Estudios sobre la transmisión por "moscas blancas" (homoptera: aleyrodidae) de virus asociados con el "cuero de sapo" en yuca (manihot esculenta crantz)

Estudios realizados en la zona endémica al "cuero de sapo" (Quilcacé, Cauca), encaminados a determinar la presencia de vectores de la enfermedad mostraron la existencia de dos virus asociados con "moscas blancas". El primero denominado "agente mosaico" fue transmitido por Bemisia tuberculata, el segundo asintomático, por Aleurotrachelus socialis. El 3.3% de la población de B. tuberculata utilizada transmitió el "agente mosaico" al clón M Col 2063 (Secundina) y no a M Col 113: el 2.4 % de A. socialis transmitió el asintomático al clón Secundina y el 4.7% a M Col 113. El "agente mosaico", no fue identificado, pero si se demostró que el asintomático presente era CsXV; este sería el primer registro de un potexvirus transmitido por "moscas blancas". El papel de los dos virus en la etiología del “cuero de sapo” continúa en estudio.Whiteflies collected from a frogskin infested field in Quilcacé (Cauca) were caged individually on M Col 2063 (Secundina) and M Col 113 plants. It was possible to identify the species (Aleurotrachelus socialis, Trialeurodes variabilis and Bemisia tuberculata) from pupae present on over 50% of the plants. A. socialis was found most f frequently and B. tuberculata the least com mom of the species. A. socialis was associated with the transmission of both CsXV and a serologically related strain, identified on the basis of symptoms produced on Nicotiana bentamiana, B. tuberculata was associated with the transmission of a mosaic agent to Secundina. The identify of the mosaic agent is unknown

An Economic Assessment of Smokefree Restaurant Establishments in Tennessee: Implications for Other Smoking Establishments

In 2007 Tennessee enacted and implemented the Nonsmoker Protection Act (NSPA) to protect nonsmokers by creating 100% smoke-free restaurants. Several venues were exempted, including age-restricted ones such as bars, and tobacco regulation was preempted. Thus, the NSPA is not equitable smoke free policy (SFP) because it has left vast segments of nonsmokers such as employees and patrons of bars unprotected from second-hand smoke (SHS) exposure and thwarted any local initiative to pursue 100% comprehensive SFPs. While this predisposes these nonsmokers to the health dangers of SHS exposure, it makes the NSPA incompatible with the objectives of the Healthy People 2020 and 2030 as well as goals of the state health plan. In 2021, the American Lung Association graded the NSPA “C,” and the United Health Foundation ranked it 42nd out of 50 states. This project assessed the effects of smoke-free venues across different economic domains through quantitative and qualitative data review to determine the implications for venues exempted by NSPA. By delineating any economic effects of SFP across several economic domains, the quantitative data gleaned from NAICS, Census Bureau, and Tennessee Dept. of Revenue were supplemented with interviews of establishments in Tennessee that voluntarily transitioned to smoke-free environment. A total of 7 such establishments with capacities ranging from 50 to over 69,000 people and number of employees ranging from 6 to over 1300 were interviewed. It was discovered that smoke-free environments have positive economic effects on restaurant establishments in Tennessee. By focusing on the SFP effect on restaurant establishments, the findings can be extrapolated to support the case for 100% smoke-free environments for other hospitality locations such as bars, music venues, and casinos. After analysis of trends for retail sales, number of establishments, employment, and payrolls by size of establishment and Metropolitan Statistical Area, a positive economic effect was identified for majority of these indicators between 2010 and 2019, a 10-year period following restaurants becoming smoke-free. Highlights include: Retail sales in Tennessee eating and drinking establishments increased by 62% The number of restaurant establishments increased by 16% Employment in the restaurant sector increased by 23% The qualitative data from the interviews reinforces these findings, with 100% of respondents supporting smoke-free age-restricted venues in their local communities. Thus, it can be inferred from these Tennessee-specific data with high degree of confidence that other hospitality venues will benefit economically in some way by becoming smoke-free with the following considerations: Provide protections from SHS exposure and health risks to nonsmokers; Do not adversely affect sales or employment in the hospitality, entertainment or sport industries, including bars, hotels and motels, and restaurants; Have strong public support and compliance

