The Roman Republican Navy : from the sixth century to 167 BC

Työ käsittelee Rooman laivaston kehitystä, toimintaa ja osallistumista laajenemispolitiikkaan, jossa Rooma kasvoi kaupunkivaltiosta Välimeren hallitsijaksi. Rooma on aikaisemmissa tutkimuksissa nähty maavaltiona vailla kiinnostusta merenkulkuun. On katsottu, että ainoa merkittävä merisota Rooman historiassa on ensimmäinen puunilaissota (264-241 eKr.) ja että siinäkin roomalaiset (jotka historioitsija Polybius kuvaa vasta-alkajiksi) menestyivät Karthagoa vastaan turvautumalla laskusiltoihin, joiden avulla he saattoivat muuttaa meritaistelun maataisteluksi. Polybiuksen kuvaukseen on aina tähän asti luotettu. On katsottu että Roomalla ei ollut laivastoa ennen ensimmäistä puunilaissotaa ja että Rooma kaikissa sodissaan panosti merisodankäyntiin mahdollisimman vähän. Tämä työ pyrkii kumoamaan nämä käsitykset. Laivasto oli osallisena ja ehdottoman välttämätön kaikissa Rooman laajenemispolitiikan käänteissä. Arkeologian tiedot osoittavat, että ennen ensimmäistä puunilaissotaa Rooma kehittyi ja siitä tuli merkittävä kaupunki nimenomaan kaupankäynnin ja ulkomaisten kontaktien seurauksena. Se ei siis ollut puhdas agraarivaltio. Roomalaisilla oli laivasto jo viimeistään 500-luvulta lähtien eKr. ja sitä käytettiin Rooman laajentaessa valtaansa Italiassa. Näin ollen ensimmäisessä puunilaissodassa läntisen Välimeren herruudesta kilpaili kaksi merivaltiota, Rooma ja Karthago. Toinen puunilaissota (218-201) tunnetaan yleensä Hannibalin tulosta Alppien yli Italiaan, mutta se oli myöskin merkittävä merisota ja karthagolaiset hävisivät sen nimenomaan merellä. Rooma osallistui kilpailuun itäisen Välimeren hallinnasta ja kukisti Makedonian ja Syyrian laivastot, jotka eivät olleet mitenkään Rooman laivaston veroisia. Kaikista Rooman vastustajista Karthagolla olisi ollut suurin mahdollisuus pysäyttää Rooman laivaston voittokulu toisessa puunilaissodassa. Laivastoa käytettiin moniin eri tarkoituksiin. Suuret meritaistelut eivät ole ainoa osoitus laivastojen mukanaolosta ja merkityksestä, vaan on myös otettava huomion sotalaivojen rakenne ja toimintaedellytykset. Sotalaivat oli rakennettu taisteluita varten ja niissä oli hyvin niukasti säilytystilaa. Niiden oli päästävä laskemaan maihin aina kun miehistö tarvitsi vettä, ruokaa ja lepoa. Laivastot saattoivat toimia vain niiden rannikoiden tuntumassa, joiden satamiin ja laskupaikkoihin niillä oli turvallinen pääsy. Roomalaiset olivat hyvin tietoisia tästä. Suuret merentakaiset sotaretket Afrikkaan, Espanjaan, Kreikkaan ja Vähän-Aasian rannikolle perustuivat kaikki siihen, että Rooman laivasto hallitsi purjehdusreittejä ja sopivia laskupaikkoja ja saattoi huolehtia joukkojen ja varusteiden kuljettamisesta kaukana taisteleville armeijoille. Samalla Rooman laivasto kävi itsenäistä sotaa merellä ja haastoi ja kukisti kaikki Välimeren merivaltiot. 130-luvulle eKr. tultaessa se oli lyönyt vihollisensa ja riisunut aseista liittolaisensa; Rooman laivasto hallitsi Välimerta yksin.

Strike Hard, Strike Sure - Operation Musketeer : British Military Planning during the Suez Crisis, 1956

