47 research outputs found
Mid-term evaluation of CATIE's program on ecologically-based participatory implementation of IPM and agroforestry in Nicaragua and Central America (CATI-MIP/AF) Phase III
CATIE-MIP/AF is a well-conceived and well-managed program that has capitalized on lessons learned in previous phases and from other programs. It developed in response to the weakening of the extension function within national agricultural systems in Central America and has contributed to the reorientation of the linear transfer-of-technology model prevailing in Nicaragua and other Central American Countries into a participatory extension approach that links farm families, extensionists, researchers and trainers, and decision-makers. The participatory methodologies developed by the program are a major strength in addressing challenges posed by modern-day complexity, uncertainty and dynamism in agriculture and natural resource management by farmers. The Program has catalyzed the establishment of a field-based multi-level, multi-institutional platform for participatory development and extension of technology for three important Central American farming systems, coffee, vegetables and basic grains (maize and beans), combining these with a broad array of ecological practices based on principles of agroforestry, integrated pest management, and natural resource conservation. The participatory capacity-building supported by the program develops powers of ecological reasoning, and incorporates a gender and family focus. The program has supported participatory training of 19,964 farmers, 861extensionists, 133 trainers (specialists) and has involved 380 decision-makers in joint planning and public monitoring of the process. Benefits to participating farmers of at least US$3.7 million have accrued during the first three years of the program. High priorities during the remaining two years of the program include Sustained effort in:
systematization of program experience,
promotion of institutional learning in CATIE about the MIP/AF experience;
capacity-building to develop ecological reasoning;
development of the regionalization process for scaling-out the work of the program to pilot areas in other Central Amercian countries
capacity-building work on basic grains,
The mission also recommends formulation of a plan to ensure devolution of the field based, multi-level, multi-institutional process in Nicaragua and elswhere when appropriate. This could occur by establishment of a process for promoting proposal development by counterparts, and by the program, that will ensure the future integrity of the multinstitutional platform and of the integrated MIP/AF focus. The review mission recommends further sustained funding counterpart organisations and to the program. The mission sees a need for developing empresarial reasoning as a complement to the current focus on ecological reasoning. Combining the two within a new cycle of funding involving both counterpart organisations and CATIE will increase the sustainability of achievements and the chances of significant impact on poverty alleviation in the future
Measurement of the cosmic ray spectrum above eV using inclined events detected with the Pierre Auger Observatory
A measurement of the cosmic-ray spectrum for energies exceeding
eV is presented, which is based on the analysis of showers
with zenith angles greater than detected with the Pierre Auger
Observatory between 1 January 2004 and 31 December 2013. The measured spectrum
confirms a flux suppression at the highest energies. Above
eV, the "ankle", the flux can be described by a power law with
index followed by
a smooth suppression region. For the energy () at which the
spectral flux has fallen to one-half of its extrapolated value in the absence
of suppression, we find
eV.Comment: Replaced with published version. Added journal reference and DO
Energy Estimation of Cosmic Rays with the Engineering Radio Array of the Pierre Auger Observatory
The Auger Engineering Radio Array (AERA) is part of the Pierre Auger
Observatory and is used to detect the radio emission of cosmic-ray air showers.
These observations are compared to the data of the surface detector stations of
the Observatory, which provide well-calibrated information on the cosmic-ray
energies and arrival directions. The response of the radio stations in the 30
to 80 MHz regime has been thoroughly calibrated to enable the reconstruction of
the incoming electric field. For the latter, the energy deposit per area is
determined from the radio pulses at each observer position and is interpolated
using a two-dimensional function that takes into account signal asymmetries due
to interference between the geomagnetic and charge-excess emission components.
The spatial integral over the signal distribution gives a direct measurement of
the energy transferred from the primary cosmic ray into radio emission in the
AERA frequency range. We measure 15.8 MeV of radiation energy for a 1 EeV air
shower arriving perpendicularly to the geomagnetic field. This radiation energy
-- corrected for geometrical effects -- is used as a cosmic-ray energy
estimator. Performing an absolute energy calibration against the
surface-detector information, we observe that this radio-energy estimator
scales quadratically with the cosmic-ray energy as expected for coherent
emission. We find an energy resolution of the radio reconstruction of 22% for
the data set and 17% for a high-quality subset containing only events with at
least five radio stations with signal.Comment: Replaced with published version. Added journal reference and DO
Measurement of the Radiation Energy in the Radio Signal of Extensive Air Showers as a Universal Estimator of Cosmic-Ray Energy
We measure the energy emitted by extensive air showers in the form of radio
emission in the frequency range from 30 to 80 MHz. Exploiting the accurate
energy scale of the Pierre Auger Observatory, we obtain a radiation energy of
15.8 \pm 0.7 (stat) \pm 6.7 (sys) MeV for cosmic rays with an energy of 1 EeV
arriving perpendicularly to a geomagnetic field of 0.24 G, scaling
quadratically with the cosmic-ray energy. A comparison with predictions from
state-of-the-art first-principle calculations shows agreement with our
measurement. The radiation energy provides direct access to the calorimetric
energy in the electromagnetic cascade of extensive air showers. Comparison with
our result thus allows the direct calibration of any cosmic-ray radio detector
against the well-established energy scale of the Pierre Auger Observatory.Comment: Replaced with published version. Added journal reference and DOI.
Supplemental material in the ancillary file
Käytännön kosteikkosuunnittelu
Maatalouden vesiensuojelua edistetään monin tavoin. Ravinteita ja eroosioainesta sisältäviä valumavesiä pyritään puhdistamaan erilaisissa kosteikoissa. Tämä opas on kirjoitettu avuksi pienimuotoisten kosteikkojen perustamiseen. Oppaassa esitetään käytännönläheisesti kosteikon toteuttamisen eri vaiheet paikan valinnasta suunnitteluun ja rakentamiseen. Vuonna 2010 julkaistun painoksen tiedot on saatettu ajantasalle.
Julkaisu on toteutettu osana Tehoa maatalouden vesiensuojeluun (TEHO) -hanketta ja päivitetty TEHO Plus -hankkeen toimesta. Oppaan toivotaan lisäävän kiinnostusta kosteikkojen suunnitteluun ja edelleen niiden rakentamiseen
Number of Hajj Pilgrims Departured(1) to the Holyland of Mecca by Province, 2012–2015
The azimuthal asymmetry in the risetime of signals in Auger surface detector stations is a source of information on shower development. The azimuthal asymmetry is due to a combination of the longitudinal evolution of the shower and geometrical effects related to the angles of incidence of the particles into the detectors. The magnitude of the effect depends upon the zenith angle and state of development of the shower and thus provides a novel observable, (secθ)max, sensitive to the mass composition of cosmic rays above 3×1018 eV. By comparing measurements with predictions from shower simulations, we find for both of our adopted models of hadronic physics (QGSJETII-04 and EPOS-LHC) an indication that the mean cosmic-ray mass increases slowly with energy, as has been inferred from other studies. However, the mass estimates are dependent on the shower model and on the range of distance from the shower core selected. Thus the method has uncovered further deficiencies in our understanding of shower modeling that must be resolved before the mass composition can be inferred from (secθ)max