Water vapor line parameters in the 13 000-9250 cm-1 region.

info:eu-repo/semantics/published

A pll based frequency synthesizer in 0.13 um sige bicmos for mb-ofdm uwb systems

With the growing demand for high-speed and high-quality short-range communication, multi-band orthogonal frequency division multiplexing ultra-wide band (MB-OFDM UWB) systems have recently garnered considerable interest in industry and in academia. To achieve a low-cost solution, highly integrated transceivers with small die area and minimum power consumption are required. The key building block of the transceiver is the frequency synthesizer. A frequency synthesizer comprised of two PLLs and one multiplexer is presented in this thesis. Ring oscillators are adopted for PLL implementation in order to drastically reduce the die area of the frequency synthesizer. The poor spectral purity appearing in the frequency synthesizers involving mixers is greatly improved in this design. Based on the specifications derived from application standards, a design methodology is presented to obtain the parameters of building blocks. As well, the simulation results are provided to verify the performance of proposed design.

Indication of electron neutrino appearance from an accelerator-produced off-axis muon neutrino beam.

The T2K experiment observes indications of ν(μ) → ν(e) appearance in data accumulated with 1.43×10(20) protons on target. Six events pass all selection criteria at the far detector. In a three-flavor neutrino oscillation scenario with |Δm(23)(2)| = 2.4×10(-3)  eV(2), sin(2)2θ(23) = 1 and sin(2)2θ(13) = 0, the expected number of such events is 1.5±0.3(syst). Under this hypothesis, the probability to observe six or more candidate events is 7×10(-3), equivalent to 2.5σ significance. At 90% C.L., the data are consistent with 0.03(0.04) < sin(2)2θ(13) < 0.28(0.34) for δ(CP) = 0 and a normal (inverted) hierarchy.

On-board Robotic Multi-pinhole SPECT System for Region-of-interest (ROI) Imaging

On-board image guidance, such as cone-beam CT (CBCT) and kV/MV 2D imaging, is essential in many radiation therapy procedures, such as intensity modulated radiotherapy (IMRT) and stereotactic body radiation therapy (SBRT). These imaging techniques provide predominantly anatomical information for treatment planning and target localization. Recently, studies have shown that treatment planning based on functional and molecular information about the tumor and surrounding tissue could potentially improve the effectiveness of radiation therapy. However, current on-board imaging systems are limited in their functional and molecular imaging capability. Single Photon Emission Computed Tomography (SPECT) is a candidate to achieve on-board functional and molecular imaging. Traditional SPECT systems typically take 20 minutes or more for a scan, which is too long for on-board imaging. A robotic multi-pinhole SPECT system was proposed in this dissertation to provide shorter imaging time by using a robotic arm to maneuver the multi-pinhole SPECT system around the patient in position for radiation therapy.

A 49-pinhole collimated SPECT detector and its shielding were designed and simulated in this work using the computer-aided design (CAD) software. The trajectories of robotic arm about the patient, treatment table and gantry in the radiation therapy room and several detector assemblies such as parallel holes, single pinhole and 49 pinholes collimated detector were investigated. The rail mounted system was designed to enable a full range of detector positions and orientations to various crucial treatment sites including head and torso, while avoiding collision with linear accelerator (LINAC), patient table and patient.

An alignment method was developed in this work to calibrate the on-board robotic SPECT to the LINAC coordinate frame and to the coordinate frames of other on-board imaging systems such as CBCT. This alignment method utilizes line sources and one pinhole projection of these line sources. The model consists of multiple alignment parameters which maps line sources in 3-dimensional (3D) space to their 2-dimensional (2D) projections on the SPECT detector. Computer-simulation studies and experimental evaluations were performed as a function of number of line sources, Radon transform accuracy, finite line-source width, intrinsic camera resolution, Poisson noise and acquisition geometry. In computer-simulation studies, when there was no error in determining angles (α) and offsets (ρ) of the measured projections, the six alignment parameters (3 translational and 3 rotational) were estimated perfectly using three line sources. When angles (α) and offsets (ρ) were provided by Radon transform, the estimation accuracy was reduced. The estimation error was associated with rounding errors of Radon transform, finite line-source width, Poisson noise, number of line sources, intrinsic camera resolution and detector acquisition geometry. The estimation accuracy was significantly improved by using 4 line sources rather than 3 and also by using thinner line-source projections (obtained by better intrinsic detector resolution). With 5 line sources, median errors were 0.2 mm for the detector translations, 0.7 mm for the detector radius of rotation, and less than 0.5° for detector rotation, tilt and twist. In experimental evaluations, average errors relative to a different, independent registration technique were about 1.8 mm for detector translations, 1.1 mm for the detector radius of rotation (ROR), 0.5° and 0.4° for detector rotation and tilt, respectively, and 1.2° for detector twist.

