Photograph - Julia Cleveland Woodruff, Side angle Pose

Black and white photograph, mounted on board, 7 cm x 4 cm, of Julia in a side angle face pose. This photo was taken by Fred Pfaff of Peach Street, Erie, Pennsylvania.

Photograph - Julia Cleveland Woodruff at Dr. Cleveland's Home

Black and white photograph, mounted on board, 18 cm x 12 cm, of Julia Cleveland wife of Hamilton K. Woodruff. She is posing with a setter and the Chihuahua at Dr. Cleveland’s house in Erie Pennsylvania. This photograph is mounted on a board. This was described by R. Band of Toronto on the back of the photo in 1975.

Marriage Certificate - Hamilton K. Woodruff and Julia C. Cleveland

The marriage certificate of Mr. Hamilton K. Woodruff of St. Catharines and Miss Julia C. Cleveland of Erie, Pennsylvania. This is certificate no. 5221 signed by James C. Wilson. This is accompanied by 2 envelopes; one envelope is from Henry L. Rea, clerk of courts, Erie Pennsylvania to Mr. H. K. Woodruff, the other envelope just says "marriage certificate Mrs. H. K. Woodruff", Nov. 21, 1894.

Ivory Victorian Day Planner

The planner has an ivory cover and 6 celluloid pages which fan out. The days of the week were stamped on each page, except Sunday. In this case, the days of the week are faded away and someone has rewritten them and included Sunday on the back cover. The front cover has a metal escutcheon engraved with the letter C and it closes with a metal latch. The front ivory cover is cracked down the middle and the front page is also cracked. R. Band has written on the “Monday” page that this belonged to Dr. Cleveland, this note is dated June 6, 2004. The “Tuesday” page has the title “Julia’s house” and gives the numbers of doors, lights, windows and water closets etc. within the house. On the back of the “Friday” page is the number 4784 and on the back of the Saturday page is the name and address of Dr. Mafarlan [?] of Pennsylvania.

Letter - D.K. Minor to S.D. Woodruff

Letter with the letterhead Franklin House, Chestnut Street, Philadelphia. The letter is addressed to S.D. Woodruff. The sender, D.K. Minor is sending nos. 25 and 37 of the volume for 184b of the R.R.J. [Railroad Journal]. He says that he is pleased to see that there is a prospect of an early movement in relation to the Great Western Railroad in Canada. [D. Kimball Minor was the founder of the American Railroad Journal], Jan. 18, 1847.

Letter - William Young to James Woodruff

Letter to James D. Woodruff at the Welland Canal, St. Catharines. The letter is postmarked Philadelphia [date illegible] and Queenston, Feb. 7, 1847. In this letter William Young of Philadelphia describes some of the prices and features of his wares including compasses and levels, Feb. 3, 1847.

The Physician’s Visiting List for 1869

The Physician’s Visiting List for 1869, Lindsay and Blakiston, Philadelphia, 1869. This is an almanac that contains handwritten recipes and household hints. Newspaper clippings of household hints are also glued into the back pages. The name Dr. W. K. Cleveland is embossed on the outer leather cover. The leather cover is quite deteriorated and the leather clasp is gone, 1869.

Letter with the letterhead “H.H. Warner and Co.” of Rochester, N.Y. from the H.H. Warner Co

Letter with the letterhead “H.H. Warner and Co.” of Rochester, N.Y. from the H.H. Warner Co. The writer asks why Mr. Woodruff did not stop there on his way home from Pennsylvania regarding his shooting share at Point Mouillee [a game area in Monroe County, Michigan]. This letter is accompanied by an envelope, May 19, 1886.

Letter to J.P. Bradley from his brother Dr. John Bradley

Letter to J.P. Bradley from his brother Dr. John Bradley regarding settling in Pottsville, Pennsylvania to serve the coal miners, Oct. 28 (3 pages, handwritten). This letter is torn and has a hole in it which affects text slightly, 1847.

Study on period search methods of variable stars: Application to ASAS and CRTS databases

