Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/8563
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dc.contributor.authorKumar, Hirdesh-
dc.contributor.authorBrajesh Kumar-
dc.contributor.authorMathew, Shibu K-
dc.contributor.authorBayanna, A. Raja-
dc.contributor.authorRajaguru, S. P-
dc.date.accessioned2024-11-04T05:17:55Z-
dc.date.available2024-11-04T05:17:55Z-
dc.date.issued2024-09-01-
dc.identifier.citationThe Astrophysical Journal, Vol. 972, No. 1, 39en_US
dc.identifier.issn1538-4357-
dc.identifier.urihttp://hdl.handle.net/2248/8563-
dc.descriptionOpen Acessen_US
dc.descriptionOriginal content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.-
dc.description.abstractWe report and discuss the phase shift and phase travel time of low-frequency (ν < 5.0 mHz) acoustic waves estimated within the photosphere and photosphere–chromosphere interface regions, utilizing multiheight velocities in the quiet Sun. The bisector method has been employed to estimate seven height velocities in the photosphere within the Fe I 6173 Å line scan, while nine height velocities are estimated from the chromospheric Ca II 8542 Å line scan observations obtained from the narrowband imager instrument installed on the Multi-Application Solar Telescope operational at the Udaipur Solar Observatory, India. Utilizing a fast Fourier transform at each pixel over the full field of view, phase shift and coherence have been estimated. The frequency and height-dependent phase shift integrated over the regions having an absolute line-of-sight magnetic field of less than 10 G indicates the nonevanescent nature of low-frequency acoustic waves within the photosphere and photosphere–chromosphere interface regions. Phase travel time estimated within the photosphere shows nonzero values, aligning with previous simulations and observations. Further, we report that the nonevanescent nature persists beyond the photosphere, encompassing the photospheric–chromospheric height range. We discuss possible factors contributing to the nonevanescent nature of low-frequency acoustic waves. Additionally, our observations reveal a downward propagation of high-frequency acoustic waves indicating refraction from higher layers in the solar atmosphere. This study contributes valuable insights into the understanding of the complex dynamics of acoustic waves within different lower solar atmospheric layers, shedding light on the nonevanescent nature and downward propagation of the acoustic waves.en_US
dc.language.isoenen_US
dc.publisherThe American Astronomical Societyen_US
dc.relation.urihttps://doi.org/10.3847/1538-4357/ad5d60-
dc.rights© 2024.The Author(s)-
dc.subjectSolar oscillationsen_US
dc.subjectQuiet sunen_US
dc.subjectHelioseismologyen_US
dc.subjectSolar photosphereen_US
dc.subjectSolar chromosphereen_US
dc.titleInvestigation of phase shift and travel time of acoustic waves in the lower solar atmosphere using multiheight velocitiesen_US
dc.typeArticleen_US
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