000 03872nam a22004455i 4500
001 978-1-4614-3761-1
003 DE-He213
005 20140220083248.0
007 cr nn 008mamaa
008 120328s2012 xxu| s |||| 0|eng d
020 _a9781461437611
_9978-1-4614-3761-1
024 7 _a10.1007/978-1-4614-3761-1
_2doi
050 4 _aQB495-500.269
072 7 _aTTDS
_2bicssc
072 7 _aSCI005000
_2bisacsh
082 0 4 _a520
_223
082 0 4 _a500.5
_223
100 1 _aFan, Yuhong.
_eeditor.
245 1 0 _aSolar Flare Magnetic Fields and Plasmas
_h[electronic resource] /
_cedited by Yuhong Fan, George Fisher.
264 1 _aNew York, NY :
_bSpringer US,
_c2012.
300 _aVIII, 202p. 50 illus., 25 illus. in color.
_bonline resource.
336 _atext
_btxt
_2rdacontent
337 _acomputer
_bc
_2rdamedia
338 _aonline resource
_bcr
_2rdacarrier
347 _atext file
_bPDF
_2rda
505 0 _aEfficient Techniques for Radiation Transfer in Three-Dimensional MHD Models -- Radiative Cooling in MHD Models of the Quiet Sun Convection Zone and Corona -- Understanding Flare Radiation Processes -- Global Forces and Momenta During Solar Flare Energy Release -- The Evolution of Sunspot Magnetic Fields Associated with a Solar Flare -- Global Forces in Eruptive Solar Flares -- Data Analysis and Theory for Analysis of Vector Magnetogram Data -- Modeling and Interpreting the Effects of Spatial Resolution on Solar Magnetic Field Maps -- Magnetic Connectivity Between Active Regions 10987, 10988, 10989 by Means of Nonlinear Force-Free Field Extrapolation -- Magnetic Energy Storage and Current Density Distributions for Different Force-Free Models -- Connections Between Magnetic Topology in the Solar Atmosphere and Eruptive Flares and CMEs -- Predictions of Energy and Helicity in Four Major Eruptive Solar Flares.
520 _aThis volume is devoted to the dynamics and diagnostics of solar magnetic fields and plasmas in the Sun’s atmosphere. Five broad areas of current research in Solar Physics are presented: (1) New techniques for incorporating radiation transfer effects into three-dimensional magnetohydrodynamic models of the solar interior and atmosphere, (2) The connection between observed radiation processes occurring during flares and the underlying flare energy release and transport mechanisms, (3) The global balance of forces and momenta that occur during flares, (4) The data-analysis and theoretical tools needed to understand and assimilate vector magnetogram observations and (5) Connecting flare and CME phenomena to the topological properties of the magnetic field in the Solar Atmosphere. The role of the Sun’s magnetic field is a major emphasis of this book, which was inspired by a workshop honoring Richard C. (Dick) Canfield.  Dick has been making profound contributions to these areas of research over a long and productive scientific career.  Many of the articles in this topical issue were first presented as talks during this workshop and represent substantial original work.  The workshop was held 9 – 11 August 2010, at the Center Green campus of the National Center for Atmospheric Research (NCAR) in Boulder, Colorado. This volume is aimed at researchers and graduate students active in solar physics, solar-terrestrial physics and magneto-hydrodynamics. Previously published in Solar Physics journal, Vol. 277/1, 2012.
650 0 _aPhysics.
650 0 _aAstrophysics.
650 1 4 _aPhysics.
650 2 4 _aExtraterrestrial Physics, Space Sciences.
650 2 4 _aPlasma Physics.
700 1 _aFisher, George.
_eeditor.
710 2 _aSpringerLink (Online service)
773 0 _tSpringer eBooks
776 0 8 _iPrinted edition:
_z9781461437604
856 4 0 _uhttp://dx.doi.org/10.1007/978-1-4614-3761-1
912 _aZDB-2-PHA
999 _c101437
_d101437