'Field models' presentation slideshows

Content of the talk

Content of the talk. Exotic clustering in neutron-rich nuclei Brief overview for the history of the cluster study Cluster model v.s. Density functional theory for the study of the stability of the cluster states Connection between cluster structure and shell structure.

509 views • 50 slides

The Solar Dynamo I M.R.E.Proctor DAMTP, University of Cambridge

The Solar Dynamo I M.R.E.Proctor DAMTP, University of Cambridge. Leeds, 6 September 2005. Indicators of the Solar Cycle: Sunspots. Cyclical behaviour of the Sun is shown by the evolution of sunspots, observed since time of Galileo.

556 views • 43 slides

Solar stereoscopy - where we are and which developments do we require to progress?

Solar stereoscopy - where we are and which developments do we require to progress?. Thomas Wiegelmann, Bernd Inhester, Li Feng, Judith de Patoul. How?. What do we have and what we want?. 3D geometry/physics of e.g. coronal loops and polar plumes. EUV-images from 2 viewpoints.

508 views • 43 slides

Solar stereoscopy - where we are and which developments do we require to progress?

Solar stereoscopy - where we are and which developments do we require to progress?. Thomas Wiegelmann, Bernd Inhester, Li Feng, Judith de Patoul. How?. What do we have and what we want?. 3D geometry/physics of e.g. coronal loops and polar plumes. EUV-images from 2 viewpoints.

437 views • 43 slides

Experimental measurement of the deformation through the electromagnetic probe

484 views • 38 slides

1. FY08 GOES-R3 Project Proposal Title Page

1. FY08 GOES-R3 Project Proposal Title Page. Title : Space Weather Risk Reduction for GOES-R including Solar Observing Instruments (SUVI and EUVS), In-situ Instruments (SEISS and MAG) and Data Browse and Retrieval Interface

362 views • 24 slides

SECCHI-3D reconstruction software

SECCHI-3D reconstruction software. Wiegelmann, Inhester, Feng, Ruan, Thalmann, Podlipnik. Tools to compute coronal magnetic fields Selfconsistent magnetohydrostatic equilibria Feature recognition Stereoscopy Tomography. Aim: 3D Reconstruction of Solar Corona.

315 views • 19 slides

M- flation after BICEP2

Cosmo 2014 Chicago, IL August 25 th , 2014. M- flation after BICEP2. Amjad Ashoorioon (Lancaster University). Mainly in collaboration with Shahin Sheikh- Jabbari (IPM ). Based on A.A, M.M . Sheikh- Jabbari , arXiv:1405.1685 [ hep-th ]]

263 views • 17 slides

Baroclinic Instability Variations

300 views • 11 slides

E-Field Models

232 views • 8 slides

Separating internal geomagnetic secular variation and long-term magnetospheric field variations

Separating internal geomagnetic secular variation and long-term magnetospheric field variations. Monika Korte Deutsches GeoForschungsZentrum GFZ. Motivation. Separation of different geomagnetic field sources remains a challenge

269 views • 6 slides