Simulation studies were performed to investigate the improvement of imaging sensitivity and accuracy of hot sphere localization for breast imaging of patients in prone position. A 3D XCAT phantom was simulated in the prone position with nine hot spheres of 10 mm diameter added in the left breast. A no-treatment-table case and two commercial prone breast boards, 7 and 24 cm thick, were simulated. Different pinhole focal lengths were assessed for root-mean-square-error (RMSE). The pinhole focal lengths resulting in the lowest RMSE values were 12 cm, 18 cm and 21 cm for no table, thin board, and thick board, respectively. In both no table and thin board cases, all 9 hot spheres were easily visualized above background with 4-minute scans utilizing the 49-pinhole SPECT system while seven of nine hot spheres were visible with the thick board. In comparison with parallel-hole system, our 49-pinhole system shows reduction in noise and bias under these simulation cases. These results correspond to smaller radii of rotation for no-table case and thinner prone board. Similarly, localization accuracy with the 49-pinhole system was significantly better than with the parallel-hole system for both the thin and thick prone boards. Median localization errors for the 49-pinhole system with the thin board were less than 3 mm for 5 of 9 hot spheres, and less than 6 mm for the other 4 hot spheres. Median localization errors of 49-pinhole system with the thick board were less than 4 mm for 5 of 9 hot spheres, and less than 8 mm for the other 4 hot spheres.

Besides prone breast imaging, respiratory-gated region-of-interest (ROI) imaging of lung tumor was also investigated. A simulation study was conducted on the potential of multi-pinhole, region-of-interest (ROI) SPECT to alleviate noise effects associated with respiratory-gated SPECT imaging of the thorax. Two 4D XCAT digital phantoms were constructed, with either a 10 mm or 20 mm diameter tumor added in the right lung. The maximum diaphragm motion was 2 cm (for 10 mm tumor) or 4 cm (for 20 mm tumor) in superior-inferior direction and 1.2 cm in anterior-posterior direction. Projections were simulated with a 4-minute acquisition time (40 seconds per each of 6 gates) using either the ROI SPECT system (49-pinhole) or reference single and dual conventional broad cross-section, parallel-hole collimated SPECT. The SPECT images were reconstructed using OSEM with up to 6 iterations. Images were evaluated as a function of gate by profiles, noise versus bias curves, and a numerical observer performing a forced-choice localization task. Even for the 20 mm tumor, the 49-pinhole imaging ROI was found sufficient to encompass fully usual clinical ranges of diaphragm motion. Averaged over the 6 gates, noise at iteration 6 of 49-pinhole ROI imaging (10.9 µCi/ml) was approximately comparable to noise at iteration 2 of the two dual and single parallel-hole, broad cross-section systems (12.4 µCi/ml and 13.8 µCi/ml, respectively). Corresponding biases were much lower for the 49-pinhole ROI system (3.8 µCi/ml), versus 6.2 µCi/ml and 6.5 µCi/ml for the dual and single parallel-hole systems, respectively. Median localization errors averaged over 6 gates, for the 10 mm and 20 mm tumors respectively, were 1.6 mm and 0.5 mm using the ROI imaging system and 6.6 mm and 2.3 mm using the dual parallel-hole, broad cross-section system. The results demonstrate substantially improved imaging via ROI methods. One important application may be gated imaging of patients in position for radiation therapy.

