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In the 19th century De la Rue, Stewart, and Loewy carried out a compilation of drawings and photographs of the solar sunspots corresponding to the interval 1832–1868. Using these drawings and photographs, they determined fortnightly values of the percentage of the solar photosphere covered by the sunspots. In this work, we have performed a spectral analysis of these data in order to determine possible periodic signals. In addition to the 11-year solar cycle, short cycles of about 330 days and 30–50 days have been recovered, lacking the 150–160 days period discovered by other authors using several solar activity indicators. 相似文献
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S. Fritz M. Massart I. Savin J. Gallego F. Rembold 《International Journal of Applied Earth Observation and Geoinformation》2008,10(4):453
Recent developments in remote sensing technology, in particular improved spatial and temporal resolution, open new possibilities for estimating crop acreage over larger areas. Remotely sensed data allow in some cases the estimation of crop acreage statistics independently of sub-national survey statistics, which are sometimes biased and incomplete. This work focuses on the use of MODIS data acquired in 2001/2002 over the Rostov Oblast in Russia, by the Azov Sea. The region is characterised by large agricultural fields of around 75 ha on average. This paper presents a methodology to estimate crop acreage using the MODIS 16-day composite NDVI product. Particular emphasis is placed on a good quality crop mask and a good quality validation dataset. In order to have a second dataset which can be used for cross-checking the MODIS classification a Landsat ETM time series for four different dates in the season of 2002 was acquired and classified. We attempted to distinguish five different crop types and achieved satisfactory and good results for winter crops. Three hundred and sixty fields were identified to be suitable for the training and validation of the MODIS classification using a maximum likelihood classification. A novel method based on a pure pixel field sampling is introduced. This novel method is compared with the traditional hard classification of mixed pixels and was found to be superior. 相似文献
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J.R. Gallego E. Gonzlez-Rojas A.I. Pelez J. Snchez M.J. García-Martínez J.E. Ortiz T. Torres J.F. Llamas 《Organic Geochemistry》2006,37(12):1869
Heavy fuel oil spilled from the oil tanker Prestige in November 2002 affected hundreds of km of Spanish shoreline. We carried out a two year study at two highly contaminated sites in order to monitor natural attenuation of the residues coating shore rocks and to test the effectiveness of bioremediation with an oleophilic fertilizer (S200). The methodology included an innovative approach for oil load calculation (based on image analysis techniques), the analysis of the fate of hydrocarbons by means of chemical biomarkers and different microbiological techniques for isolating and examining hydrocarbon degraders.Considerable hydrocarbon depletion from shorelines (≈100% for light-medium linear alkanes and ≈35% for aromatics such as pyrene) was observed within the first months after the spill. However, this natural attenuation effect dramatically slowed down in the following year, although partial enhancement (especially for the aromatic fraction) was attained as a result of the application of S200 to stimulate indigenous microorganisms. In addition, one of the main outcomes of this work concerns the remarkable hydrocarbon depletion achieved at points where fresh water flowed through the shore rocks. The study of samples collected where this natural attenuation phenomenon took place made it possible to isolate heterotrophic bacteria and fungi that are likely to cooperate with cyanobacteria in hydrocarbon biodegradation. The overall results strongly advocate the implementation of new bioremediation approaches, including alternatives such as the use of natural fresh water to irrigate polluted areas. 相似文献
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A typical agricultural water reservoir (AWR) of 2400 m2 area and 5 m depth, located in a semi‐arid area (southern Spain), was surveyed on a daily basis for 1 year. The annual evaporation flux was 102·7 W m?2, equivalent to an evaporated water depth of 1310 mm year?1. The heat storage rate G exhibited a clear annual cycle with a peak gain in April (G ～ 45 W m?2) and a peak loss in November (G ～ 40 W m?2), leading to a marked annual hysteretic trend when evaporation (λE) was related to net radiation (Rn). λE was strongly correlated with the available energy A, representing 91% of the annual AWR energy loss. The sensible heat flux H accounted for the remaining 9%, leading to an annual Bowen ratio in the order of 0·10. The equilibrium and advective evaporation terms of the Penman formula represented 76 and 24%, respectively, of the total evaporation, corresponding to a annual value of the Priestley–Taylor (P–T) coefficient (α) of 1·32. The P–T coefficient presented a clear seasonal pattern, with a minimum of 1·23 (July) and a maximum of 1·65 (December), indicating that, during periods of limited available energy, AWR evaporation increased above the potential evaporation as a result of the advection process. Overall, the results stressed that accurate prediction of monthly evaporation by means of the P–T formula requires accounting for both the annual cycle of storage and the advective component. Some alternative approaches to estimating Rn, G and α are proposed and discussed. Copyright © 2009 John Wiley & Sons, Ltd. 相似文献