Strong absorption by interstellar hydrogen fluoride: Herschel/HIFI observations of the sight-line to G10.6-0.4 (W31C)

We report the detection of strong absorption by interstellar hydrogen fluoride along the sight-line to the submillimeter continuum source G10.6-0.4 (W31C). We have used Herschel's HIFI instrument, in dual beam switch mode, to observe the 1232.4763 GHz J=1-0 HF transition in the upper sideband of the Band 5a receiver. The resultant spectrum shows weak HF emission from G10.6-0.4 at LSR velocities in the range -10 to -3 km/s, accompanied by strong absorption by foreground material at LSR velocities in the range 15 to 50 km/s. The spectrum is similar to that of the 1113.3430 GHz 1(11)-0(00) transition of para-water, although at some frequencies the HF (hydrogen fluoride) optical depth clearly exceeds that of para-H2O. The optically-thick HF absorption that we have observed places a conservative lower limit of 1.6E+14 cm-2 on the HF column density along the sight-line to G10.6-0.4. Our lower limit on the HF abundance, 6E-9 relative to hydrogen nuclei, implies that hydrogen fluoride accounts for between ~ 30 and 100% of the fluorine nuclei in the gas phase along this sight-line. This observation corroborates theoretical predictions that - because the unique thermochemistry of fluorine permits the exothermic reaction of F atoms with molecular hydrogen - HF will be the dominant reservoir of interstellar fluorine under a wide range of conditions.Comment: Accepted for publication in Astronomy and Astrophysics (Herschel special issue). This revised version corrects a typographic error in the HTML abstract, in which the lower limit on the HF abundance (should be 6E-9) was previously misstated. The abstract in the PDF version is correct and the latter has not been modifie

Detection of hydrogen fluoride absorption in diffuse molecular clouds with Herschel/HIFI: a ubiquitous tracer of molecular gas

We discuss the detection of absorption by interstellar hydrogen fluoride (HF) along the sight line to the submillimeter continuum sources W49N and W51. We have used Herschel's HIFI instrument in dual beam switch mode to observe the 1232.4762 GHz J = 1 - 0 HF transition in the upper sideband of the band 5a receiver. We detected foreground absorption by HF toward both sources over a wide range of velocities. Optically thin absorption components were detected on both sight lines, allowing us to measure - as opposed to obtain a lower limit on - the column density of HF for the first time. As in previous observations of HF toward the source G10.6-0.4, the derived HF column density is typically comparable to that of water vapor, even though the elemental abundance of oxygen is greater than that of fluorine by four orders of magnitude. We used the rather uncertain N(CH)-N(H2) relationship derived previously toward diffuse molecular clouds to infer the molecular hydrogen column density in the clouds exhibiting HF absorption. Within the uncertainties, we find that the abundance of HF with respect to H2 is consistent with the theoretical prediction that HF is the main reservoir of gas-phase fluorine for these clouds. Thus, hydrogen fluoride has the potential to become an excellent tracer of molecular hydrogen, and provides a sensitive probe of clouds of small H2 column density. Indeed, the observations of hydrogen fluoride reported here reveal the presence of a low column density diffuse molecular cloud along the W51 sight line, at an LSR velocity of ~ 24kms-1, that had not been identified in molecular absorption line studies prior to the launch of Herschel.Comment: 4 pages, 3 figures, A&A Letter special issue, accepted on 07/13/201

Herschel observations of extra-ordinary sources: Detection of Hydrogen Fluoride in absorption towards Orion~KL

