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020 _a9783642200151
_99783642200151
024 7 _a10.1007/9783642200151
_2doi
035 _avtls000356772
039 9 _a201509030549
_bVLOAD
_c201405060410
_dVLOAD
_y201402191301
_zstaff
040 _aMX-SnUAN
_bspa
_cMX-SnUAN
_erda
050 4 _aQB495-500.269
100 1 _aChernov, Gennady P.
_eautor
_9341095
245 1 0 _aFine Structure of Solar Radio Bursts /
_cby Gennady P. Chernov.
264 1 _aBerlin, Heidelberg :
_bSpringer Berlin Heidelberg :
_bImprint: Springer,
_c2011.
300 _axvI, 284 páginas
_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 Library,
_x0067-0057 ;
_v375
500 _aSpringer eBooks
505 0 _aPreface -- Acknowledgments -- 1 Introduction -- 2 Pulsations -- 3 Spike bursts -- 4 Zebra pattern and fiber bursts -- 5 Recent results of zebra patterns in solar radio bursts -- References -- Subject Index.
520 _aThe study of the fine structure of solar radio emissions is key to understanding plasma processes in the solar corona. It remains a reliable means for both diagnosing the corona and verifying the results of laboratory plasma experiments on wave-wave and wave-particle interactions. This monograph provides a comprehensive review of the fine structure of solar radio bursts. Based on the diversity of experimental data resulting from the progress made in observational techniques, the validity of various theoretical models is reexamined. The book serves as an up-to-date reference work for all researchers in this field.
590 _aPara consulta fuera de la UANL se requiere clave de acceso remoto.
710 2 _aSpringerLink (Servicio en línea)
_9299170
776 0 8 _iEdición impresa:
_z9783642200144
856 4 0 _uhttp://remoto.dgb.uanl.mx/login?url=http://dx.doi.org/10.1007/978-3-642-20015-1
_zConectar a Springer E-Books (Para consulta externa se requiere previa autentificación en Biblioteca Digital UANL)
942 _c14
999 _c302710
_d302710