Sökning: "plage"
Visar resultat 1 - 5 av 9 avhandlingar innehållade ordet plage.
1. Physical properties of chromospheric features : Plage, peacock jets, and calibrating it all
Sammanfattning : The chromosphere is a complex and dynamic layer of the solar atmosphere, largely dominated by the local magnetic field configuration. It acts as an important interface between the photosphere below it and the hot corona above. However, studying this layer is not straightforward, as it is largely transparent in optical wavelengths. LÄS MER
2. Investigating magnetic fields in the solar chromosphere
Sammanfattning : Solar plage has been the topic of many studies since its initial description in the mid 19th century, but as of yet it has not been understood to the point where we can reproduce all aspects of these active regions in quasi-realistic numerical models. To a large extent, this is caused by an incomplete understanding of the magnetic structure that drives the activity in these areas. LÄS MER
3. Entre identification et différenciation : La mère et l’amour dans la constitution de l’identité féminine dans La fille démantelée, La plage d’Ostende et Orlanda de Jacqueline Harpman
Sammanfattning : The aim of this dissertation is to investigate the importance of the mother figure for the definition of the female identity in three novels by the Belgian writer and psychoanalyst Jacqueline Harpman: La fille démantelée, La plage d’Ostende and Orlanda. This perspective is largely motivated by the specific character of the mother-daughter relation which is crucial to the formation of female identity. LÄS MER
4. Entre identification et différentiation : Étude de la relation entre mère et fille dans "La Fille démantelée" et "La Plage d'Ostende" de Jacqueline Harpman
Sammanfattning : .... LÄS MER
5. Imaging spectropolarimetry of solar active regions
Sammanfattning : Solar magnetic fields span a wide range of spatial scales from sunspots and plages to magnetic bright points. A clear understanding of the physical processes underlying the evolution of these magnetic features requires high-resolution spectropolarimetric observations of solar active regions and comparisons with synthetic data from simulations. LÄS MER