Study on variable stars is an important topic of modern astrophysics. After the invention of powerful telescopes and high resolving powered CCD’s, the variable star data is accumulating in the order of peta-bytes. The huge amount of data need lot of automated methods as well as human experts. This thesis is devoted to the data analysis on variable star’s astronomical time series data and hence belong to the inter-disciplinary topic, Astrostatistics. For an observer on earth, stars that have a change in apparent brightness over time are called variable stars. The variation in brightness may be regular (periodic), quasi periodic (semi-periodic) or irregular manner (aperiodic) and are caused by various reasons. In some cases, the variation is due to some internal thermo-nuclear processes, which are generally known as intrinsic vari- ables and in some other cases, it is due to some external processes, like eclipse or rotation, which are known as extrinsic variables. Intrinsic variables can be further grouped into pulsating variables, eruptive variables and flare stars. Extrinsic variables are grouped into eclipsing binary stars and chromospheri- cal stars. Pulsating variables can again classified into Cepheid, RR Lyrae, RV Tauri, Delta Scuti, Mira etc. The eruptive or cataclysmic variables are novae, supernovae, etc., which rarely occurs and are not periodic phenomena. Most of the other variations are periodic in nature. Variable stars can be observed through many ways such as photometry, spectrophotometry and spectroscopy. The sequence of photometric observa- xiv tions on variable stars produces time series data, which contains time, magni- tude and error. The plot between variable star’s apparent magnitude and time are known as light curve. If the time series data is folded on a period, the plot between apparent magnitude and phase is known as phased light curve. The unique shape of phased light curve is a characteristic of each type of variable star. One way to identify the type of variable star and to classify them is by visually looking at the phased light curve by an expert. For last several years, automated algorithms are used to classify a group of variable stars, with the help of computers. Research on variable stars can be divided into different stages like observa- tion, data reduction, data analysis, modeling and classification. The modeling on variable stars helps to determine the short-term and long-term behaviour and to construct theoretical models (for eg:- Wilson-Devinney model for eclips- ing binaries) and to derive stellar properties like mass, radius, luminosity, tem- perature, internal and external structure, chemical composition and evolution. The classification requires the determination of the basic parameters like pe- riod, amplitude and phase and also some other derived parameters. Out of these, period is the most important parameter since the wrong periods can lead to sparse light curves and misleading information. Time series analysis is a method of applying mathematical and statistical tests to data, to quantify the variation, understand the nature of time-varying phenomena, to gain physical understanding of the system and to predict future behavior of the system. Astronomical time series usually suffer from unevenly spaced time instants, varying error conditions and possibility of big gaps. This is due to daily varying daylight and the weather conditions for ground based observations and observations from space may suffer from the impact of cosmic ray particles. Many large scale astronomical surveys such as MACHO, OGLE, EROS, xv ROTSE, PLANET, Hipparcos, MISAO, NSVS, ASAS, Pan-STARRS, Ke- pler,ESA, Gaia, LSST, CRTS provide variable star’s time series data, even though their primary intention is not variable star observation. Center for Astrostatistics, Pennsylvania State University is established to help the astro- nomical community with the aid of statistical tools for harvesting and analysing archival data. Most of these surveys releases the data to the public for further analysis. There exist many period search algorithms through astronomical time se- ries analysis, which can be classified into parametric (assume some underlying distribution for data) and non-parametric (do not assume any statistical model like Gaussian etc.,) methods. Many of the parametric methods are based on variations of discrete Fourier transforms like Generalised Lomb-Scargle peri- odogram (GLSP) by Zechmeister(2009), Significant Spectrum (SigSpec) by Reegen(2007) etc. Non-parametric methods include Phase Dispersion Minimi- sation (PDM) by Stellingwerf(1978) and Cubic spline method by Akerlof(1994) etc. Even though most of the methods can be brought under automation, any of the method stated above could not fully recover the true periods. The wrong detection of period can be due to several reasons such as power leakage to other frequencies which is due to finite total interval, finite sampling interval and finite amount of data. Another problem is aliasing, which is due to the influence of regular sampling. Also spurious periods appear due to long gaps and power flow to harmonic frequencies is an inherent problem of Fourier methods. Hence obtaining the exact period of variable star from it’s time series data is still a difficult problem, in case of huge databases, when subjected to automation. As Matthew Templeton, AAVSO, states “Variable star data analysis is not always straightforward; large-scale, automated analysis design is non-trivial”. Derekas et al. 2007, Deb et.al. 2010 states “The processing of xvi huge amount of data in these databases is quite challenging, even when looking at seemingly small issues such as period determination and classification”. It will be beneficial for the variable star astronomical community, if basic parameters, such as period, amplitude and phase are obtained more accurately, when huge time series databases are subjected to automation. In the present thesis work, the theories of four popular period search methods are studied, the strength and weakness of these methods are evaluated by applying it on two survey databases and finally a modified form of cubic spline method is intro- duced to confirm the exact period of variable star. For the classification of new variable stars discovered and entering them in the “General Catalogue of Vari- able Stars” or other databases like “Variable Star Index“, the characteristics of the variability has to be quantified in term of variable star parameters.

