Crassostrea patagonica (d'Orbigny, 1842) shell concentrations from the late Miocene Rio Negro province, NE Patagonia, Argentina

The Río Negro Formation (late Miocene-early Pliocene) mainly consists of continental deposits, but it contains a middle member of marine origin. It represents a transgressive-regressive sequence that can be seen at several outcrops along the N Patagonian coast. The taphonomical approach to the El Espigón marine deposits permits the identification of four main layers containing different kinds of skeletal accumulation, which mainly consist of oyster shells [Crassostrea patagonica (D'Orbigny, 1842)]. These concentrations display three different morphologies (pouches, pavements and bouquets) with a different taphonomic signature. These deposits were formed in shallow marine environments influenced by wave activity that produced valve concentrations of different entities. They contain several shell beds that represent event, composite, hiatal to lag skeletal concentrations. Traces of bioturbation in the sediment (Thalassinoides, Teichichnus) and bioerosion on the shells (Entobia, Gastrochaeonolites, Caulostrepsis), and encrusters (cirripeds, bryozoans), are also abundant in the outcrop and consititue common components of these Miocene materials. Layers 1 and 2 of the sequence were deposited in shoreface/foreshore environments at the beginning of a highstand systems tract, while layers 3 and 4 were deposited at the end, or at the beginning of a forced regression, in foreshore environments. A final erosional episode cut the top of the layer 4, which truncated the abundant bioturbaation developed there.

Sisäisen toimittajan palvelutasosopimuksen kehittäminen ja toimitusvarmuuden parantaminen, CASE: oy Shell ab

Tämän tutkielman tarkoituksena on tehostaa toimitusketjua kehittämällä palvelutasosopimusta ja parantamalla toimitusvarmuutta toimittajan ja oy Shell ab:n välillä. Työssä perehdytään näiden kahden yrityksen väliseen sopimukseen ja toimitusvarmuutta kuvaavaan mittariin nimeltä Supplier OTIF. Nykytila arvioidaan molempien osalta ja mahdollisia parantavia toimenpiteitä tuodaan esille. Tämä tutkimus perustuu yrityksessä työskentelyn ohella haastatteluihin, kyselyihin sekä omiin havaintoihin eri osastoilla. Työn teoriaosuudessa tarkastellaan ostosopimuksen yleisintä kaupallista sisältöä. Lisäksi paneudutaan palveluyrityksen käytäntöihin, tulkitaan palveluyrityksen suorituskykyä ja sen mittaamista tunnuslukujen avulla. Tutkimus osoittaa, että niin palvelutasosopimus kuin toimitusvarmuuskin eivät ole riittävällä tasolla case-yrityksessä. Erityisesti osapuolien välistä yhteistyötä ja tiedonjakoa on parannettava tavoitteiden saavuttamiseksi. Työssä esiteltyjen kehitys- ja parannusehdotusten osittainen käyttöönotto aikaansai toimitusketjun tehokkaamman toiminnan. Case-yrityksen tuleekin harkita lisätoimenpiteiden käyttöönottoa. Toiminnan sekä yhteistyön parantaminen yhä edelleen jää case-yrityksen ja toimittajien yhteisesti tulevaisuudessa tehtävien ratkaisujen varaan.

Cluster structure of atomic nuclei

Kirjallisuusarvostelu

Multifrequency VLBI Observations of Selected Active Galactic Nuclei

In this dissertation, active galactic nuclei (AGN) are discussed, as they are seen with the high-resolution radio-astronomical technique called Very Long Baseline Interferometry (VLBI). This observational technique provides very high angular resolution (_ 10−300 = 1 milliarcsecond). VLBI observations, performed at different radio frequencies (multi-frequency VLBI), allow to penetrate deep into the core of an AGN to reveal an otherwise obscured inner part of the jet and the vicinity of the AGN’s central engine. Multi-frequency VLBI data are used to scrutinize the structure and evolution of the jet, as well as the distribution of the polarized emission. These data can help to derive the properties of the plasma and the magnetic field, and to provide constraints to the jet composition and the parameters of emission mechanisms. Also VLBI data can be used for testing the possible physical processes in the jet by comparing observational results with results of numerical simulations. The work presented in this thesis contributes to different aspects of AGN physics studies, as well as to the methodology of VLBI data reduction. In particular, Paper I reports evidence of optical and radio emission of AGN coming from the same region in the inner jet. This result was obtained via simultaneous observations of linear polarization in the optical and in radio using VLBI technique of a sample of AGN. Papers II and III describe, in detail, the jet kinematics of the blazar 0716+714, based on multi-frequency data, and reveal a peculiar kinematic pattern: plasma in the inner jet appears to move substantially faster that that in the large-scale jet. This peculiarity is explained by the jet bending, in Paper III. Also, Paper III presents a test of the new imaging technique for VLBI data, the Generalized Maximum Entropy Method (GMEM), with the observed (not simulated) data and compares its results with the conventional imaging. Papers IV and V report the results of observations of the circularly polarized (CP) emission in AGN at small spatial scales. In particular, Paper IV presents values of the core CP for 41 AGN at 15, 22 and 43 GHz, obtained with the help of the standard Gain transfer (GT) method, which was previously developed by D. Homan and J.Wardle for the calibration of multi-source VLBI observations. This method was developed for long multi-source observations, when many AGN are observed in a single VLBI run. In contrast, in Paper V, an attempt is made to apply the GT method to single-source VLBI observations. In such observations, the object list would include only a few sources: a target source and two or three calibrators, and it lasts much shorter than the multi-source experiment. For the CP calibration of a single-source observation, it is necessary to have a source with zero or known CP as one of the calibrators. If the archival observations included such a source to the list of calibrators, the GT could also be used for the archival data, increasing a list of known AGN with the CP at small spatial scale. Paper V contains also calculation of contributions of different sourced of errors to the uncertainty of the final result, and presents the first results for the blazar 0716+714.

Tukkukauppiaille : Shell hintaluettelo C

kuv., 21 x 27 cm

Shell huolto

kuv., 15 x 22 cm

Kuluttajille : Shell hintaluettelo C

kuv., 21 x 27 cm

Shell service

kuv., 15 x 22 cm

Kuluttajille : Shell hintaluettelo C

kuv., 22 x 27 cm

Shell prislista

kuv., 22 x 28 cm

Shell huolto

kuv., 15 x 22 cm

Kuluttajille : Shell hintaluettelo C

kuv., 22 x 27 cm

Shell service

kuv., 15 x 22 cm