This study analyses British military planning and actions during the Suez Crisis in 1956. It seeks to find military reasons for the change of concepts during the planning and compares these reasons with the tactical doctrines of the time. The thesis takes extensive advantage of military documents preserved in the National Archives, London. In order to expand the understanding of the exchange of views during the planning process, the private papers of high ranking military officials have also been consulted. French military documents preserved in the Service Historique de la Defence, Paris, have provided an important point of comparison. The Suez Crisis caught the British armed forces in the middle of a transition phase. The main objective of the armed forces was to establish a credible deterrence against the Soviet Union. However, due to overseas commitments the Middle East playing a paramount role because of its economic importance the armed forces were compelled to also prepare for Limited War and the Cold War. The armed forces were not fully prepared to meet this demand. The Middle Eastern garrison was being re-organised after the withdrawal from the Canal Base and the concept for a strategic reserve was unimplemented. The tactical doctrines of the time were based on experiences from the Second World War. As a result, the British view of amphibious operations and the subsequent campaigns emphasised careful planning, mastery of the sea and the air, sufficient superiority in numbers and firepower, centralised command and extensive administrative preparations. The British military had realized that Nasser could nationalise the Suez Canal and prepared an outline plan to meet this contingency. Although the plan was nothing more than a concept, it was accepted as a basis for further planning when the Canal was nationalised at the end of July. This plan was short-lived. The nominated Task Force Commanders shifted the landing site from Port Said to Alexandria because it enabled faster expansion of the bridgehead. In addition, further operations towards Cairo the hub of Nasser s power would be easier to conduct. The operational concept can be described as being traditional and was in accordance with the amphibious warfare doctrine. This plan was completely changed at the beginning of September. Apparently, General Charles Keightley, the Commander-in-Chief, and the Chairman of the Chiefs of Staff Committee developed the idea of prolonged aerial operations. The essence of the concept was to break the Egyptian will to resist by attacking the oil facilities, the transportation system and the armed forces. This victory through air concept would be supported by carefully planned psychological operations. This concept was in accordance with the Royal Air Force doctrine, which promoted a bomber offensive against selected target categories. General Keightley s plan was accepted despite suspicions at every planning level. The Joint Planning Staff and the Task Force Commanders opposed the concept from the beginning to the end because of its unpredictability. There was no information that suggested the bombing would persuade the Egyptians to submit. This problem was worsened by the fact that British intelligence was unable to provide reliable strategic information. The Task Force Commanders, who were responsible for the tactical plans, were not able to change Keightley s mind, but the concept was expanded to include a traditional amphibious assault on Port Said due to their resistance. The bombing campaign was never tested as the Royal Air Force was denied authorisation to destroy the transportation and oil targets. The Chiefs of Staff and General Keightley were too slow to realise that the execution of the plan depended on the determination of the Prime Minister. However, poor health, a lack of American and domestic support and the indecisiveness of the military had ruined Eden s resolve. In the end, a very traditional amphibious assault, which was bound to succeed at the tactical level but fail at the strategic level, was launched against Port Said.

Investigations of planetary boundary layer processes and particle formation in the atmosphere of planet Mars

The planet Mars is the Earth's neighbour in the Solar System. Planetary research stems from a fundamental need to explore our surroundings, typical for mankind. Manned missions to Mars are already being planned, and understanding the environment to which the astronauts would be exposed is of utmost importance for a successful mission. Information of the Martian environment given by models is already now used in designing the landers and orbiters sent to the red planet. In particular, studies of the Martian atmosphere are crucial for instrument design, entry, descent and landing system design, landing site selection, and aerobraking calculations. Research of planetary atmospheres can also contribute to atmospheric studies of the Earth via model testing and development of parameterizations: even after decades of modeling the Earth's atmosphere, we are still far from perfect weather predictions. On a global level, Mars has also been experiencing climate change. The aerosol effect is one of the largest unknowns in the present terrestrial climate change studies, and the role of aerosol particles in any climate is fundamental: studies of climate variations on another planet can help us better understand our own global change. In this thesis I have used an atmospheric column model for Mars to study the behaviour of the lowest layer of the atmosphere, the planetary boundary layer (PBL), and I have developed nucleation (particle formation) models for Martian conditions. The models were also coupled to study, for example, fog formation in the PBL. The PBL is perhaps the most significant part of the atmosphere for landers and humans, since we live in it and experience its state, for example, as gusty winds, nightfrost, and fogs. However, PBL modelling in weather prediction models is still a difficult task. Mars hosts a variety of cloud types, mainly composed of water ice particles, but also CO2 ice clouds form in the very cold polar night and at high altitudes elsewhere. Nucleation is the first step in particle formation, and always includes a phase transition. Cloud crystals on Mars form from vapour to ice on ubiquitous, suspended dust particles. Clouds on Mars have a small radiative effect in the present climate, but it may have been more important in the past. This thesis represents an attempt to model the Martian atmosphere at the smallest scales with high resolution. The models used and developed during the course of the research are useful tools for developing and testing parameterizations for larger-scale models all the way up to global climate models, since the small-scale models can describe processes that in the large-scale models are reduced to subgrid (not explicitly resolved) scale.

