Sporadic-E layers (Es) are layers of metallic ions that appear in the lower E-region of the ionosphere and can last from under one hour to several hours. Es are found at all latitudes, but polar cap Es, and specifically over Svalbard at a latitude of around 78◦ , are the focus of this study. Data is provided from several instruments: the EISCAT Svalbard Dynasonde, the EISCAT Svalbard Incoherent Scatter Radar (ESR), SuperDARN, and modelled data from the latest Horizontal Wind Model (HWM14). Data on the Interplanetary Magnetic Field (IMF) is acquired from the NASA OMNIWeb data base. It is found that polar cap Es are a summer phenomenon, confined to the later afternoon to a couple of hours after midnight in universal time (UT), with a peak occurrence between 18-21 UT. The layer heights are mostly confined to ∼92-120 km, although there is a discrepancy between Es found in ESR data and Dynasonde data, with ESR events being confined to 92-110 km, and Dynasonde events to 95-120 km. It is also found that Es occurrence is dependent on Interplanetary Magnetic Field (IMF) direction, with a higher occurrence during a southward and eastward IMF. The Dynasonde automatic signal processing of echoes is found to be unreliable at times with intense E-region density enhancements, such as Es. From a Superposed Epoch Analysis (SEA) on Es found in ESR data, it is found that there is a density buildup from the start of the events, peaking by 30 % of the Es lifetime, that is followed by fading at a slower rate until the end of the layer lifetime. Layer thickness is found to be largely confined to <9 km. From SuperDARN E-field data it is found that layers can form and migrate downwards to low altitudes for a strictly northward E-field. ’Flat’, low altitude layers are found during E-field directions in both the southwest and northwest quadrants. Some cases of Es formation and migration fit current theories and whilst some does not. Indications of particle precipitation that induce layer formation is found. / Sporadiska E-skikt (Es) är lager av metalliska joner som uppträder i den nedre delen av jonosfärens E-region, och kan pågå från under en timme till flera timmar. Es återfinns på alla breddgrader, men Es i polarområdet, och specifikt över Svalbard på en latitud av cirka 78◦ , är fokuset för denna studie. Data tillhandahålls från flera instrument: EISCAT Svalbard Dynasonde, EISCAT Svalbard Incoherent Scatter Radar (ESR), SuperDARN och modellerade data från en updaterad modell för horisontella neutrala vindar (HWM14). Data om det interplanetära magnetfältet (IMF) hämtas från NASAs OMNIWeb databas. Det visas att Es i polarområdet är ett sommarfenomen, begränsat till mellan eftermiddagen och ett par timmar efter midnatt i universell tid (UT), med en toppförekomst mellan 18-21 UT. Höjd för skikten är mestadels begränsade till ∼92-120 km, men det finns en diskrepans mellan Es funna ur ESR-data och Dynasonde-data, med fallen från ESR data begränsade till 92-110 km och fall från Dynasonde-datan till 95-120 km. Det visas också att Es-förekomsten är beroende av det interplanetära magnetfältets (IMF) riktning, med en högre förekomst under IMF riktat söderut och österut. Dynasondens automatiska signalbehandling av ekon visas vara opålitlig under intensiva förhöjningar i E-regionens densitet, såsom är fallet vid sporadiska E-skikt. Genom en ’Superposed Epoch Analysis’ (SEA) som genoförs för de Es som lokaliseras i ESR-datan, visar det sig att det finns en densitetsuppbyggnad från början av Es fallen, med en densitetstopp vid 30 % av Es-livslängden, som sedan följs av en långsammare avtrappning tills skiktet helt dött ut. Skikttjockleken visar sig vara i stort sett begränsad till <9 km. Ur E-fältdata från SuperDARN visar det sig att lager kan bildas och migrera nedåt, till låga höjder för ett nordligt riktat E-fält. ’Platta’ skikt på låg höjd återfinns under E-fältsriktningar i både sydvästra och nordvästra kvadranten. Vissa fall med Es formation och migration följer teorin på området medan andra fall inte gör det. Det finns vissa indikationer på att partikelprecipitation kan inducera skiktbildning.

