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<article language="en">
	<journal>
		<journal_title>Astrophysics and Space Sciences Transactions</journal_title>
		<journal_url>www.astrophys-space-sci-trans.net</journal_url>
		<issn>1810-6528</issn>
		<eissn>1810-6536</eissn>
		<volume_number>4</volume_number>
		<issue_number>2</issue_number>
		<publication_year>2008</publication_year>
	</journal>
	<doi>10.5194/astra-4-59-2008</doi>
	<article_url>http://www.astrophys-space-sci-trans.net/4/59/2008/</article_url>
	<abstract_html>http://www.astrophys-space-sci-trans.net/4/59/2008/astra-4-59-2008.html</abstract_html>
	<fulltext_pdf>http://www.astrophys-space-sci-trans.net/4/59/2008/astra-4-59-2008.pdf</fulltext_pdf>
	<start_page>59</start_page>
	<end_page>63</end_page>
	<publication_date>2008-12-04</publication_date>
	<article_title content_type="html">Forbush decrease of the galactic cosmic ray intensity: experimental study and theoretical modeling</article_title>
	<authors>
		<author numeration="1" affiliations="1,2">
			<name>M. V. Alania</name>
		</author>
		<author numeration="2" affiliations="3">
			<name>A. Wawrzynczak</name>
		</author>
	</authors>
	<affiliations>
		<affiliation numeration="1" content_type="html">Institute of Math. and Physics of University of Podlasie, Siedlce, Poland</affiliation>
		<affiliation numeration="2" content_type="html">Institute of Geophysics, Georgian Academy of Sciences, Tbilisi, Georgia</affiliation>
		<affiliation numeration="3" content_type="html">Institute of Computer Science of University of Podlasie, Siedlce, Poland</affiliation>
	</affiliations>
	<abstract content_type="html">We study the temporal changes of the power law rigidity spectrum
of the Forbush decrease (Fd) of the galactic cosmic ray (GCR)
intensity. We show that the power law rigidity spectrum of Fd for
the period of  6–20 November 2004 found by neutron monitors and
ground muon telescopes experimental data, gradually is hardening
during the decreasing phase of the intensities and then steadily
is softening during the recovery phase. A relation of the rigidity
spectrum exponent of the Fd of the GCR intensity with the exponent
of the power spectral density (PSD) of the components of the
interplanetary magnetic field (IMF) turbulence is established. We
develop three dimensional (3-D) non stationary model of the Fd and
show that the results of the theoretical modeling are in good
agreement with the experimental data. We suppose that temporal
changes of the rigidity spectrum exponent of the Fd of GCR
intensity can be used to calculate the exponent of the PSD of the
IMF turbulence for the arbitrary period, which is not achievable
by the in situ measurements of the IMF.</abstract>
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</article>