Characterization of non-imaging semiconductor X-ray solar monitors

The first observations of solar X-rays date back to late 1940 s. In order to observe solar X-rays the instruments have to be lifted above the Earth s atmosphere, since all high energy radiation from the space is almost totally attenuated by it. This is a good thing for all living creatures, but bad for X-ray astronomers. Detectors observing X-ray emission from space must be placed on-board satellites, which makes this particular discipline of astronomy technologically and operationally demanding, as well as very expensive. In this thesis, I have focused on detectors dedicated to observing solar X-rays in the energy range 1-20 keV. The purpose of these detectors was to measure solar X-rays simultaneously with another X-ray spectrometer measuring fluorescence X-ray emission from the Moon surface. The X-ray fluorescence emission is induced by the primary solar X-rays. If the elemental abundances on the Moon were to be determined with fluorescence analysis methods, the shape and intensity of the simultaneous solar X-ray spectrum must be known. The aim of this thesis is to describe the characterization and operation of our X-ray instruments on-board two Moon missions, SMART-1 and Chandrayaan-1. Also the independent solar science performance of these two almost similar X-ray spectrometers is described. These detectors have the following two features in common. Firstly, the primary detection element is made of a single crystal silicon diode. Secondly, the field of view is circular and very large. The data obtained from these detectors are spectra with a 16 second time resolution. Before launching an instrument into space, its performance must be characterized by ground calibrations. The basic operation of these detectors and their ground calibrations are described in detail. Two C-flares are analyzed as examples for introducing the spectral fitting process. The first flare analysis shows the fit of a single spectrum of the C1-flare obtained during the peak phase. The other analysis example shows how to derive the time evolution of fluxes, emission measures (EM) and temperatures through the whole single C4 flare with the time resolution of 16 s. The preparatory data analysis procedures are also introduced in detail. These are required in spectral fittings of the data. A new solar monitor design equipped with a concentrator optics and a moderate size of field of view is also introduced.

Hybrid Modelling of Titan's Interaction with the Magnetosphere of Saturn

In this dissertation we study the interaction between Saturn's moon Titan and the magnetospheric plasma and magnetic field. The method of research is a three-dimensional computer simulation model, that is used to simulate this interaction. The simulation model used is a hybrid model. Hybrid models enable individual tracking or tracing of ions and also take into account the particle motion in the propagation of the electromagnetic fields. The hybrid model has been developed at the Finnish Meteorological Institute. This thesis gives a general description of the effects that the solar wind has on Earth and other planets of our solar system. Planetary satellites can also have similar interactions with the solar wind but also with the plasma flows of planetary magnetospheres. Titan is clearly the largest among the satellites of Saturn and also the only known satellite with a dense atmosphere. It is the atmosphere that makes Titan's plasma interaction with the magnetosphere of Saturn so unique. Nevertheless, comparisons with the plasma interactions of other solar system bodies are valuable. Detecting charged plasma particles requires in situ measurements obtainable through scientific spacecraft. The Cassini mission has been one of the most remarkable international efforts in space science. Since 2004 the measurements and images obtained from instruments onboard the Cassini spacecraft have increased the scientific knowledge of Saturn as well as its satellites and magnetosphere in a way no one was probably able to predict. The current level of science on Titan is practically unthinkable without the Cassini mission. Many of the observations by Cassini instrument teams have influenced this research both the direct measurements of Titan as well as observations of its plasma environment. The theoretical principles of the hybrid modelling approach are presented in connection to the broader context of plasma simulations. The developed hybrid model is described in detail: e.g. the way the equations of the hybrid model are solved is shown explicitly. Several simulation techniques, such as the grid structure and various boundary conditions, are discussed in detail as well. The testing and monitoring of simulation runs is presented as an essential routine when running sophisticated and complex models. Several significant improvements of the model, that are in preparation, are also discussed. A main part of this dissertation are four scientific articles based on the results of the Titan model. The Titan model developed during the course of the Ph.D. research has been shown to be an important tool to understand Titan's plasma interaction. One reason for this is that the structures of the magnetic field around Titan are very much three-dimensional. The simulation results give a general picture of the magnetic fields in the vicinity of Titan. The magnetic fine structure of Titan's wake as seen in the simulations seems connected to Alfvén waves an important wave mode in space plasmas. The particle escape from Titan is also a major part of these studies. Our simulations show a bending or turning of Titan's ionotail that we have shown to be a direct result of the basic principles in plasma physics. Furthermore, the ion flux from the magnetosphere of Saturn into Titan's upper atmosphere has been studied. The modelled ion flux has asymmetries that would likely have a large impact in the heating in different parts of Titan's upper atmosphere.

