The Problem of Coronal Heating A Rosetta Stone for Electrodynamic Coupling in Cosmic Plasmas /

This 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 cal...

Ful tanımlama

Kaydedildi:
Detaylı Bibliyografya
Asıl Yazarlar: Judge, Philip (Yazar), Ionson, James A. (Yazar)
Müşterek Yazar: SpringerLink (Online service)
Materyal Türü: Elektronik Ekitap
Dil:İngilizce
Baskı/Yayın Bilgisi: Cham : Springer Nature Switzerland : Imprint: Springer, 2024.
Edisyon:1st ed. 2024.
Seri Bilgileri:Astrophysics and Space Science Library, 470
Konular:
Online Erişim:https://doi.org/10.1007/978-3-031-46273-3
Etiketler: Etiketle
Etiket eklenmemiş, İlk siz ekleyin!

MARC

LEADER 00000nam a22000005i 4500
001 978-3-031-46273-3
003 DE-He213
005 20251113191220.0
007 cr nn 008mamaa
008 240319s2024 sz | s |||| 0|eng d
020 |a 9783031462733  |9 978-3-031-46273-3 
024 7 |a 10.1007/978-3-031-46273-3  |2 doi 
050 4 |a QB520-545 
072 7 |a PGS  |2 bicssc 
072 7 |a SCI004000  |2 bisacsh 
072 7 |a PGS  |2 thema 
082 0 4 |a 523.7  |2 23 
100 1 |a Judge, Philip.  |e author.  |0 (orcid)0000-0001-5174-0568  |1 https://orcid.org/0000-0001-5174-0568  |4 aut  |4 http://id.loc.gov/vocabulary/relators/aut 
245 1 4 |a The Problem of Coronal Heating  |h [electronic resource] :  |b A Rosetta Stone for Electrodynamic Coupling in Cosmic Plasmas /  |c by Philip Judge, James A. Ionson. 
250 |a 1st ed. 2024. 
264 1 |a Cham :  |b Springer Nature Switzerland :  |b Imprint: Springer,  |c 2024. 
300 |a XVII, 263 p. 1 illus.  |b online resource. 
336 |a text  |b txt  |2 rdacontent 
337 |a computer  |b c  |2 rdamedia 
338 |a online resource  |b cr  |2 rdacarrier 
341 0 |b Table of contents navigation  |2 onix 
341 0 |b Single logical reading order  |2 onix 
341 0 |b Short alternative textual descriptions  |2 onix 
341 0 |b Use of color is not sole means of conveying information  |2 onix 
341 0 |b Use of high contrast between text and background color  |2 onix 
341 0 |b Next / Previous structural navigation  |2 onix 
341 0 |b All non-decorative content supports reading without sight  |2 onix 
347 |a text file  |b PDF  |2 rda 
490 1 |a Astrophysics and Space Science Library,  |x 2214-7985 ;  |v 470 
505 0 |a Introduction -- Magneto-hydrodynamics -- Challenges -- Methodologies -- Seeking the Sun’s Achilles’ Heels -- Fresh approaches -- Closing thoughts. 
520 |a This 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. 
532 8 |a Accessibility summary: This PDF does not fully comply with PDF/UA standards, but does feature limited screen reader support, described non-text content (images, graphs), bookmarks for easy navigation and searchable, selectable text. Users of assistive technologies may experience difficulty navigating or interpreting content in this document. We recognize the importance of accessibility, and we welcome queries about accessibility for any of our products. If you have a question or an access need, please get in touch with us at accessibilitysupport@springernature.com. 
532 8 |a No reading system accessibility options actively disabled 
532 8 |a Publisher contact for further accessibility information: accessibilitysupport@springernature.com 
650 0 |a Sun. 
650 0 |a Plasma astrophysics. 
650 0 |a Sampling (Statistics). 
650 0 |a Astronomy  |x Observations. 
650 1 4 |a Solar Physics. 
650 2 4 |a Astrophysical Plasma. 
650 2 4 |a Methodology of Data Collection and Processing. 
650 2 4 |a Astronomy, Observations and Techniques. 
700 1 |a Ionson, James A.  |e author.  |4 aut  |4 http://id.loc.gov/vocabulary/relators/aut 
710 2 |a SpringerLink (Online service) 
773 0 |t Springer Nature eBook 
776 0 8 |i Printed edition:  |z 9783031462726 
776 0 8 |i Printed edition:  |z 9783031462740 
776 0 8 |i Printed edition:  |z 9783031462757 
830 0 |a Astrophysics and Space Science Library,  |x 2214-7985 ;  |v 470 
856 4 0 |u https://doi.org/10.1007/978-3-031-46273-3 
912 |a ZDB-2-PHA 
912 |a ZDB-2-SXP 
950 |a Physics and Astronomy (SpringerNature-11651) 
950 |a Physics and Astronomy (R0) (SpringerNature-43715)