% for color. Roughness variations are evident in one small area, with a roughness parameter about twice the average and appearing to correlate with the complex morphological texture seen in high-resolution images.  相似文献   

On the ability to estimate narrow-band signal parameters usingtowed arrays     

Edelson  G.S. Tufts  D.W. 《Oceanic Engineering, IEEE Journal of》1992,17(1):48-61

Using the Cramer-Rao lower bound (CRLB) as an indicator of potential performance, the limits on the estimation and resolution capabilities of a towed line array of uniformly spaced hydrophones to provide frequency and bearing information about narrowband signals are examined. It is assumed that a monochromatic plane wave arrives at the array for each source. Several versions of the bounds are computed using different assumptions about which parameters have known values and about the way in which the samples are taken in space and in time. It is shown that the CRLB values for different situations can be compared to provide information about the effective use of a moving aperture for estimation of the parameters of narrowband signals arriving at the array. It is also shown that adding at least one hydrophone occupying a fixed position in space can improve the bearing estimates of a towed array by supplying additional frequency information if both the bearings and frequencies of the sources are unknown  相似文献   

The Source Regions of Impulsive Solar Electron Events   总被引：1，自引：0，他引：1  

Benz  Arnold O.  Lin  Robert P.  Sheiner  Olga A.  Krucker  Säm  Fainberg  Joe 《Solar physics》2001,203(1):131-144

Low-energy (2–19 keV) impulsive electron events observed in interplanetary space have been traced back to the Sun, using their interplanetary type III radiation and metric/decimetric radio-spectrograms. For the first time we are able to study the highest frequencies and thus the radio signatures closest to the source region. All the selected impulsive solar electron events have been found to be associated with an interplanetary type III burst. This allows to time the particle events at the 2 MHz plasma level and identify the associated coronal radio emissions. Except for 5 out of 27 cases, the electron events were found to be associated with a coronal type III burst in the metric wavelength range. The start frequency yields a lower limit to the density in the acceleration region. We also search for narrow-band spikes at the start of the type III bursts. In about half of the observed cases we find metric spikes or enhancements of type I bursts associated with the start of the electron event. If interpreted as the plasma emission of the acceleration process, the observed average frequency of spikes suggests a source density of the order of 3×10⁸ cm^–3 consistent with the energy cut-off observed.  相似文献   

Sleeping with the past? Heritage,recreation and transition in New Zealand tramping huts     

Robin Kearns  Joe Fagan 《New Zealand geographer》2014,70(2):116-130

New Zealand tramping huts are a rudimentary but valued form of recreational accommodation. While huts fundamentally offer shelter, their aesthetics and history can also be valued. We review the origins of the huts system and draw on entries in visitor books to demonstrate divergent views regarding newer and more traditional huts. We conclude that while ‘new‐generation’ huts facilitate a broader spectrum of users, ‘heritage’ huts may need partnerships with user groups and corporate sponsorship to ensure their survival.  相似文献   

Numerical study of mean flow patterns in the South China Sea and the Luzon Strait   总被引：2，自引：1，他引：1  

Ching-Sheng Chern  Sen Jan  Joe Wang 《Ocean Dynamics》2010,60(5):1047-1059

Previous investigations have suggested that wind stress curl, the balance of influx- and outflux-induced upwelling, as well as a positive vorticity source fed from the left flank of the Kuroshio are all possible mechanisms that contribute to a persistent cyclonic gyre in the South China Sea (SCS). Studies have also suggested that the loop current that forms from the Kuroshio intrusion in the Luzon Strait, similar to the Loop Current in the Gulf of Mexico (GOM), has rarely been observed in the northern SCS. In this research, an idealized numerical model driven by annual mean wind stress was adopted to investigate the relative importance of dynamic processes that control the mean flow pattern of Kuroshio in the Luzon Strait and regulate circulation in the SCS. An analysis of results drawn from numerical experiments suggests that the three mechanisms are of approximately equal importance in the formation of the persistent cyclonic gyre in the northern SCS. Unlike the Gulf Stream which enters the Gulf of Mexico through the Yucatan Channel, the two topographic ridges that align nearly meridionally in the Luzon Strait keep the Kuroshio flowing roughly northward without distinct intrusion into the SCS. Unsurprisingly, an anticyclonic loop current similar to the Gulf Stream pathway in the GOM was barely observed in the northern SCS.  相似文献