000			03936nam a22003975i 4500
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007			cr nn 008mamaa
008			150903s2012 gw | o |||| 0|eng d
020			_a9783642294174 _99783642294174
024	7		_a10.1007/9783642294174 _2doi
035			_avtls000359035
039		9	_a201509031018 _bVLOAD _c201405070240 _dVLOAD _y201402191545 _zstaff
040			_aMX-SnUAN _bspa _cMX-SnUAN _erda
050		4	_aQB460-466
100	1		_aObridko, Vladimir N. _eeditor. _9344805
245	1	4	_aThe Sun: New Challenges : _bProceedings of Symposium 3 of JENAM 2011 / _cedited by Vladimir N. Obridko, Katya Georgieva, Yury A. Nagovitsyn.
264		1	_aBerlin, Heidelberg : _bSpringer Berlin Heidelberg : _bImprint: Springer, _c2012.
300			_aviii, 237 páginas 106 ilustraciones _brecurso en línea.
336			_atexto _btxt _2rdacontent
337			_acomputadora _bc _2rdamedia
338			_arecurso en línea _bcr _2rdacarrier
347			_aarchivo de texto _bPDF _2rda
490	0		_aAstrophysics and Space Science Proceedings, _x1570-6591 ; _v30
500			_aSpringer eBooks
505	0		_a1. The unusual sunspot minimum - challenge to the solar dynamo theory -- 2. The evolution of cyclic activity of the Sun in the context of physical processes on late-type stars -- 3. Long-term variations of the solar supergranulation size according to the observations in CaIIK line -- 4. On the Problem of Heat Transport in the Solar Atmosphere -- 5. Dynamics of the electrical currents in coronal magnetic loops -- 6. Observations of solar flares from GHz to THz frequencies -- 7. On the Interaction of Solar Rotational Discontinuities with a Contact Discontinuity Inside the Solar Transition Region as a Source of Plasma Heating in the Solar Corona -- 8. Complex magnetic evolution and magnetic helicity in the solar Atmosphere -- 9. On Our Ability to Predict Major Solar Flares -- 10. Chormospheric Evaporation in Solar Flares -- 11. Evolutionary of Discontinuous Plasma Flows in the Vicinity of Reconnecting Current Layers -- 12. Analytical Models of Generalized Syrovatskiis Current Layer with MHD Shock Waves -- 13. Solar Convection And Self-Similar Atmospheres Structures -- 14. SDO in Pulkovo Observatory -- 15. Variations of microwave emission and MDI topology in the Active Region NOAA 10030 before and during the power flare series -- 16. Scenario of evolution of the epoch of minimum at the final stage of Cycle 23 -- 17. Solar magnetic fields as a clue for the mystery of the permanent solar wind and the solar corona -- 18. Two types of coronal bright points in the 24-th cycle of solar activity -- 19. The Self-Similar Shrinkage of Force-Free Magnetic Flux Ropes in a Passive Medium of Finite Conductivity -- 20. Solar Activity Indices In The Cycles 21–23 -- 21. Coronal Mass Ejections on the Sun and their Relationship with Flares and Magnetic Helicity.
520			_aThese are the proceedings of the Symposium 3 of JENAM 2011 on new scientific challenges posed by the Sun. The topics covered are   1. The unusual sunspot minimum, which poses challenges to the solar dynamo theory 2. The Sun’s Terra-Hertz emission, which opens a new observational window 3. Corona wave activity 4. Space weather agents - initiation, propagation, and forecasting In 21 in-depth contributions, the reader will be presented with the latest findings.
590			_aPara consulta fuera de la UANL se requiere clave de acceso remoto.
700	1		_aGeorgieva, Katya. _eeditor. _9344806
700	1		_aNagovitsyn, Yury A. _eeditor. _9344807
710	2		_aSpringerLink (Servicio en línea) _9299170
776	0	8	_iEdición impresa: _z9783642294167
856	4	0	_uhttp://remoto.dgb.uanl.mx/login?url=http://dx.doi.org/10.1007/978-3-642-29417-4 _zConectar a Springer E-Books (Para consulta externa se requiere previa autentificación en Biblioteca Digital UANL)
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999			_c305700 _d305700