As one of the most common minerals in crustal rocks, quartz has been widely used as an indicator for shock metamorphism. Shocked quartz is found in the Chicxulub impact crater, an impact crater that has been linked to the Cretaceous-Tertiary extinction ~66 million years ago. The microstructural deformation features found in the shocked quartz do not form randomly, and their orientation provides a better understanding of the impact cratering process. At present, there are no studies of EBSD data analysis of shocked quartz from Chicxulub. We investigated six thin sections from two samples from the M0077A borehole in the lower peak ring of the Chicxulub impact crater, using the Scanning Electron Microscopy (SEM)-EBSD technique. Both samples consist of shocked granite, with a significant amount of quartz.  Therefore, this study investigates the crystallographic preferred orientation (CPO) of shocked quartz and predicts the seismic velocities and anisotropy, based on the EBSD data. We carried out the analysis of EBSD data by using the MATLAB-based MTEX toolbox that can perform CPO analysis from pole figure plots and the prediction of seismic properties of minerals based on the Voigt-Reuss-Hill effective medium method. Although acquiring the EBSD data from these samples is challenging, leading to the lack of data measured, we found out that the prediction of P wave seismic velocity is in good agreement with other recent studies conducted in the same area. The range of predicted P wave velocities is 5.5-6.5 km/s with anisotropy of 8-15%. The actual observed laboratory measurements and in-situ seismic measurements are considerably smaller than this velocity range because our calculations do not incorporate pores or take microcracks into account.  A likely explanation for the large variability of anisotropy in shocked quartz is the relatively few mapped grains with EBSD, which would influence the CPO and lead to high predicted seismic anisotropy. Considering a greaternumber of grains in the CPO analysis, the CPO is reduced, and seismic anisotropy becomes smaller.

The Northern Norrbotten ore district hosts a multitude of Sweden’s mineral deposits including world class deposits such as the Malmberget and Kirunavaara Iron oxide apatite deposits, the Aitik Iron oxide copper gold deposit, and a multitude of smaller deposits. Northern Norrbotten has been shaped by tectonothermal events related to the evolution of the Fennoscandian Shield and is a geologically complex environment. Without extensive rock outcropping and with most drilling localized to known deposits the regional to local scale of mineralization is not fully understood. To better understand the evolution and extent of the mineralization’s cross-disciplinary geosciences must be applied, where geophysical methods allow for interpretations of the deep and non-outcropping subsurface. Common earth modelling is a term describing a joint model derived from all available geoscientific data in an area, where geophysical models provide the framework.This study describes the geophysical modeling of two IOA deposits in Norrbotten, the Malmberget deposit in Gällivare and the Per-Geijer deposit in Kiruna. To better put these two deposits into a semi-regional setting magnetotelluric (MT) measurements have been conducted together with LKAB. LTU and LKAB have measured more than 200 MT stations in the two areas from 2016-2023. These measurements have then been robustly processed into magnetic transfer functions (impedances) for the broadband MT frequency spectrum (1000Hz,1000s). Then, all processed data judged to be of sufficient quality have been used for 3D inversion modelling using the ModEM code. The resulting conductivity/resistivity models reveals the local conductivity structure of the area, believed to be closely tied to the mineralization due to the conductive properties of the iron bearing minerals. Both areas yielded believable models which pinpointed known mineralization’s at surface as conductive anomalies and their connections to deeper regional anomalies.During modelling a robust iteratively re-weighted least square (IRLS) scheme has been implemented in the inversion algorithms. This scheme allows for objective re-weighting of data errors based on the ability for a given model discretization to predict individual datums. This, to better identify measurements which have been contaminated by local electromagnetic noise due to anthropogenic sources (mainly the power grid and railway). Due to the mathematical properties of the scheme, it allows for models which minimizes the L1 data error-norm instead of usual L2 minimization. This has yielded models whit sharper contrasts in resistivity and successfully emphasizes data believed to be reliable. Results indicate that the scheme was implemented successfully and the tradeoffs in data-fit are deemed acceptable.In addition, in the Kiruna study potential field data (magnetic total field and gravimetry) have been 3D modelled for the same area. These data sets have been inversion modelled in 3D using the MR3D-code developed at LTU with partners. Resulting 3D models have then been interpreted collectively both traditionally and with the use of machine learning methods. To guide interpretations more than 100 rock samples have been collected in the area and their petrophysical properties (density, magnetic susceptibility, electrical resistivity) have been measured at LTU. These petrophysical properties have been used to guide the machine learning methods for the 3D models by first using K-mean clustering on normalized petrophysical data and then using the resulting centroid vectors as input for a Gaussian mixture model of the similarly normalized 3D models. Resulting clusters show potential in being able to pick up sharp geological boundaries but expectedly is unable to fully capture geological structures one to one.

