Kolmiulotteinen visualisointi mikromaailman konenäköjärjestelmässä

Työssä oli tarkoituksena saada toteutettua kolmiulotteiseen visualisointiin soveltuva ohjelmisto mikrokokoluokkaa olevien kappaleiden konenäköjärjestelmään. Työssä jouduttiin myös jatkokehittämään menetelmää kolmiulotteisen kuvan hankkimiseksi yhdellä kameralla mikrokokoisesta kohteesta. Kohteen kolmiulotteisella kuvalla voitaisiin suorittaa automaattista järjestelmäohjausta. Työssä tutkittiin ja selvitettiin laitteistolla saavutettavia tarkkuuksia ja nopeuksia, sen soveltamiseksi esimerkiksi mikromanipulaattorin ohjaamiseen. Lisäksi tutkittiin erilaisia kohteita joissa voitaisiin hyödyntää kolmiulotteista visualisointia. Tällaisia kohteita on kappaleiden laadunvalvonnassa tai niiden tutkimisessa ja esittämisessä. Syvyystiedon keräävällä menetelmällä oli saavutettava riittävä nopeus, jotta sillä voitaisiin tarvittaessa ohjata reaaliaikaisesti toimilaitteita. Menetelmänä käytettiin "Depth from Focusing" -menetelmää, johon VTT:llä oli jo aiemmin kehitetty automaattinen fokusointiohjelmisto. Työn puitteissa suoritettiin laitteisto- ja menetelmäkehitystä järjestelmän nopeuttamiseksi. Visualisoinnin toteuttamisen eri mahdollisuuksia kartoitettiin ja sellainen toteutettiin rakennettuun konenäköjärjestelmään.

The 2010 May Flaring Episode of Cygnus X-3 in Radio, X-rays, and γ-rays

In 2009, Cygnus X-3 (Cyg X-3) became the first microquasar to be detected in the GeV γ-ray regime, via the satellites Fermi and AGILE. The addition of this new band to the observational toolbox holds promise for building a more detailed understanding of the relativistic jets of this and other systems. We present a rich data set of radio, hard and soft X-ray, and γ-ray observations of Cyg X-3 made during a flaring episode in 2010 May. We detect a ~3 day softening and recovery of the X-ray emission, followed almost immediately by a ~1 Jy radio flare at 15 GHz, followed by a 4.3σ γ-ray flare (E > 100 MeV) ~1.5 days later. The radio sampling is sparse, but we use archival data to argue that it is unlikely the γ-ray flare was followed by any significant unobserved radio flares. In this case, the sequencing of the observed events is difficult to explain in a model in which the γ-ray emission is due to inverse Compton scattering of the companion star's radiation field. Our observations suggest that other mechanisms may also be responsible for γ-ray emission from Cyg X-3.

Mueller matrix microscope with a dual continuous rotating compensator setup and digital demodulation

In this paper we describe a new Mueller matrix (MM) microscope that generalizes and makes quantitative the polarized light microscopy technique. In this instrument all the elements of the MU are simultaneously determined from the analysis in the frequency domain of the time-dependent intensity of the light beam at every pixel of the camera. The variations in intensity are created by the two compensators continuously rotating at different angular frequencies. A typical measurement is completed in a little over one minute and it can be applied to any visible wavelength. Some examples are presented to demonstrate the capabilities of the instrument.

Piirilevyn emissiivisyyden vakiointi lämpökamerasovelluksiin

Lämpökameroiden kehitys on mahdollistanut lämpökameroiden käytön myös erittäin pienien kohteiden tarkastelussa. Luotettava absoluuttisten lämpötilojen selvittäminen lämpökameralla vaatii, että tarkasteltavan kohteen emissiivisyys on kauttaaltaan vakio ja tunnettu. Käytännössä erilaisten materiaalipintojen emissiivisyyksissä on merkittäviä eroja, mikä aiheuttaa virheitä mittaustuloksiin. Tutkimuksen tavoitteena oli löytää halpa ja käytännöllinen keino piirilevyn emissiivisyyden vakiointiin. Työssä kartoitettiin erilaisia pinnoitteita, joille tehtiin resistanssi-, impedanssi- sekä lämpökameramittaukset. Mittauksilla selvitettiin pinnoitteen soveltuvuus emissiivisyyden vakiointiin. Lisäksi tutustuttiin pintapuolisesti pinnoiteaineiden kemialliseen rakenteeseen, jotta saatiin peruskäsitys siitä, onko aineiden kemiallisella rakenteella merkitystä pinnoiteaineen emissiivisyyden vakiointikykyyn. Tutkimustulosten perusteella tutkituista pinnoitteista parhaaksi todettiin talkkijauhe. Talkkipinnoitteella saatiin luotettavia mittaustuloksia. Tällä hetkellä pinnoitemenetelmää voidaan käyttää yksittäisten piirilevyjen testauksessa laboratorio-olosuhteissa. Tulevaisuudessa menetelmää voitaisiin soveltaa myös piirilevyjen tuotantolinjalle.

