000			03030nam a22004815i 4500
001			978-3-642-16803-1
003			DE-He213
005			20140220083256.0
007			cr nn 008mamaa
008			120210s2012 gw | s |||| 0|eng d
020			_a9783642168031 _9978-3-642-16803-1
024	7		_a10.1007/978-3-642-16803-1 _2doi
050		4	_aR-RZ
072		7	_aMBGR _2bicssc
072		7	_aMED000000 _2bisacsh
082	0	4	_a610 _223
100	1		_aTroshichev, Oleg. _eauthor.
245	1	0	_aSpace Weather Monitoring by Ground-Based Means _h[electronic resource] : _bPC Index / _cby Oleg Troshichev, Alexander Janzhura.
264		1	_aBerlin, Heidelberg : _bSpringer Berlin Heidelberg : _bImprint: Springer, _c2012.
300			_aXXIII, 287 p. 127 illus., 43 illus. in color. _bonline resource.
336			_atext _btxt _2rdacontent
337			_acomputer _bc _2rdamedia
338			_aonline resource _bcr _2rdacarrier
347			_atext file _bPDF _2rda
490	1		_aSpringer Praxis Books
505	0		_aPhysical backgrounds and origin of the idea -- Concept of the PC index -- Unified procedure for on-line calculation of the 1-min PCN and PCS indices -- Validation of the unified procedure -- Differences in summer and winter PC indices and their physical reasons -- Response of PC index to sudden pulses in the solar wind dynamic pressure -- PC index as an indicator of the substorm development -- PC index as an indicator of the magnetic storm development -- PC index as an input to monitor the disturbances in the polar ionosphere -- Relationship between magnetic activity in the polar cap and atmospheric processes in the winter Antarctica -- Solar wind - magnetosphere coupling in the light of the PC dynamics.
520			_aThis book demonstrates that the method, based on the ground polar cap magnetic observations is a reliable diagnosis of  the solar wind energy coming into the magnetosphere Method for the uninterruptive monitoring of the magnetosphere state (i.e. space weather). It shows that the solar wind energy pumping power, can be described by the PC growth rate, thus,  the magnetospheric substorms features are predetermined by the PC dynamics. Furthermore, it goes on to show that the beginning and ending of magnetic storms is predictable. The magnetic storm start only if the solar energy input into the magnetosphere exceeds a certain level and stops when the energy input turns out to be below this  level.
650		0	_aMedicine.
650		0	_aMeteorology.
650		0	_aPhysical geography.
650	1	4	_aBiomedicine.
650	2	4	_aBiomedicine general.
650	2	4	_aMeteorology/Climatology.
650	2	4	_aEnvironmental Physics.
700	1		_aJanzhura, Alexander. _eauthor.
710	2		_aSpringerLink (Online service)
773	0		_tSpringer eBooks
776	0	8	_iPrinted edition: _z9783642168024
830		0	_aSpringer Praxis Books
856	4	0	_uhttp://dx.doi.org/10.1007/978-3-642-16803-1
912			_aZDB-2-SBL
999			_c101868 _d101868