Shore displacement has largely affected both the natural landscape and the humans within. This is especially true for Västergarn parish on Gotland, where low-lying plains make up large parts of the domain. Yet, the land–sea interaction of Västergarn, has not been studied closely for a long time. Through a comprehensive study, as well as a reexamination, of different sources and materials, this study aims to shed new light on the spatial distribution and chronology of Västergarn. To understand this, we need to get a scope of the extent of the sea. Previous research (e.g. Ilves & Darmark 2011; Mikołajczyk et al. 2015) has showed that phosphate analysis may help indicate the position of former shorelines. How can this, methodologically, be applied to phosphate-mapping carried out well over 50 years ago? This thesis does not aim to completely answer this question, but rather to analyze what went into determining a shore-level for 1000 AD during earlier research (e.g. Lundström 1979, 1981). Moreover, this study aims to critically examine the interplay between historical shore-levels and the built world within Västergarn. The Västergarn defensive wall and Paviken bay constitute the two main areas of study, owing to the pursuit of understanding the interplay between these two sites. Västergarn cannot be fully understood without also including the Kronholmen peninsula (formerly island, as the name suggests), why some attention is also directed towards this area. / Strandförskjutningen har till stor del påverkat både naturlandskapet och människorna inom. Detta stämmer i synnerhet för Västergarns socken på Gotland, där i princip hela området är att betrakta som synnerligen låglänt. Ändå har relationen mellan land och hav i Västergarn, inte utforskats närmare på länge. Genom att inkludera och ompröva ett flertal olika källor och material, syftar denna studie till att på nytt belysa Västergarns rumsliga fördelning och kronologi. Tidigare forskning (se Ilves & Darmark 2011; Mikołajczyk et al. 2015) har visat på att analys fosfatvärden kan bära med sig insikt i forna strandlinjenivåer. Hur kan denna kunskap metodologiskt tillämpas på fosfatkarteringar som genomfördes för mer än 50 år sedan? Denna uppsats syftar inte till att fullständigt besvara denna fråga, men däremot att närma sig vad som legat till grund för att fastställa en strandnivå för 1000 e.Kr. under tidigare forskning (se Lundström 1979, 1981). Huvudfokus för denna studie är att kritiskt granska samspelet mellan historiska strandlinjenivåer och bebyggelse i Västergarn. Västergarnsvallen och Paviken utgör, i strävan efter att förstå relationen mellan dessa två platser, de huvudsakliga studieområdena. Västergarn kan dock inte förstås till fullo utan att även blicka mot halvön Kronholmen (tidigare ö, som namnet vittnar om), varför en viss uppmärksamhet också riktas mot detta område.

<p>This paper deals with archaeological prospection of an Iron Age farm site in Toland, Fresta parish, Uppland County in Sweden. The purpose of the paper has been to see whether the geophysical methods applied (GPR & EM-38) could produce useful results that could motivate its use in similar surveys in the future. Geochemistry has been used for the purpose of identifying possible activity areas on the site. The results have shown that it is possible with a GPR survey to identify postholes originating from the Migration Period longhouse at the site. The combining of several methods have been important for the identification and interpretation of several areas of interest.</p>

This paper deals with archaeological prospection of an Iron Age farm site in Toland, Fresta parish, Uppland County in Sweden. The purpose of the paper has been to see whether the geophysical methods applied (GPR &amp; EM-38) could produce useful results that could motivate its use in similar surveys in the future. Geochemistry has been used for the purpose of identifying possible activity areas on the site. The results have shown that it is possible with a GPR survey to identify postholes originating from the Migration Period longhouse at the site. The combining of several methods have been important for the identification and interpretation of several areas of interest.

An integrated use of radio magnetotelluric (RMT) and controlled source tensor magnetotelluric (CSTMT) measurements, the so-called CSRMT method, has been employed in environmental and resource exploration studies. A number of case histories, including a groundwater investigation in glacial deposits, a study of fracture zones for geotechnical purposes and a mining exploration study of a copper deposit, are presented in this thesis in order to illustrate the usefulness and capability of the CSRMT method. The resolutions of the estimated models using various types of data are studied. Magnetotelluric transfer functions are used to analyze the dimensionality, the near surface resistivity distortions and the near field effects in the case of CSTMT data analysis. The near field effects in CSTMT data have also been identified by performing 2½D forward modelling. Data analysis, dimensionality tests and forward modelling show that at the lowest frequencies used the CSTMT transfer functions are generally distorted by source effects, except when the source-receiver distances are sufficient large compared with the penetration depth. Regarding CSTMT transfer functions, apparent resistivities are generally less distorted than phases. TM mode transfer functions are more affected by the sources than TE mode, while tipper vectors generally contain source signatures at all frequencies. Based on the analysis of dimensionality and source effects 2D inverse modelling of CSTMT and RMT data, as well as their combination, have been performed under the plane wave assumption. The RMT method proved to be a powerful tool for imaging the upper 50 m near-surface, but their penetration depth reduces as a conductive layer structures cover the targets at depth. The penetration depth can be increased by including the CSTMT data in the modelling if the measurements are in the far field range. The resolution of the deeper parts of the models may be improved by performing a joint inversion of TE and TM modes, if the strike direction is well-defined. Alternatively, inversion of determinant data can be performed, since the determinant data are less affected by 3D structures and source effects. However the resolution of the determinant models is somewhat degraded compared to the models inverted from combined TE and TM modes.