Deep radio images of the HEGRA and Whipple TeV sources in the Cygnus OB2 region.

The modern generation of Cherenkov telescopes has revealed a new population of gamma-ray sources in the Galaxy. Some of them have been identified with previously known X-ray binary systems while other remain without clear counterparts a lower energies. Our initial goal here was reporting on extensive radio observations of the first extended and yet unidentified source, namely TeV J2032+4130. This object was originally detected by the HEGRA telescope in the direction of the Cygnus OB2 region and its nature has been a matter of debate during the latest years. The situation has become more complex with the Whipple and MILAGRO telescopes new TeV detections in the same field which could be consistent with the historic HEGRA source, although a different origin cannot be ruled out. Aims.We aim to pursue our radio exploration of the TeV J2032+4130 position that we initiated in a previous paper but taking now into account the latest results from new Whipple and MILAGRO TeV telescopes. The data presented here are an extended follow up of our previous work. Methods.Our investigation is mostly based on interferometric radio observations with the Giant Metre Wave Radio Telescope (GMRT) close to Pune (India) and the Very Large Array (VLA) in New Mexico (USA). We also conducted near infrared observations with the 3.5 m telescope and the OMEGA2000 camera at the Centro Astronómico Hispano Alemán (CAHA) in Almería (Spain). Results.We present deep radio maps centered on the TeV J2032+4130 position at different wavelengths. In particular, our 49 and 20 cm maps cover a field of view larger than half a degree that fully includes the Whipple position and the peak of MILAGRO emission. Our most important result here is a catalogue of 153 radio sources detected at 49 cm within the GMRT antennae primary beam with a full width half maximum (FWHM) of 43 arc-minute. Among them, peculiar sources inside the Whipple error ellipse are discussed in detail, including a likely double-double radio galaxy and a one-sided jet source of possible blazar nature. This last object adds another alternative counterpart possibility to be considered for both the HEGRA, Whipple and MILAGRO emission. Moreover, our multi-configuration VLA images reveal the non-thermal extended emission previously reported by us with improved angular resolution. Its non-thermal spectral index is also confirmed thanks to matching beam observations at the 20 and 6 cm wavelengths.

Discovery of a High-Energy Gamma-Ray-Emitting Persistent Microquasar

Microquasars are stellar x-ray binaries that behave as a scaled down version of extragalactic quasars. The star LS 5039 is a new microquasar system with apparent persistent ejection of relativistic plasma at a 3 kiloparsec distance from the sun. It may also be associated with a gamma-ray source discovered by the Energetic Gamma Ray Experiment Telescope (EGRET) on board the COMPTON-Gamma Ray Observatory satellite. Before the discovery of LS 5039, merely a handful of microquasars had been identified in the Galaxy, and none of them was detected in high-energy gamma-rays.

Viivakoodin lukeminen matkapuhelimella

Purpose of this work was to study different types of barcodes and possibilities of reading them with mobile phones camera. Another goal was to transfer product information from a server to a mobile phone according to a barcode. There is existing software to read barcodes with mobile phones camera. They also open a www – page to mobile phones browser according to a URL address interpreted from a barcode. I simulated a use-case scenario, in which product delivery related information was controlled by a mobile phone. The information was located in a MySQL database and it was controlled with www – pages through mobile phones browser. I also made tests about how possible difficulties effect on successful interpretation of a barcode.

