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Forward Modelling of Coronal Intensity Perturbations View all abstracts by submitter

Ineke De Moortel   Submitted: 2008-06-20 07:35

In this paper, forward modelling is used to investigate the relation between given temperature and density perturbations and the resulting (synthesised) intensity perturbations, as would be observed by e.g. TRACE and EIS (onboard Hinode). Complex and highly non-linear interactions between the components which make up the intensity (density, ionisation balance and emissivity) mean that it is non-trivial to reverse this process, i.e. obtain the density and temperature perturbations associated with observed intensity oscillations. In particular, it is found that the damping rate does not often `survive' the forward modelling process, highlighting the need for a very careful interpretation of observed (intensity) damping rates. With a few examples, it is demonstrated that in some cases even the period of the oscillations can be altered and that it is possible for two different sets of input temperature and density to lead to very similar intensities (the well-known `ill-posed' inversion process).

Authors: I. De Moortel, S.J. Bradshaw
Projects: None

Publication Status: Solar Physics (accepted)
Last Modified: 2008-09-23 20:59
Go to main E-Print page  Solar surface emerging flux regions: a comparative study of radiative MHD modeling and Hinode SOT observations  New Aspects on Particle Acceleration in Solar Flares from RHESSI Observations  Edit Entry  Download Preprint  Submitter's Homepage Delete Entry 

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