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001			280087
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008			150903s2007 xxu| o |||| 0|eng d
020			_a9780387684697 _99780387684697
024	7		_a10.1007/9780387684697 _2doi
035			_avtls000331871
039		9	_a201509030215 _bVLOAD _c201404121943 _dVLOAD _c201404091710 _dVLOAD _y201402041015 _zstaff
040			_aMX-SnUAN _bspa _cMX-SnUAN _erda
050		4	_aQB1-991
100	1		_aBone, Neil. _eautor _9304781
245	1	0	_aAurora : _bObserving and Recording Nature’s Spectacular Light Show / _cby Neil Bone.
264		1	_aNew York, NY : _bSpringer New York, _c2007.
300			_ax, 182 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		_aPatrickMoore’s Practical Astronomy Series, _x1431-9756
500			_aSpringer eBooks
505	0		_aAtmospheric Phenomena -- Causes of the Aurora -- Auroral Forecasting -- Observing the Aurora -- Historical Aurorae and More Recent Events -- Aurora Elsewhere -- Early observers and theorists of the aurora classed it along with other atmospheric phenomena as a “meteor.” In common with many of his other ideas that remained unchallenged until well into the sixteenth century, Aristotle’s fourth century BC view of these events being the result of ignition of rising vapors belowthe innermost celestial sphere prevailed for some time. An alternative, proposed by the Roman philosopher Seneca in his Questiones Naturales, was that aurorae were flames viewed through chasmata—cracks in the heavenly firmament. -- Noctilucent Clouds and other Phenomena.
520			_aThe uniquely beautiful light display of an aurora is the result of charged particles colliding with tenuous atmospheric oxygen and nitrogen, more than 60 miles above the Earth, when the magnetosphere is disturbed by changes in the solar wind. Often - and incorrectly - regarded as being confined to high northern and southern latitudes, major auroral displays are visible from even the southern USA and the south of England, and occur perhaps twenty times in each eleven-year sunspot cycle. Major auroral storms always cause great interest and excitement in the media, and of course provide practical astronomers with the opportunity to study and image them. This book describes the aurora from the amateur observational viewpoint, discusses professional studies of auroral and geomagnetic phenomena to put amateur work in context, and explains how practical observers can go about observing and recording auroral displays.
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: _z9780387360522
856	4	0	_uhttp://remoto.dgb.uanl.mx/login?url=http://dx.doi.org/10.1007/978-0-387-68469-7 _zConectar a Springer E-Books (Para consulta externa se requiere previa autentificación en Biblioteca Digital UANL)
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999			_c280087 _d280087