A robotic SPECT imaging system was constructed utilizing a gamma camera detector (Digirad 2020tc) and a robot (KUKA KR150-L110 robot). An imaging study was performed with a phantom (PET CT PhantomTM), which includes 5 spheres of 10, 13, 17, 22 and 28 mm in diameter. The phantom was placed on a flat-top couch. SPECT projections were acquired with a parallel-hole collimator and a single-pinhole collimator both without background in the phantom, and with background at 1/10th the sphere activity concentration. The imaging trajectories of parallel-hole and pinhole collimated detectors spanned 180 degrees and 228 degrees respectively. The pinhole detector viewed a 14.7 cm-diameter common volume which encompassed the 28 mm and 22 mm spheres. The common volume for parallel-hole was a 20.8-cm-diameter cylinder which encompassed all five spheres in the phantom. The maneuverability of the robotic system was tested by navigating the detector to trace the flat-top table while avoiding collision with the table and maintaining the closest possible proximity to the common volume. For image reconstruction, detector trajectories were described by radius-of-rotation and detector rotation angle θ. These reconstruction parameters were obtained from the robot base and tool coordinates. The robotic SPECT system was able to maneuver the parallel-hole and pinhole collimated SPECT detectors in close proximity to the phantom, minimizing impact of the flat-top couch on detector to center-of-rotation (COR) distance. In no background case, all five spheres were visible in the reconstructed parallel-hole and pinhole images. In with background case, three spheres of 17, 22 and 28 mm diameter were readily observed with the parallel-hole imaging, and the targeted spheres (22 and 28 mm diameter) were readily observed in the pinhole ROI imaging.

In conclusion, the proposed on-board robotic SPECT can be aligned to LINAC/CBCT with a single pinhole projection of the line-source phantom. Alignment parameters can be estimated using one pinhole projection of line sources. This alignment method may be important for multi-pinhole SPECT, where relative pinhole alignment may vary during rotation. For single pinhole and multi-pinhole SPECT imaging onboard radiation therapy machines, the method could provide alignment of SPECT coordinates with those of CBCT and the LINAC. In simulation studies of prone breast imaging and respiratory-gated lung imaging, the 49-pinhole detector showed better tumor contrast recovery and localization in a 4-minute scan compared to parallel-hole detector. On-board SPECT could be achieved by a robot maneuvering a SPECT detector about patients in position for radiation therapy on a flat-top couch. The robot inherent coordinate frames could be an effective means to estimate detector pose for use in SPECT image reconstruction.

Dinámica del carbono en sistemas agrícolas bajo siembra directa : nuevas evidencias obtenidas mediante el uso de 13 C sobre la importancia de las raíces, la calidad de los residuos y el laboreo

El carbono orgánico del suelo (COS) es uno de los principales determinantes de la productividad de los ecosistemas, afectando la fertilidad del suelo y su capacidad de secuestrar CO2. La agricultura es uno de los principales cambios de uso del suelo que afecta significativamente el COS. En esta tesis se examinan, mediante experimentos de campo y usando al 13C como trazador isotópico, tres aspectos de la dinámica de C en sistemas agrícolas: 1) la importancia de las raíces en la formación de COS, 2) los efectos de la cantidad y calidad de los residuos sobre la tasa de descomposición y humificación del COS y 3) la dinámica del COS en sistemas de agricultura continua iniciados sobre pastizales naturales nunca laboreados. Los resultados obtenidos muestran que 1) en cultivos de soja y maíz, la formación de COS se deriva principalmente de la biomasa subterránea y en menor medida de los residuos aéreos, al menos en la fracción de la materia orgánica particulada (MOP). También, se observó 2) que el agregado de residuos de maíz con alta relación C:N aumentó la tasa de descomposición de la MOAM (materia orgánica asociada a los minerales) cuando se la compara con el agregado de residuos de soja (baja relación C:N), efecto conocido como priming. Sin embargo, también existió una mayor formación de materia orgánica bajo cultivos de maíz, y por ende se conservaron las reservas de COS, pero su ciclado fue más rápido. Finalmente, 3) los cultivos en sistemas de siembra directa establecidos sobre suelos nunca laboreados presentaron niveles de COS similares a los de los pastizales naturales remplazados. Estos resultados cuestionan parte de nuestro conocimiento sobre los sistemas agrícolas bajo siembra directa, aportando nuevas evidencias experimentales y destacando el uso de marcadores isotópicos de 13C para comprender el flujo de C en los agroecosistemas.

