LEADER 03339nam 22006255 450 001 9910845095603321 005 20240321231811.0 010 $a3-031-46273-4 024 7 $a10.1007/978-3-031-46273-3 035 $a(MiAaPQ)EBC31221916 035 $a(Au-PeEL)EBL31221916 035 $a(DE-He213)978-3-031-46273-3 035 $a(CKB)30995940000041 035 $a(EXLCZ)9930995940000041 100 $a20240319d2024 u| 0 101 0 $aeng 135 $aurcnu|||||||| 181 $ctxt$2rdacontent 182 $cc$2rdamedia 183 $acr$2rdacarrier 200 14$aThe Problem of Coronal Heating $eA Rosetta Stone for Electrodynamic Coupling in Cosmic Plasmas /$fby Philip Judge, James A. Ionson 205 $a1st ed. 2024. 210 1$aCham :$cSpringer Nature Switzerland :$cImprint: Springer,$d2024. 215 $a1 online resource (275 pages) 225 1 $aAstrophysics and Space Science Library,$x2214-7985 ;$v470 311 $a3-031-46272-6 327 $aIntroduction -- Magneto-hydrodynamics -- Challenges -- Methodologies -- Seeking the Sun?s Achilles? Heels -- Fresh approaches -- Closing thoughts. 330 $aThis book reflects on 8 decades of research on one of the longest-standing unsolved problems in modern astrophysics: why does the Sun form a hot corona? The authors give a critical overview of the field and offer suggestions on how to bridge the chasm between what we can measure, and what we can calculate. They go back to basics to explain why the problem is difficult, where we have made progress and where we have not, to help the next generation of scientists devise novel techniques to crack such a long-lasting problem. A way forward is formulated centered around refutation, using Bayesian methods to propose and to try to reject hypotheses and models, and avoiding seduction by ``confirmation bias??. This book is aimed at physicists, students and researchers interested in understanding, learning from and solving the coronal heating problem, in an era of new dedicated facilities such as the Parker Solar Probe and the Daniel K. Inouye Solar Telescope. The book will appeal to those interested in understanding research methods and how they are changing in the modern academic environment, particular in astrophysics and Earth sciences where remote sensing is essential. 410 0$aAstrophysics and Space Science Library,$x2214-7985 ;$v470 606 $aSun 606 $aPlasma astrophysics 606 $aSampling (Statistics) 606 $aAstronomy$xObservations 606 $aSolar Physics 606 $aAstrophysical Plasma 606 $aMethodology of Data Collection and Processing 606 $aAstronomy, Observations and Techniques 615 0$aSun. 615 0$aPlasma astrophysics. 615 0$aSampling (Statistics). 615 0$aAstronomy$xObservations. 615 14$aSolar Physics. 615 24$aAstrophysical Plasma. 615 24$aMethodology of Data Collection and Processing. 615 24$aAstronomy, Observations and Techniques. 676 $a523.7 700 $aJudge$b Philip$01733521 701 $aIonson$b James A$01733522 801 0$bMiAaPQ 801 1$bMiAaPQ 801 2$bMiAaPQ 906 $aBOOK 912 $a9910845095603321 996 $aThe Problem of Coronal Heating$94149355 997 $aUNINA