61 research outputs found
Multiwavelength studies of MHD waves in the solar chromosphere: An overview of recent results
The chromosphere is a thin layer of the solar atmosphere that bridges the
relatively cool photosphere and the intensely heated transition region and
corona. Compressible and incompressible waves propagating through the
chromosphere can supply significant amounts of energy to the interface region
and corona. In recent years an abundance of high-resolution observations from
state-of-the-art facilities have provided new and exciting ways of
disentangling the characteristics of oscillatory phenomena propagating through
the dynamic chromosphere. Coupled with rapid advancements in
magnetohydrodynamic wave theory, we are now in an ideal position to thoroughly
investigate the role waves play in supplying energy to sustain chromospheric
and coronal heating. Here, we review the recent progress made in
characterising, categorising and interpreting oscillations manifesting in the
solar chromosphere, with an impetus placed on their intrinsic energetics.Comment: 48 pages, 25 figures, accepted into Space Science Review
Isozyme and RAPD studies in Prosopis glandulosa and P. Velutina (Leguminosae, Mimosoideae)
Ethylene evolution and endo-beta-mannanase activity during lettuce seed germination at high temperature
Man's Impact on the Antarctic Environment, by W. A. Benninghoff & W.N. Bonner. Scientific Committee on Antarctic Research, Scott Polar Research Institute, Cambridge, England, UK: 55 pp., illustr., 24.5 × 17.0 × 0.5 cm, stiff paper cover, available from the above, 1985.
Regulation of myocardial BARK1 expression in catecholamine-induced cardiac hypertrophy in transgenic mice overexpression alpha1B-adrenergic receptors.
International Management Games: Laboratories for Performance‐based Intercultural Learning
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