Laboratory magnetic measurements are used to develop a methodology to characterize the Kiruna-type Rare Earth Elements (REE) bearing apatite iron-oxide deposits at Blötberget in central Sweden. This high-grade ore deposit is known to have sharp boundaries between lens shaped main ore bodies of magnetite-rich ore, and a complex hematite-rich ore associated with pegmatites and skarn formation. The thesis covers laboratory magnetic measurements of 37 samples originating from eight drill cores and reference samples from previously mined area. It focuses on on-covering how the samples relate in terms of magnetic susceptibility, further its dependency on temperature, frequency, field and the orientation. The results are correlated with petrographic analysis previously performed on accompanying thin sections. The measurements show that magnetite with strong susceptibility contribution overshadow the hematite contribution in the samples. Transition changes in susceptibility are noticeable when crossing the Verwey temperature; -153°C, Curie temperature; 580°C and Néel temperature; 680°C. The Morin temperature appears at -60°C, or is missing. Linear relationships are identified between the magnitude difference in susceptibilities across transitions at high temperature and wt% magnetite and hematite have been identified. The Blötberget skarn and hematite-rich ore samples have a higher degree of susceptibility anisotropy than the other ore-types. Blötberget samples are dominated by multidomain characteristics in remanence, saturation and coercivity. High temperature measurements have shown that the magnetite is close to pure. The low temperature measurements suggest hematite is impure or bears a petrological footprint. The study also shows that rich iron ore samples sometimes can be at risk of being overlooked with standard methods of measuring susceptibility / Laboratorietekniska metoder kan användas som ett komplement till malmgeologi och geofysisk prospektering. I denna metodstudie karaktäriseras apatitjärnmalm från Blötberget, nära Grängesberg. En fyndighet bestående av linsformade malmkroppar rika på magnetit och ofta avskilda men komplexa hematitrika stråk. Studien är gjord 37 prover från totalt 8 borrkärnor, och lokaler som tillhörde produktion från gruvverksamhet under 1900-talet. Mätmetoderna fokuserar på att kartlägga malmens magnetiska egenskaper, och hur temperatur, frekvens, fältstyrka samt riktning påverkar dessa. Resultaten jämfördes med tidigare petrografisk studie av tillhörande tunnslip Resultaten visar att magnetit står för merparten av susceptibiliteten i proverna, men att även hematit kan urskiljas och kvantifieras. Temperaturberoende har påvisats vid övergångar för Verwey-temperatur; -153°C, Curie-temperatur; 580 °C, och Néeltemperatur; 680 °C. Den förväntade Morin-temperaturen vid -14°C, påträffades vid -60 °C eller saknas helt för flera av de hematitrika proverna. Magnetiskt anisotropa prover återfinns bland prover som identifierats som skarn eller hematitrika. Magnetisk granulometri visar karaktär av multidomäntyp med låg magnetisk coercivitet och hög satureringsförmåga. Högtemperaturmätningar av susceptibilitet visar på ren magnetit för prover från Blötberget. Samtidigt visar lågtemperaturemätningar att hematit sannolikt har inblandning av titanium eller bär på ett mer komplext förflutet. Studien visar också att det finns en risk i att enbart förlita sig på bulksusceptibilitet för prover rika på malm.

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Mars’ climate has undergone many massive changes over the course of it’s lifetime. In order toestablish how Mars lost the vast majority of its water, we must be able to understand how Marsis losing its atmosphere today. By understanding the current escape rates of H and D and theprocesses that control them, we can extrapolate back in time to model the escape rates under pastconditions. By using the Exospheric General Model (EGM) developed by researchers at LATMOS,Sorbonne University, I have simulated the density profiles and escape rates of H, D, related isotopesand particles due to collisions with hot oxygen particles in the Martian exosphere at the currentepoch at mean solar activity. By adding H and D to the model and implementing changes to theprogram between simulations, I have improved the accuracy of the escape rate of these particlesfrom Mars in the EGM. While my results for H, H2 and HD reflect what has been observed fromin-situ Martian Satellite, MAVEN, future work is needed to include the solar wind interaction for Din the model, as it has been shown to be significant and has been left out of this work.