The Propagation of Coherent Waves Across Multiple Solar Magnetic Pores | Samuel Grant
Queen's University Belfast, United Kingdom
Natural Sciences (Astrophysics and Astrononmy)
Solar pores have long been documented as efficient magnetic conduits for propagating magnetohydrodynamic wave energy from the photosphere into the outer regions of the solar atmosphere. Observations of pores often contain isolated and/or unconnected structures, which prevents the statistical examination of wave activity inter- play as a function of atmospheric height. Here, using high resolution observations acquired by the Dunn Solar Telescope, we examine photospheric and chromospheric wave signatures stemming from a unique collection of magnetic pores originating from the same decaying sunspot.
See more at https://espos.stream/2022/05/26/Grant/.
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