We report a detection of the fundamental rotational transition of hydrogen fluoride in absorption towards Orion KL using Herschel/HIFI. After the removal of contaminating features associated with common molecules ("weeds"), the HF spectrum shows a P-Cygni profile, with weak redshifted emission and strong blue-shifted absorption, associated with the low-velocity molecular outflow. We derive an estimate of 2.9 x 10^13 cm^-2 for the HF column density responsible for the broad absorption component. Using our best estimate of the H2 column density within the low-velocity molecular outflow, we obtain a lower limit of ~1.6 x 10^-10 for the HF abundance relative to hydrogen nuclei, corresponding to 0.6% of the solar abundance of fluorine. This value is close to that inferred from previous ISO observations of HF J=2--1 absorption towards Sgr B2, but is in sharp contrast to the lower limit of 6 x 10^-9 derived by Neufeld et al. (2010) for cold, foreground clouds on the line of sight towards G10.6-0.4.Comment: 5 pages, 3 figures, paper to be published in the Herschel special issue of A&A letter

Adaptive Filtering Enhances Information Transmission in Visual Cortex

Sensory neuroscience seeks to understand how the brain encodes natural environments. However, neural coding has largely been studied using simplified stimuli. In order to assess whether the brain's coding strategy depend on the stimulus ensemble, we apply a new information-theoretic method that allows unbiased calculation of neural filters (receptive fields) from responses to natural scenes or other complex signals with strong multipoint correlations. In the cat primary visual cortex we compare responses to natural inputs with those to noise inputs matched for luminance and contrast. We find that neural filters adaptively change with the input ensemble so as to increase the information carried by the neural response about the filtered stimulus. Adaptation affects the spatial frequency composition of the filter, enhancing sensitivity to under-represented frequencies in agreement with optimal encoding arguments. Adaptation occurs over 40 s to many minutes, longer than most previously reported forms of adaptation.Comment: 20 pages, 11 figures, includes supplementary informatio

Toxic equivalency factors (TEFs) for PCBs, PCDDs, PCDFs for humans and wildlife.

An expert meeting was organized by the World Health Organization (WHO) and held in Stockholm on 15-18 June 1997. The objective of this meeting was to derive consensus toxic equivalency factors (TEFs) for polychlorinated dibenzo-p-dioxins (PCDDs) and dibenzofurans (PCDFs) and dioxinlike polychlorinated biphenyls (PCBs) for both human, fish, and wildlife risk assessment. Based on existing literature data, TEFs were (re)evaluated and either revised (mammals) or established (fish and birds). A few mammalian WHO-TEFs were revised, including 1,2,3,7,8-pentachlorinated DD, octachlorinated DD, octachlorinated DF, and PCB 77. These mammalian TEFs are also considered applicable for humans and wild mammalian species. Furthermore, it was concluded that there was insufficient in vivo evidence to continue the use of TEFs for some di-ortho PCBs, as suggested earlier by Ahlborg et al. [Chemosphere 28:1049-1067 (1994)]. In addition, TEFs for fish and birds were determined. The WHO working group attempted to harmonize TEFs across different taxa to the extent possible. However, total synchronization of TEFs was not feasible, as there were orders of a magnitude difference in TEFs between taxa for some compounds. In this respect, the absent or very low response of fish to mono-ortho PCBs is most noticeable compared to mammals and birds. Uncertainties that could compromise the TEF concept were also reviewed, including nonadditive interactions, differences in shape of the dose-response curve, and species responsiveness. In spite of these uncertainties, it was concluded that the TEF concept is still the most plausible and feasible approach for risk assessment of halogenated aromatic hydrocarbons with dioxinlike properties

The polarization effects of radiation from magnetized envelopes and extended accretion structures

The results of numerical calculations of linear polarization from magnetized spherical optically thick and optically thin envelopes are presented. We give the methods how to distinguish magnetized optically thin envelopes from optically thick ones using observed spectral distributions of the polarization degree and the positional angle. The results of numerical calculations are used for analysis of polarimetric observations of OB and WR stars, X-ray binaries with black hole candidates (Cyg X-1, SS 433) and supernovae. The developed method allows to estimate magnetic field strength for the objects mentioned above.Comment: 18 pages, 6 figure