Dinámica del carbono en sistemas agrícolas bajo siembra directa : nuevas evidencias obtenidas mediante el uso de 13 C sobre la importancia de las raíces, la calidad de los residuos y el laboreo

El carbono orgánico del suelo (COS) es uno de los principales determinantes de la productividad de los ecosistemas, afectando la fertilidad del suelo y su capacidad de secuestrar CO2. La agricultura es uno de los principales cambios de uso del suelo que afecta significativamente el COS. En esta tesis se examinan, mediante experimentos de campo y usando al 13C como trazador isotópico, tres aspectos de la dinámica de C en sistemas agrícolas: 1) la importancia de las raíces en la formación de COS, 2) los efectos de la cantidad y calidad de los residuos sobre la tasa de descomposición y humificación del COS y 3) la dinámica del COS en sistemas de agricultura continua iniciados sobre pastizales naturales nunca laboreados. Los resultados obtenidos muestran que 1) en cultivos de soja y maíz, la formación de COS se deriva principalmente de la biomasa subterránea y en menor medida de los residuos aéreos, al menos en la fracción de la materia orgánica particulada (MOP). También, se observó 2) que el agregado de residuos de maíz con alta relación C:N aumentó la tasa de descomposición de la MOAM (materia orgánica asociada a los minerales) cuando se la compara con el agregado de residuos de soja (baja relación C:N), efecto conocido como priming. Sin embargo, también existió una mayor formación de materia orgánica bajo cultivos de maíz, y por ende se conservaron las reservas de COS, pero su ciclado fue más rápido. Finalmente, 3) los cultivos en sistemas de siembra directa establecidos sobre suelos nunca laboreados presentaron niveles de COS similares a los de los pastizales naturales remplazados. Estos resultados cuestionan parte de nuestro conocimiento sobre los sistemas agrícolas bajo siembra directa, aportando nuevas evidencias experimentales y destacando el uso de marcadores isotópicos de 13C para comprender el flujo de C en los agroecosistemas.

Utilización de la historia de las matemáticas en clase con alumnos de 6 a 13 años

En mi conferencia consideraré varias maneras de utilizar la historia de las matemáticas en la didáctica de las matemáticas para la escuela obligatoria; se trata de experiencias y reflexiones relacionadas con la elaboración y la experimentación de currículos para la enseñanza de las matemáticas en las edades comprendidas entre los 6 y los 13 años, desarrollados a partir de 1975 en el grupo de universitarios y enseñantes que coordina personalmente en Génova. El trabajo se ha efectuado en colaboración con Elda Guala; algunos artículos relacionados con estas cuestiones ya han sido publicados o están en curso de publicación.

Utilización de la Historia de las Matemáticas en clase con alumnos de 6 a 13 años

En mi conferencia consideraré varias maneras de utilizar la historia de las matemáticas en la didáctica de las matemáticas para la escuela obligatoria; se trata de experiencias y reflexiones relacionadas con la elaboración y la experimentación de currículos para la enseñanza de las Matemáticas en las edades comprendidas entre los 6 y los 13 años, desarrollados a partir de 1975 en el grupo de universitarios y enseñantes que coordino personalmente en Génova. El trabajo se ha efectuado en colaboración con Elda Guala; algunos artículos relacionados con estas cuestiones ya han sido publicados o están en curso de publicación.

[Conference report] Magic and mathematics: The life and work of John Dee. National Maritime Museum, Greenwich, 13-14 June 2003

Tony Mann provides a report of a two-day meeting "Magic and mathematics: The life and work of John Dee" held from 13-14 June 2003 at the National Maritime Museum, Greenwich.

[Recording review] William Herschel, Symphonies Nos. 2, 8, 12, 13, 14, 17

Tony Mann provides a review of the recording: William Herschel, Symphonies Nos. 2, 8, 12, 13, 14, 17, soloists, London Mozart Players / Matthias Bamert, Chandos 10048, 2003, (68 mins). [CD]

‘The trouble with Year 10’: 13 – 16 year old school students’ attitudes to higher education

This study looked at the impact of Widening Participation interventions on the attitudes of young people towards higher education. A total of 2731 adolescents aged 13–16 years completed a self-report measure of their attitudes to higher education, general and academic self concept and identification with school, family and peers. This was matched with data on the students’ academic attainment and social backgrounds. As expected, attainment scores were significantly positively correlated with take up of Widening Participation activities aimed at increasing participation in higher education, attitudes towards going to university and academic motivation. However, attainment was negatively correlated with perceptions of family attending university and identification with family. Regression analyses found that perceptions of family views about attending university were not a predictor of taking part in Widening Participation activities but were a predictor of attitudes towards higher education. Students in Year 10 aged 14–15 were significantly more negative on most factors than either older or younger students.