| 000 | 03567nam a22005775i 4500 | ||
|---|---|---|---|
| 001 | 978-3-031-46273-3 | ||
| 003 | DE-He213 | ||
| 005 | 20251030111727.0 | ||
| 007 | cr nn 008mamaa | ||
| 008 | 240319s2024 sz | s |||| 0|eng d | ||
| 020 |
_a9783031462733 _9978-3-031-46273-3 |
||
| 024 | 7 |
_a10.1007/978-3-031-46273-3 _2doi |
|
| 050 | 4 | _aQB520-545 | |
| 072 | 7 |
_aPGS _2bicssc |
|
| 072 | 7 |
_aSCI004000 _2bisacsh |
|
| 072 | 7 |
_aPGS _2thema |
|
| 100 | 1 |
_aJudge, Philip. _eauthor. _4aut _4http://id.loc.gov/vocabulary/relators/aut _973286 |
|
| 245 | 1 | 4 |
_aThe Problem of Coronal Heating _h[electronic resource] : _bA Rosetta Stone for Electrodynamic Coupling in Cosmic Plasmas / _cby Philip Judge, James A. Ionson. |
| 250 | _a1st ed. 2024. | ||
| 264 | 1 |
_aCham : _bSpringer Nature Switzerland : _bImprint: Springer, _c2024. |
|
| 300 |
_aXVII, 263 p. 1 illus. _bonline resource. |
||
| 336 |
_atext _btxt _2rdacontent |
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| 337 |
_acomputer _bc _2rdamedia |
||
| 338 |
_aonline resource _bcr _2rdacarrier |
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| 347 |
_atext file _bPDF _2rda |
||
| 490 | 1 |
_aAstrophysics and Space Science Library, _x2214-7985 ; _v470 |
|
| 505 | 0 | _aIntroduction -- Magneto-hydrodynamics -- Challenges -- Methodologies -- Seeking the Sun’s Achilles’ Heels -- Fresh approaches -- Closing thoughts. | |
| 520 | _aThis book reflects on 8 decades of research on one of the longest-standing unsolved problems in modern astrophysics: why does the Sun form a hot corona? The authors give a critical overview of the field and offer suggestions on how to bridge the chasm between what we can measure, and what we can calculate. They go back to basics to explain why the problem is difficult, where we have made progress and where we have not, to help the next generation of scientists devise novel techniques to crack such a long-lasting problem. A way forward is formulated centered around refutation, using Bayesian methods to propose and to try to reject hypotheses and models, and avoiding seduction by ``confirmation bias’’. This book is aimed at physicists, students and researchers interested in understanding, learning from and solving the coronal heating problem, in an era of new dedicated facilities such as the Parker Solar Probe and the Daniel K. Inouye Solar Telescope. The book will appeal to those interested in understanding research methods and how they are changing in the modern academic environment, particular in astrophysics and Earth sciences where remote sensing is essential. | ||
| 650 | 0 |
_aSun. _968136 |
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| 650 | 0 |
_aPlasma astrophysics. _973287 |
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| 650 | 0 |
_aSampling (Statistics). _959805 |
|
| 650 | 0 |
_aAstronomy _xObservations. _967976 |
|
| 650 | 1 | 4 |
_aSolar Physics. _968138 |
| 650 | 2 | 4 |
_aAstrophysical Plasma. _973288 |
| 650 | 2 | 4 |
_aMethodology of Data Collection and Processing. _965946 |
| 650 | 2 | 4 |
_aAstronomy, Observations and Techniques. _967977 |
| 700 | 1 |
_aIonson, James A. _eauthor. _4aut _4http://id.loc.gov/vocabulary/relators/aut _973289 |
|
| 710 | 2 | _aSpringerLink (Online service) | |
| 773 | 0 | _tSpringer Nature eBook | |
| 776 | 0 | 8 |
_iPrinted edition: _z9783031462726 |
| 776 | 0 | 8 |
_iPrinted edition: _z9783031462740 |
| 776 | 0 | 8 |
_iPrinted edition: _z9783031462757 |
| 830 | 0 |
_aAstrophysics and Space Science Library, _x2214-7985 ; _v470 _973290 |
|
| 856 | 4 | 0 | _uhttps://doi.org/10.1007/978-3-031-46273-3 |
| 912 | _aZDB-2-PHA | ||
| 912 | _aZDB-2-SXP | ||
| 999 |
_c58427 _d58427 |
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