MHD waves in the solar atmosphere / (Record no. 84357)
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| 000 -LEADER | |
|---|---|
| fixed length control field | 02569nam a22003858i 4500 |
| 001 - CONTROL NUMBER | |
| control field | CR9781108613774 |
| 005 - DATE AND TIME OF LATEST TRANSACTION | |
| control field | 20240730160827.0 |
| 008 - FIXED-LENGTH DATA ELEMENTS--GENERAL INFORMATION | |
| fixed length control field | 170911s2019||||enk o ||1 0|eng|d |
| 020 ## - INTERNATIONAL STANDARD BOOK NUMBER | |
| ISBN | 9781108613774 (ebook) |
| 082 00 - CLASSIFICATION NUMBER | |
| Call Number | 523.7/6 |
| 100 1# - AUTHOR NAME | |
| Author | Roberts, Bernard, |
| 245 10 - TITLE STATEMENT | |
| Title | MHD waves in the solar atmosphere / |
| 300 ## - PHYSICAL DESCRIPTION | |
| Number of Pages | 1 online resource (xx, 508 pages) : |
| 500 ## - GENERAL NOTE | |
| Remark 1 | Title from publisher's bibliographic system (viewed on 15 Jul 2019). |
| 505 0# - FORMATTED CONTENTS NOTE | |
| Remark 2 | General principles page -- Waves in a uniform medium -- Magnetically structured atmospheres -- Surface waves -- Magnetic slabs -- Magnetic flux tubes -- The twisted magnetic flux tube -- Connection formulas -- Gravitational effects -- Thin flux tubes : the sausage mode -- Thin flux tubes : the kink mode -- Damping -- Nonlinear aspects -- Solar applications of mhd wave theory. |
| 520 ## - SUMMARY, ETC. | |
| Summary, etc | This volume presents a full mathematical exposition of the growing field of coronal seismology which will prove invaluable for graduate students and researchers alike. Roberts' detailed and original research draws upon the principles of fluid mechanics and electromagnetism, as well as observations from the TRACE and SDO spacecraft and key results in solar wave theory. The unique challenges posed by the extreme conditions of the Sun's atmosphere, which often frustrate attempts to develop a comprehensive theory, are tackled with rigour and precision; complex models of sunspots, coronal loops and prominences are presented, based on a magnetohydrodynamic (MHD) view of the solar atmosphere, and making use of Faraday's concept of magnetic flux tubes to analyse oscillatory phenomena. The rapid rate of progress in coronal seismology makes this essential reading for those hoping to gain a deeper understanding of the field. |
| 856 40 - ELECTRONIC LOCATION AND ACCESS | |
| Uniform Resource Identifier | https://doi.org/10.1017/9781108613774 |
| 942 ## - ADDED ENTRY ELEMENTS (KOHA) | |
| Koha item type | eBooks |
| 264 #1 - | |
| -- | Cambridge : |
| -- | Cambridge University Press, |
| -- | 2019. |
| 336 ## - | |
| -- | text |
| -- | txt |
| -- | rdacontent |
| 337 ## - | |
| -- | computer |
| -- | c |
| -- | rdamedia |
| 338 ## - | |
| -- | online resource |
| -- | cr |
| -- | rdacarrier |
| 650 #0 - SUBJECT ADDED ENTRY--SUBJECT 1 | |
| -- | Helioseismology. |
| 650 #0 - SUBJECT ADDED ENTRY--SUBJECT 1 | |
| -- | Magnetohydrodynamic waves. |
| 650 #0 - SUBJECT ADDED ENTRY--SUBJECT 1 | |
| -- | Fluid dynamics. |
| 650 #0 - SUBJECT ADDED ENTRY--SUBJECT 1 | |
| -- | Solar atmosphere. |
| 650 #0 - SUBJECT ADDED ENTRY--SUBJECT 1 | |
| -- | Electromagnetism. |
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