03362nam a22005295i 4500001001800000003000900018005001700027007001500044008004100059020003700100024003500137050001400172072001600186072002300202072001500225100008300240245016000323250001800483264006900501300004400570336002600614337002600640338003600666347002400702490006200726505015500788520119000943650001602133650003202149650003402181650003602215650002602251650003302277650005802310650005102368700008502419710003402504773002602538776003602564776003602600776003602636830006902672856004602741912001402787912001402801999001702815978-3-031-46273-3DE-He21320251030111727.0cr nn 008mamaa240319s2024    sz |    s    |||| 0|eng d  a97830314627339978-3-031-46273-37 a10.1007/978-3-031-46273-32doi 4aQB520-545 7aPGS2bicssc 7aSCI0040002bisacsh 7aPGS2thema1 aJudge, Philip.eauthor.4aut4http://id.loc.gov/vocabulary/relators/aut97328614aThe Problem of Coronal Heatingh[electronic resource] :bA Rosetta Stone for Electrodynamic Coupling in Cosmic Plasmas /cby Philip Judge, James A. Ionson.  a1st ed. 2024. 1aCham :bSpringer Nature Switzerland :bImprint: Springer,c2024.  aXVII, 263 p. 1 illus.bonline resource.  atextbtxt2rdacontent  acomputerbc2rdamedia  aonline resourcebcr2rdacarrier  atext filebPDF2rda1 aAstrophysics and Space Science Library,x2214-7985 ;v4700 aIntroduction -- Magneto-hydrodynamics -- Challenges -- Methodologies -- Seeking the Sun’s Achilles’ Heels -- Fresh approaches -- Closing thoughts.  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. 0aSun.968136 0aPlasma astrophysics.973287 0aSampling (Statistics).959805 0aAstronomyxObservations.96797614aSolar Physics.96813824aAstrophysical Plasma.97328824aMethodology of Data Collection and Processing.96594624aAstronomy, Observations and Techniques.9679771 aIonson, James A.eauthor.4aut4http://id.loc.gov/vocabulary/relators/aut9732892 aSpringerLink (Online service)0 tSpringer Nature eBook08iPrinted edition:z978303146272608iPrinted edition:z978303146274008iPrinted edition:z9783031462757 0aAstrophysics and Space Science Library,x2214-7985 ;v47097329040uhttps://doi.org/10.1007/978-3-031-46273-3  aZDB-2-PHA  aZDB-2-SXP  c58427d58427