Gamma-ray emission from massive young stellar objects

Context.Massive stars form in dense and massive molecular cores. The exact formation mechanism is unclear, but it is possible that some massive stars are formed by processes similar to those that produce the low-mass stars, with accretion/ejection phenomena occurring at some point of the evolution of the protostar. This picture seems to be supported by the detection of a collimated stellar wind emanating from the massive protostar IRAS 16547-4247. A triple radio source is associated with the protostar: a compact core and two radio lobes. The emission of the southern lobe is clearly non-thermal. Such emission is interpreted as synchrotron radiation produced by relativistic electrons locally accelerated at the termination point of a thermal jet. Since the ambient medium is determined by the properties of the molecular cloud in which the whole system is embedded, we can expect high densities of particles and infrared photons. Because of the confirmed presence of relativistic electrons, inverse Compton and relativistic Bremsstrahlung interactions are unavoidable. Aims.We aim to make quantitative predictions of the spectral energy distribution of the non-thermal spots generated by massive young stellar objects, with emphasis on the particular case of IRAS 16547-4247. Methods.We study the high-energy emission generated by the relativistic electrons which produce the non-thermal radio source in IRAS 16547-4247. We also study the result of proton acceleration at the terminal shock of the thermal jet and make estimates of the secondary gamma rays and electron-positron pairs produced by pion decay. Results.We present spectral energy distributions for the southern lobe of IRAS 16547-4247, for a variety of conditions. We show that high-energy emission might be detectable from this object in the gamma-ray domain. The source may also be detectable in X-rays through long exposures with current X-ray instruments. Conclusions.Gamma-ray telescopes such as GLAST, and even ground-based Cherenkov arrays of new generation can be used to study non-thermal processes occurring during the formation of massive stars.

A microquasar model applied to unidentified gamma-ray sources

Among unidentified gamma-ray sources in the galactic plane, there are some that present significant variability and have been proposed to be high-mass microquasars. To deepen the study of the possible association between variable low galactic latitude gamma-ray sources and microquasars, we have applied a leptonic jet model based on the microquasar scenario that reproduces the gamma-ray spectrum of three unidentified gamma-ray sources, 3EG J1735-1500, 3EG J1828+0142 and GRO J1411-64, and is consistent with the observational constraints at lower energies. We conclude that if these sources were generated by microquasars, the particle acceleration processes could not be as efficient as in other objects of this type that present harder gamma-ray spectra. Moreover, the dominant mechanism of high-energy emission should be synchrotron self-Compton (SSC) scattering, and the radio jets may only be observed at low frequencies. For each particular case, further predictions of jet physical conditions and variability generation mechanisms have been made in the context of the model. Although there might be other candidates able to explain the emission coming from these sources, microquasars cannot be excluded as counterparts. Observations performed by the next generation of gamma-ray instruments, like GLAST, are required to test the proposed model.

Performance Evaluation of Imaging Systems

Imaging systems have developed latest years and developing is still continuing following years. Manufacturers of imaging systems give promises for the quality of the performance of imaging systems to advertise their products. Promises for the quality of the performance are often so good that they will not be tested in normal usage. The main target in this research is to evaluate the quality of the performance of two imaging systems: Scanner and CCD color camera. Optical measurement procedures were planned to evaluate the quality of imaging performances. Other target in this research is to evaluate calibration programs for the camera and the scanner. Measuring targets had to choose to evaluate the quality of imaging performances. Manufacturers have given definitions for targets. The third task in this research is to evaluate and consider how good measuring targets are.

Avainnustekniikat kuvaajan näkökulmasta

Työ käsittelee liikkuvan kuvan digitaalisissa erikoistehosteissa käytettäviä avainnustekniikoita kuvaajan näkökulmasta. Opinnäytetyö on monimuototyö, joka koostuu kirjallisesta osasta ja teososasta, jossa käytetään tekniikan eri sovelluksia osana fiktiivisten mainoselokuvien kerrontaa. Lähtökohtana on ollut tutkia avainnuksen toteuttamiseen liittyviä asioita käytännönläheisesti ja perehtyä teoriaan niin paljon kuin on tarpeellista, jotta tekniikan tehokas soveltaminen olisi mahdollista. Työssä käydään läpi avainnuksen historiaa lyhyesti ja esitellään sen tarjoamia mahdollisuuksia. Myös teososaa varten toteutetut avainnetut kuvat puretaan ja niiden tuloksia analysoidaan. Taustatietona esitellään jälkituotantoon liittyvää peitteiden luomisen prosessia, jonka ymmärtäminen on tärkeää myös avainnuskuvia toteuttaville kuvaajille. Valtaosa työstä on oppaan muotoon jäsenneltyä tietoa aiheesta. Työssä on pohdittu teososan toteuttamisen yhteydessä saatuja kokemuksia ja tuotu esiin myös asioita, jotka jälkikäteen ajatellen olisi kannattanut tehdä toisin. Lähdemateriaalina on käytetty aihetta tutkivia englanninkielisiä teoksia, Internetistä löytyneitä dokumentteja ja keskusteluja sekä suomalaisen jälkikäsittelyn asiantuntijan haastattelua. Työtä tehtäessä on vertailtu eri lähteitä ja pyritty rakentamaan niiden sekä työn tekijän oman kokemuksen pohjalta mahdollisimman luotettava kokonaisuus, josta olisi hyötyä kaikille avainnustekniikoiden parissa työskenteleville.