Piezoelectric Ultrasonic Micromotors

This report describes development of micro-fabricated piezoelectric ultrasonic motors and bulk-ceramic piezoelectric ultrasonic motors. Ultrasonic motors offer the advantage of low speed, high torque operation without the need for gears. They can be made compact and lightweight and provide a holding torque in the absence of applied power, due to the traveling wave frictional coupling mechanism between the rotor and the stator. This report covers modeling, simulation, fabrication and testing of ultrasonic motors. Design of experiments methods were also utilized to find optimal motor parameters. A suite of 8 mm diameter x 3 mm tall motors were machined for these studies and maximum stall torques as large as 10^(- 3) Nm, maximum no-load speeds of 1710 rpm and peak power outputs of 27 mW were realized. Aditionally, this report describes the implementation of a microfabricated ultrasonic motor using thin-film lead zirconate titanate. In a joint project with the Pennsylvania State University Materials Research Laboratory and MIT Lincoln Laboratory, 2 mm and 5 mm diameter stator structures were fabricated on 1 micron thick silicon nitride membranes. Small glass lenses placed down on top spun at 100-300 rpm with 4 V excitation at 90 kHz. The large power densities and stall torques of these piezoelectric ultrasonic motors offer tremendous promis for integrated machines: complete intelligent, electro-mechanical autonomous systems mass-produced in a single fabrication process.

How to improve the formal analytic reasoning and scientific motivation in the intellectual training of medical students

A review article of the The New England Journal of Medicine refers that almost a century ago, Abraham Flexner, a research scholar at the Carnegie Foundation for the Advancement of Teaching, undertook an assessment of medical education in 155 medical schools in operation in the United States and Canada. Flexner’s report emphasized the nonscientific approach of American medical schools to preparation for the profession, which contrasted with the university-based system of medical education in Germany. At the core of Flexner’s view was the notion that formal analytic reasoning, the kind of thinking integral to the natural sciences, should hold pride of place in the intellectual training of physicians. This idea was pioneered at Harvard University, the University of Michigan, and the University of Pennsylvania in the 1880s, but was most fully expressed in the educational program at Johns Hopkins University, which Flexner regarded as the ideal for medical education. (...)

Análisis del proceso que condujo a la construcción del concepto de explotación inserto en el Protocolo para prevenir, reprimir y sancionar la trata de personas, incorporado a la legislación colombiana a través de la Ley 800 de 2003

El objetivo de este trabajo de grado es describir una disputa política por el significado del concepto de explotación en el marco de la redacción del “Protocolo para prevenir, reprimir y sancionar la trata de personas, especialmente mujeres y niños”, en el cual se define aquello que se entiende por trata de personas. La construcción de este concepto excluye e invisibiliza otros tipos de explotación comunes en el sistema de producción capitalista contemporánea que pertenecen al universo de violencia objetiva sistémica a través del énfasis en la explotación sexual que hace parte de la violencia subjetiva.

Comparación: injerto libre o cierre primario más lente de contacto, en resección de tumores de conjuntiva limbar

INTRODUCCION: Existe controversia en cuanto a la técnica quirúrgica para el manejo de tumores del limbo conjuntival. El uso de cierre primario con uso de lente de contacto puede ofrecer una mejor cicatrización y tener ventajas adicionales sobre la técnica tradicional con el uso de plastia. OBJETIVOS: Comparar los resultados en cuanto a grado de dolor, picadas, prurito, porcentaje de epitelización y cicatrización, comodidad del paciente, grado de quemosis y tiempo de retorno a actividades diarias en ambas técnicas quirúrgicas. MATERIALES Y METODOS: Experimento clínico controlado aleatorizado en dos grupos: Al primer grupo se le realizó cirugía de resección de la lesión más plastia. Al segundo grupo se le practicó la resección de la lesión cierre primario y lente de contacto. El seguimiento se realizó al primer y cuarto día, y cada semana durante el primer mes de postoperatorio. Se utilizó el SPSS 20.0 ® para análisis estadístico de datos y se utilizó estadística no paramétrica. RESULTADOS: Se conto con 10 pacientes por grupo. El dolor y porcentaje de cicatrización al primer día postoperatorio fueron mayores en el grupo usando lente de contacto (p=0.048). Al cuarto día postquirúrgico se encontró un mayor porcentaje de cicatrización en el grupo usando lente de contacto. (p=0.075). CONCLUSIONES: El cierre por afrontamiento con uso de lente de contacto mostró dolor y picadas mayores al primer y cuarto día postoperatorio. Pero la epitelización y cicatrización fueron tempranas con un retorno corto a actividades cotidianas.

Transmisiones deportivas como género mediático y periodístico: Análisis pragmático de las transmisiones colombianas de la Copa Mundial – Sudáfrica 2010

En este trabajo académico se presentan los resultados de un estudio cualitativo-pragmático de una muestra de las transmisiones la Copa del Mundo de fútbol de 2010 realizadas por la televisión abierta colombiana. Se argumenta que las transmisiones deportivas (dentro de las cuales las transmisiones de fútbol son las más extendidas) deben ser entendidas como un género mediático y periodístico específico y, por tanto, deben ser analizadas desde criterios diferentes a otros productos tradicionales de la comunicación masiva.