2,138 research outputs found
Magneto-seismology of solar atmospheric loops by means of longitudinal oscillations
There is increasingly strong observational evidence that slow magnetoacoustic
modes arise in the solar atmosphere. Solar magneto-seismology is a novel tool
to derive otherwise directly un-measurable properties of the solar atmosphere
when magnetohydrodynamic (MHD) wave theory is compared to wave observations.
Here, MHD wave theory is further developed illustrating how information about
the magnetic and density structure along coronal loops can be determined by
measuring the frequencies of the slow MHD oscillations. The application to
observations of slow magnetoacoustic waves in coronal loops is discused.Comment: 4 pages, 2 figures, to appear in Proceedings of IAU Symp 286,
Comparative Magnetic Minima, C. H. Mandrini, ed
A conceptual framework to analyse the multiscalar politics of education for sustainable peacebuilding
Rethinking the state and education in conflict-affected contexts:a co-constructed auto-ethnography of supportive mentorship and academic friendship
Reclaiming Reconciliation through Community Education for the Muslims and Tamils of post-war Jaffna, Sri Lanka
‘The fruit caught between two stones’: the conflicted position of teachers within Aceh's independence struggle
The Retention of Organic and Inorganic Compounds on Clay Minerals. Part II: The Interaction of Attaplugus Clay and Polyphenylic Nuclear Reactor Coolants. EUR 2646.
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