Evaluation of the behavior of common bean cultivars and promising lines under natural virus infection = Evaluación del comportamiento de cultivares y líneas experimentales de poroto común frente a infecciones naturales de virus

Las enfermedades virales pueden afectar la estabilidad de la producción de poroto común (Phaseolus vulgaris L.), por lo que es de interés evaluar el comportamiento de diferentes cultivares y líneas avanzadas del programa de mejoramiento de IIACS INTA, frente a infecciones naturales. Se trabajó, durante tres campañas agrícolas con 14 cultivares, evaluándose severidad de síntomas, incidencia y concentración relativa de los virus Cucumber mosaic virus (CMV), Cowpea mild mottle virus (CpMMV), Alfalfa mosaic virus (AMV), Soybean mosaic virus (SMV) y geminivirus. Se encontró muy baja incidencia de SMV y AMV en las tres campañas. Se hallaron diferencias en comportamiento entre los cultivares evaluados: L24 y L15 fueron tolerantes a begomovirus, mientras que CR8, CR5 y L22 (poroto tipo cranberry y blancos) exhibieron susceptibilidad. Los síntomas más severos se observaron en el 2013, cuando hubo una alta incidencia de begomovirus y CpMMV. No existieron diferencias entre cultivares para incidencia de CpMMV, pero se encontró una mayor concentración relativa de virus para CR5, CR8 y L17. L15, aunque tolerante a geminivirus, fue el más susceptible a CMV, hecho a tener en cuenta porque esta virosis se transmite por semilla y puede llegar a afectar significativamente la producción de poroto.Viral diseases can affect the stability of common bean (Phaseolus vulgaris L.) production, therefore it was considered of interest to evaluate the behavior of different cultivars and promising lines obtained by the INTA breeding program against natural virus infection. Symptoms severity, incidence and relative concentration of Cucumber mosaic virus (CMV), Cowpea mild mottle virus (CpMMV), Alfalfa mosaic virus (AMV), Soybean mosaic virus (SMV) and geminiviruses were evaluated for 14 bean cultivars during three growing seasons. SMV and AMV were found in very low incidence during the three years. Differences in cultivar response were observed: L24 and L15 were tolerant to begomoviruses, while CR8, CR5, L22 (cranberry and white bean types) were susceptible. The most severe symptoms were found during the 2013 growing season, when a high incidence of begomovirus and CpMMV were observed. No differences between cultivars were found for CpMMV incidence, but a higher relative concentration of virus was detected in CR5, CR8 and L17. Although L15 was tolerant to geminiviruses, it was the most susceptible to CMV, a fact that must be taken into account because this virus is transmitted by seeds and might become a serious problem in bean production.Instituto de Patología VegetalFil: Rodriguez Pardina, Patricia. Instituto Nacional de Tecnología Agropecuaria (INTA). Instituto de Patología Vegetal; ArgentinaFil: Reyna, Pablo Gastón. Instituto Nacional de Tecnología Agropecuaria (INTA). Instituto de Patología Vegetal; Argentina. Concejo Nacional de Investigaciones Científicas y Técnicas; ArgentinaFil: Campos, Ramon Eduardo. Instituto Nacional de Tecnología Agropecuaria (INTA). Instituto de Patología Vegetal; ArgentinaFil: Varela, Gonzalo Matías. Universidad Nacional de Córdoba. Facultad de Ciencias Médicas. Cátedra de Bioquímica y Biología Molecular; ArgentinaFil: Peña Malavera, Andrea Natalia. Universidad Nacional de Córdoba. Facultad de Ciencias Agropecuarias; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; ArgentinaFil: Geronimo, Luis Marcelo. Instituto Nacional de Tecnología Agropecuaria (INTA). Instituuto de Investigación Animal del Chaco Semiárido; Argentin

Measurement of the cosmic ray spectrum above 4×10184{\times}10^{18} eV using inclined events detected with the Pierre Auger Observatory

A measurement of the cosmic-ray spectrum for energies exceeding $4{\times}10^{18}$ eV is presented, which is based on the analysis of showers with zenith angles greater than $60^{\circ}$ 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 $5.3{\times}10^{18}$ eV, the "ankle", the flux can be described by a power law $E^{-\gamma}$ with index $\gamma=2.70 \pm 0.02 \,\text{(stat)} \pm 0.1\,\text{(sys)}$ followed by a smooth suppression region. For the energy ($E_\text{s}$) at which the spectral flux has fallen to one-half of its extrapolated value in the absence of suppression, we find $E_\text{s}=(5.12\pm0.25\,\text{(stat)}^{+1.0}_{-1.2}\,\text{(sys)}){\times}10^{19}$ 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

A search for ultra-high-energy photons at the Pierre Auger Observatory exploiting air-shower universality

The Pierre Auger Observatory is the most sensitive detector to primary photons with energies above ∼0.2 EeV. It measures extensive air showers using a hybrid technique that combines a fluorescence detector (FD) with a ground array of particle detectors (SD). The signatures of a photon-induced air shower are a larger atmospheric depth at the shower maximum (X$_{max}$) and a steeper lateral distribution function, along with a lower number of muons with respect to the bulk of hadron-induced background. Using observables measured by the FD and SD, three photon searches in different energy bands are performed. In particular, between threshold energies of 1-10 EeV, a new analysis technique has been developed by combining the FD-based measurement of X$_{max}$ with the SD signal through a parameter related to its muon content, derived from the universality of the air showers. This technique has led to a better photon/hadron separation and, consequently, to a higher search sensitivity, resulting in a tighter upper limit than before. The outcome of this new analysis is presented here, along with previous results in the energy ranges below 1 EeV and above 10 EeV. From the data collected by the Pierre Auger Observatory in about 15 years of operation, the most stringent constraints on the fraction of photons in the cosmic flux are set over almost three decades in energy

Study on multi-ELVES in the Pierre Auger Observatory

Since 2013, the four sites of the Fluorescence Detector (FD) of the Pierre Auger Observatory record ELVES with a dedicated trigger. These UV light emissions are correlated to distant lightning strikes. The length of recorded traces has been increased from 100 μs (2013), to 300 μs (2014-16), to 900 μs (2017-present), to progressively extend the observation of the light emission towards the vertical of the causative lightning and beyond. A large fraction of the observed events shows double ELVES within the time window, and, in some cases, even more complex structures are observed. The nature of the multi-ELVES is not completely understood but may be related to the different types of lightning in which they are originated. For example, it is known that Narrow Bipolar Events can produce double ELVES, and Energetic In-cloud Pulses, occurring between the main negative and upper positive charge layer of clouds, can induce double and even quadruple ELVES in the ionosphere. This report shows the seasonal and daily dependence of the time gap, amplitude ratio, and correlation between the pulse widths of the peaks in a sample of 1000+ multi-ELVES events recorded during the period 2014-20. The events have been compared with data from other satellite and ground-based sensing devices to study the correlation of their properties with lightning observables such as altitude and polarity