Fading Customer Relationships

This dissertation is based on the assumption that fading customer relationships are important phenomena to understand in order for companies to prevent a future relationship termination, manage a desired relationship termination, or manage the situation where the relationship strength temporarily or permanently has weakened but where the customer still stays with the same service provider. It is assumed that fading could take different forms and develop through a range of different processes. The purpose of the thesis is therefore to define and describe fading, reveal different types of fading relationship processes, and discuss the dynamics of these processes. In services literature there is a lack of research focusing on the weakening of customer relationships. Fading therefore represents a new approach to understanding issues related to the ending of customer relationships. A fading relationship process could precede a relationship ending, but could also represent a temporal weakening of the relationship without leading to termination. It thus distinguishes the concept from other concepts within ending research which focus solely on relationships that have been terminated, taking a larger aspect of the relationship into account (as a relationship could build on constant changes). A pilot study created an understanding of difficulties related to understanding and detecting fading customer relationship, which led to a follow-up study incorporating qualitative interviews in relationship dyads characterised as fading with both private banking customers and their respective financial advisor. The focus remained on the understanding of the fading process resulting in a model for analysing different types of fading processes. Four types of fading processes were also revealed; the crash landing process, the altitude drop process, the fizzle out process and the try out process. The dissertation contributes to a broadened understanding of different types of fading processes within the research area of ending relationships emphasising the dynamic aspects of the phenomenon. Managerial implications include the management of different types of fading processes and also the understanding of the financial advisor’s role in influencing the development of these processes. Helena Åkerlund is associated with CERS, the Centre for Relationship Marketing and Service Management at Hanken, Swedish School of Economics and Business Administration, Helsinki

"Helvetti on kiistaton, mutta taivas on suhteellinen." : Uskonnollisten ihanteiden ja kokemuksen välinen ristiriita L. M. Montgomeryn elämässä vuosina 1921 1927

Tässä tutkimuksessa tutkittiin kanadalaisen kirjailijan L. M. Montgomeryn (1874 1942) elämää vuosina 1921 1927. Kyseisinä vuosina Montgomery eli presbyteeripapin vaimona maaseutuseurakunnissa, ensin Leaskdalessa ja sitten Norvalissa Kanadan Ontariossa. Tutkimus keskittyi tarkastelemaan kirjailijan elämää hallinnutta ristiriitaa, joka muodostui uskonnollisten ihanteiden ja yksilöllisen kokemuksen välisistä eroavaisuuksista. Primäärilähteinä olivat Montgomeryn toimitetut ja julkaistut päiväkirjat The Selected Journals of L. M. Montgomery 1 5 (1985 2004), joista käytettiin etenkin tutkimusvuosiin keskittyvää kolmatta osaa, Montgomeryn neljä romaania Emily of New Moon (1923), Emily Climbs (1925), Blue Castle (1926) ja Emily's Quest (1927) sekä Montgomeryn toimitettu ja julkaistu kirjeenvaihto After Green Gables: L. M. Montgomery's Letters to Ephraim Weber , 1916 1941 (2006) ja My Dear Mr. M.: Letters to G. B. MacMillan (1980). Lisäksi lähteinä oli Leaskdalen seurakuntalaisten kokoama muistelmateos Montgomerysta. Kirjallisuutta käytettiin kirkkohistorian, kirjallisuudentutkimuksen ja naistutkimuksen alalta. Suositusta kirjailijasta on tehty useampia elämäkertoja ja niitä hyödynnettiin tutkimuksessa. Tutkimus jakautui kahteen päälukuun, jotka toimivat toistensa vastaparina. Ensimmäinen tutkimusluku keskittyi tarkastelemaan uskonnollisia ja viktoriaanisia ihanteita, joiden mukaisesti Montgomery oli saanut kasvatuksen. Hän pyrki täyttämään näitä ihanteita myös pappilan emäntänä. Toinen tutkimusluku tarkasteli kirjailijan elämää, uskonnollisia ajatuksia ja avioliittoa julkisivun takana, jolloin kävi selvästi ilmi kirjailijan kahtiajakautunut elämä. Montgomery sai presbyteerisen ja viktoriaanisen kasvatuksen ja oppi jo lapsena huomioimaan sen, mitä muut ihmiset ajattelevat hänestä. Hän eli pienissä maaseutuyhteisöissä, joissa juoruilu oli yksi kontrollin väline. Papin vaimolla oli velvollisuuksia seurakunnassa ja pappilan hoidossa, ja Montgomery hoiti ne tarmokkaasti ja velvollisuudentuntoisesti. Hänellä oli apulainen pappilassa, jossa arki sujui viikkoaikataulun mukaisesti. Papin vaimon roolin lisäksi Montgomery jatkoi omaa kirjoittamistyötään ja hänen runsaat tulonsa mahdollistivat nelihenkisen perheen monet hankinnat. Hänen avioliittonsa oli vaikea, sillä aviomies kärsi uskonnollisesta melankoliasta ja asia piti salata seurakuntalaisilta. Montgomery käsittelee uskonnollisia teemoja romaaneissaan ja päiväkirjassaan. Hänen uskonnolliset ajatuksensa erosivat presbyteerikirkon opista useassa kohdin. Hän ei uskonut moneenkaan opinkappaleeseen, kohtasi Jumalan ennemmin luonnossa ollessaan yksin kuin kirkossa seurakunnan keskellä sekä ajatteli kristinuskon olevan jäännös menneestä ja tieteen ottaneen sen paikan Jumalan toiminnan kanavana. Kirjailijan ajattelussa on yhtymäkohtia transsendentalismiin, teosofiaan ja darwinismiin. Hän oli innokas psykologisen kirjallisuuden lukija ja sovelsi oppejaan käytäntöön. Hän uskoi unien välittävän viestejä. Kirkkokunta oli hänelle kuitenkin merkittävä identiteetin rakentaja. Papin vaimon roolin ja yksityisesti kriittisen ajattelijan roolin yhteensovittaminen aiheutti Montogmerylle ongelmia ja väsymystä. Hän kätki uskonnolliset ajatuksensa ja yksinäisyyden aiheuttaman kivun päiväkirjaansa, jonka hän toivoi julkaistavan viimeistään kuolemansa jälkeen. Kaikenlainen kirjoittaminen oli hänelle pakoa todellisuudesta ja auttoi häntä jaksamaan. Otsikon sitatti kuvaa Montgomeryn suhdetta kristinuskoon: hän käytti kristillisiä ilmauksia, mutta muokkasi niiden sisältöä omaa uskoaan vastaavaksi. Taivas ja helvetti kuvasivat usein hänen henkistä olotilaansa sanojen uskonnollisen merkityksen sijasta.