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R. Nieto L. Gimeno J. A. Añel L. De la Torre D. Gallego D. Barriopedro M. Gallego A. Gordillo A. Redaño G. Delgado 《Meteorology and Atmospheric Physics》2007,96(1-2):103-119
Summary The Iberian Peninsula is one of the regions in the world with higher occurrence of cut-off low systems (COL). The aim of this
paper is to analyse the weather events (rainfall and cloudiness layer) associated to COLs in the Iberian Peninsula with tools
not previously used: (a) the use of the new multidecadal COLs database developed by Nieto et al (2005) that permit us to study
a 41 years period (1958–1998), (b) the checking of the expected weather events (rainfall and cloudiness layer) associated
with COLs in a conceptual model (Winkler et al, 2005) and (c) the extensive use of radiosoundings to analyse convective instability
in areas inside and close to the COL. Two points of view are used to make the analysis: (1) a source oriented method, when
a particular COL is followed and its associated precipitation and cloudiness is analysed over four quadrants in which Iberia
was divided and (2) a receptor oriented method, when the precipitation associated to COLs is analysed in given areas, defined
by patterns of precipitation. Results reveal that the precipitation and cloudiness patterns associated to COLs in the conceptual
model reproduce quite well the main characteristics found over the Iberian Peninsula. The generalized idea that most of the
COLs produce intense convective rainfall is show to be misleading. Convective phenomena are important usually when the centre
of the COL is located on the Mediterranean region. Most of the rainfall associated with COLs comes from the baroclinic shield;
specially in cases located over the west half of the Iberian Peninsula. It is shown that nearly 30% of COLs do not induce
any rainfall; most of them located in the southern half of the Peninsula, and mainly during autumn. Only 30% of COLs produce
generalized rainfall over the whole analysed territory, being most of them (about 90%) located over the western half of the
Iberian Peninsula. 相似文献
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Jesús Gallego 《Astrophysics and Space Science》1998,263(1-4):1-14
The evolution of the Star Formation Rate (SFR) density of the Universe as a function of look-back time is a fundamental parameter
in order to understand the formation and evolution of galaxies. The current picture, only outlined in the last years, is that
the global SFR density has dropped by about an order of magnitude from a redshift of z∼1.5 to the current value at z=0. Because
these SFR density studies are now extended to the whole range in redshift, it becomes mandatory to combine data from different
SFR tracers. At low redshifts, optical emission lines are the most widely used. Using Hα as current-SFR tracer, the Universidad
Complutense de Madrid (UCM) Survey provided the first estimation of the global SFR density in the Local Universe. The Hα flux
in emission is directly related to the number of ionizing photons and, modulo IMF, to the total mass of stars formed. Metallic
lines like [OII]λ3727 and [OIII]λ5007 are affected by metallicity and excitation. Beyond redshifts z∼0.4, Hα is not observable
in the optical and [OII]λ3727 or UV luminosities have to be used. The UCM galaxy sample has been used to obtain a calibration
between [OII]λ3727 luminosity and SFR specially suitable for the different types of star-forming galaxies found by deep spectroscopic
surveys in redshifts up to z∼1.5. These calibrations, when applied to recent deep redshift surveys confirm the drop of the
SFR density of the Universe since z∼1 previously infered in the UV. However, the fundamental parameter that determines galactic
evolution is mass, not luminosity. The mass function for local star-forming galaxies is critical for any future comparison
with other galaxy populations of different evolutionary status. Hα velocity-widths for UCM galaxies indicate that besides
a small fraction of 1010-1011 M⊙ starburst nuclei spirals, the majority have dynamical masses in the ∼109 M⊙ range. A comparison with published data for faint blue galaxies suggests that star-forming galaxies at z∼1 would have SFR
per unit mass and burst strengths similar to those at z=0, but being intrinsically more massive.
This revised version was published online in July 2006 with corrections to the Cover Date. 相似文献
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We have studied the velocity field of the Blue Compact Dwarf galaxy Mrk86 using an Hα Fabry-Perot image and 14 long-slit optical
spectra. From the ionized gas velocities measured we have found that Mrk86 follows a solid-body rotation law with a central
angular velocity of 34 ± 5 km s-1 kpc-1. The comparison of the modeled rotation curve with our velocity data indicates a clear dominance of the stellar mass component
over the dark matter. Related with the galaxy most intense star forming knot, a very strong gradient steeping is observed.
Finally, we give kinematic evidence for the Mrk86-C expanding bubble.
This revised version was published online in July 2006 with corrections to the Cover Date. 相似文献
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