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- W2964189806 endingPage "014001" @default.
- W2964189806 startingPage "014001" @default.
- W2964189806 abstract "As waves and oscillations carry both energy and information, they have enormous potential as a plasma heating mechanism and, through seismology, to provide estimates of local plasma properties which are hard to obtain from direct measurements. Being sufficiently near to allow high-resolution observations, the atmosphere of the Sun forms a natural plasma laboratory. Recent observations have revealed that an abundance of waves and oscillations is present in the solar atmosphere, leading to a renewed interest in wave heating mechanisms." @default.
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- W2964189806 date "2015-10-20" @default.
- W2964189806 modified "2023-10-18" @default.
- W2964189806 title "Transverse, propagating velocity perturbations in solar coronal loops" @default.
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- W2964189806 doi "https://doi.org/10.1088/0741-3335/58/1/014001" @default.
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