Inkluderande teaterverksamhet. Nya möjligheter för socialt arbete

I denna pro gradu-avhandling granskas teaterns möjligheter att främja social inklusion. Genom att analysera vad drama och teater kan ge ungdomar och hur social inklusion bland unga i ett samfund kan främjas, belyses även frågan om hur socialt arbete och teater ömsesidigt kan berika varandra. Avhandlingen är en fallstudie av Half Moon Young People’s Theatre, en barn- och ungdomsteater i Tower Hamlets i östra London. Teatern arbetar med barn och unga med ett särskilt fokus på att engagera grupper som ofta marginaliserats, exempelvis på grund av sin kulturella bakgrund eller till följd av funktionshinder. I denna studie är fokus på Half Moons projekt riktade till tonåringar: Careers in Theatre, Speak Up och ungdomsteatergrupperna Lunar och Solar. Studien är kvalitativ och studiens empiriska data har främst samlats in genom deltagande observation, intervjuer och granskning av dokument. Det empiriska materialet visar på Half Moons aktiva arbete för mångfald och för att göra verksamheten och deltagandet tillgängligt för alla barn och unga. Teatern blir en mötesplats genom vilken ungdomarna kan lära sig acceptera och uppskatta mångfalden i samfundet. Teaterarbetet bidrar till en ökad känsla för samfundet och till tolerans och förståelse för andra. Det är en glädjefylld, trygg och meningsfull fritidsverksamhet där nya vänskapskontakter kan knytas och många färdigheter övas inför framtiden. Teaterarbetet ger deltagarna bekräftelse vilket bidrar till att självförtroendet växer. Personalens engagemang och osjälviska arbete för inklusion genomsyrar verksamheten. Möjligheten att ge alla en ny chans och ett jämlikt bemötande är centralt i teaterns arbete. Forskningsresultaten pekar på teaterns potential inom socialt arbete och för att främja inklusion. Teaterns möjligheter att öka klientens delaktighet och utveckla förhållandet mellan socialarbetare och klient visar på betydelsen av etablera dylik verksamhet inom socialt arbete. Att inte låta sig begränsas, utan förutsättningslöst samarbeta över sektorer ökar chanserna att finna nya kreativa idéer och verksamhetsformer.