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Multiwavelength Studies of MHD Waves in the Solar Chromosphere

An Overview of Recent Results

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Abstract

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.

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Notes

  1. Note, that the value B 0 is the root of the sum of the squares of the external and internal magnetic fields, i.e., \(\langle B \rangle=\sqrt{B_{i}^{2}+B_{e}^{2}}\).

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Acknowledgements

D.B.J. wishes to thank the UK Science and Technology Facilities Council (STFC) for the award of an Ernest Rutherford Fellowship alongside a dedicated Research Grant. R.J.M is grateful to Northumbria University for their support via the award of an Anniversary Fellowship and the Leverhulme Trust (UK) for the award of an Early Career Fellowship. G.V. acknowledges the support of the Leverhulme Trust (UK). V.F. and D.B.J. are grateful to The Royal Society (Scientific Seminar Scheme) for support in organisation of the India–UK scientific seminar where the ideas contained within this paper were first discussed. S.D.T.G. thanks the Northern Ireland Department for Employment and Learning for a PhD studentship. I.G. would like to thank the University of Sheffield for a SHINE studentship.

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Authors and Affiliations

  1. Astrophysics Research Centre, School of Mathematics and Physics, Queen’s University Belfast, Belfast, BT7 1NN, Northern Ireland, UK

    D. B. Jess & S. D. T. Grant

  2. Department of Mathematics & Information Sciences, Northumbria University, Newcastle Upon Tyne, NE1 8ST, UK

    R. J. Morton

  3. Solar Physics and Space Plasma Research Centre (SP2RC), The University of Sheffield, Hicks Building, Hounsfield Road, Sheffield, S3 7RH, UK

    G. Verth & I. Giagkiozis

  4. Space Systems Laboratory, Department of Automatic Control and Systems Engineering, University of Sheffield, Sheffield, S1 3JD, UK

    V. Fedun

  5. Complex Optimization and Decision Making Laboratory, Automatic Control and Systems Engineering Department, University of Sheffield, Sheffield, S1 3JD, UK

    I. Giagkiozis

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Jess, D.B., Morton, R.J., Verth, G. et al. Multiwavelength Studies of MHD Waves in the Solar Chromosphere. Space Sci Rev 190, 103–161 (2015). https://doi.org/10.1007/s11214-015-0141-3

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