Police work and new 'security devices' : a tale from the beat

Mobile technologies have brought about major changes in police equipment and police work. If a utopian narrative remains strongly linked to the adoption of new technologies, often formulated as 'magic bullets' to real occupational problems, there are important tensions between their 'imagined' outcomes and the (unexpected) effects that accompany their daily 'practical' use by police officers. This article offers an analysis of police officers' perceptions and interactions with security devices. In so doing, it develops a conceptual typology of strategies for coping with new technology inspired by Le Bourhis and Lascoumes: challenging, neutralizing and diverting. To that purpose, we adopt an ethnographic approach that focuses on the discourses, practices and actions of police officers in relation to three security devices: the mobile digital terminal, the mobile phone and the body camera. Based on a case study of a North American municipal police department, the article addresses how these technological devices are perceived and experienced by police officers on the beat.

High mass microquasars and low latitude gamma-ray sources

Population studies of unidentified EGRET sources suggest that there exist at least three different populations of galactic gamma-ray sources. One of these populations is formed by young objects distributed along the galactic plane with a strong concentration toward the inner spiral arms of the Galaxy. Variability, spectral and correlation analysis indicate that this population is not homogeneous. In particular, there is a subgroup of sources that display clear variability in their gamma-ray fluxes on timescales from days to months. Following the proposal by Kaufman Bernad\'o et al. (2002), we suggest that this group of sources might be high-mass microquasars, i.e. accreting black holes or neutron stars with relativistic jets and early-type stellar companions. We present detailed inhomogeneous models for the gamma-ray emission of these systems that include both external and synchrotron self-Compton interactions. We have included effects of interactions between the jet and all external photon fields to which it is exposed: companion star, accretion disk, and hot corona. We make broadband calculations to predict the spectral energy distribution of these objects from radio up to GeV energies. The results and predictions can be tested by present and future gamma-ray instruments like INTEGRAL, AGILE, and GLAST.

AGNs and microquasars as high-energy gamma-ray sources

The possible associations between the microquasars LS 5039 and LS I +61 303 and the EGRET sources 3EG J1824-1514 and 3EG J0241+6103 suggest that microquasars could also be sources of high-energy gamma-rays. In this work, we present a detailed numerical inverse Compton (IC) model, based on a microquasar scenario, that reproduces the high-energy gamma-ray spectra and variability observed by EGRET for the mentioned sources. Our model considers a population of relativistic electrons entrained in a cylindrical inhomogeneous jet that interact through IC scattering with both the radiation and the magnetic fields.

Musiikkivideo musiikin ja laululyriikan näkökulmasta : kappaleen tulkintakeinoja audiovisuaalisen kokonaisuuden saavuttamiseksi musiikkivideoilmaisussa

Opinnäytetyöni on monimuototyö. Sen teososa on Ratas-yhtyeen musiikkivideo Mustavalkoinen maa. Toimin teososassani musiikkivideon käsikirjoittajana, ohjaajana, kuvaajan ja leikkaajana. Olen myös itse säveltänyt ja sanoittanut musiikin sekä soitan mukana yhtyeessä. Työ on hankkeistettu Pajula Records Oy:lle. Opinnäytetyössäni etsin keinoja audiovisuaalisen kokonaisuuden saavuttamiseksi musiikkivideoilmaisussa. Näkemykseni mukaan musiikkivideot ovat usein vain kappaleiden visuaalista täytettä, eivätkä vastaa tunnelmaltaan tai kuvaukseltaan musiikkia. Tilaajan näkökulma on usein kaupallinen, minkä johdosta musiikkivideo tehdään ulkomusiikillisten arvojen sanelemana. Opinnäytetyössäni etsin keinoja kuvan ja musiikin yhteisen sävelen musiikkivideoilmaisussa nimenomaan kappaleen näkökulmasta katsottuna. Tutkin käsitettä lyyrinen kamera, joka kuvaa kameran liikkeitä tekstissä ja käsittelen draaman rakenteen hahmottamista laululyriikassa. Etsin kuvallisia tulkintakeinoja musiikin rakenteista ja tutkin eri musiikkityyleihin yhdistettäviä tunnetiloja ja synestesian color-hearing käsitettä. Esittelen ensin muutamia konkreettisia tulkintakeinoja ja sitten sovellan käytännössä niitä teososani analyysissä. Tutkin myös teososan työprosessin aikana sitä, mitä mahdollisia hyötyjä on siitä, että koko projektista vastaa yksi henkilö.