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Statements

Subject Item
n2:RIV%2F67985831%3A_____%2F07%3A00089050%21RIV08-AV0-67985831
rdf:type
skos:Concept n14:Vysledek
dcterms:description
Na základě výsledků spektroskopie asteroidů existuje evidence že zdroj meteoritického materiálu je původem z asteroidů. Soušasně s jinými fyzikálními vlastnostmi asteroidů lze určit magnetickou susceptibilitu asteroidu na základě interakce asteroidu se slunečním větrem / solárním magnetickým polem. Magnetická susceptibilita po korekci vlivu tvaru asteroidu může být porovnána s existující databází magnetických susceptibilit meteoritů za účelem zpřesnění mineralogických podobností mezi asteroidy a meteority. Based on reflectance spectroscopy and chemical / mineralogical remote sensing methods it is generally assumed that asteroids are parent bodies for most meteorites reaching the Earth. However, more detailed observations indicate that differences exist in composition between asteroids and meteorites resulting in difficulties when searching for meteorite – asteroid match. We show that among other physical parameters the magnetic susceptibility of an asteroid can be determined on the asteroid orbit from the magnetic induction by solar wind and / or magnetic field from the Sun. The shape corrected value of the true magnetic susceptibility of an asteroid can be compared to those of meteorites in the existing database allowing closer match between asteroids and meteorites. Based on reflectance spectroscopy and chemical / mineralogical remote sensing methods it is generally assumed that asteroids are parent bodies for most meteorites reaching the Earth. However, more detailed observations indicate that differences exist in composition between asteroids and meteorites resulting in difficulties when searching for meteorite – asteroid match. We show that among other physical parameters the magnetic susceptibility of an asteroid can be determined on the asteroid orbit from the magnetic induction by solar wind and / or magnetic field from the Sun. The shape corrected value of the true magnetic susceptibility of an asteroid can be compared to those of meteorites in the existing database allowing closer match between asteroids and meteorites.
dcterms:title
Magnetic susceptibility as a tool to match asteroids and meteorites Magnetická susceptibilita jako nástroj k identifikaci spojitostí mezi asteroidy a meteority Magnetic susceptibility as a tool to match asteroids and meteorites
skos:prefLabel
Magnetická susceptibilita jako nástroj k identifikaci spojitostí mezi asteroidy a meteority Magnetic susceptibility as a tool to match asteroids and meteorites Magnetic susceptibility as a tool to match asteroids and meteorites
skos:notation
RIV/67985831:_____/07:00089050!RIV08-AV0-67985831
n3:strany
69;73
n3:aktivita
n18:Z
n3:aktivity
Z(AV0Z30130516)
n3:dodaniDat
n8:2008
n3:domaciTvurceVysledku
n12:2134616 n12:6180159 n12:1361074
n3:druhVysledku
n13:D
n3:duvernostUdaju
n19:S
n3:entitaPredkladatele
n16:predkladatel
n3:idSjednocenehoVysledku
431691
n3:idVysledku
RIV/67985831:_____/07:00089050
n3:jazykVysledku
n11:eng
n3:klicovaSlova
magnetic susceptibility; meteorite physical properties; asteroid
n3:klicoveSlovo
n4:meteorite%20physical%20properties n4:magnetic%20susceptibility n4:asteroid
n3:kontrolniKodProRIV
[55797008A2C3]
n3:mistoKonaniAkce
Oulu
n3:mistoVydani
Helsinki
n3:nazevZdroje
XXIII Geofysics days
n3:obor
n6:BN
n3:pocetDomacichTvurcuVysledku
3
n3:pocetTvurcuVysledku
5
n3:rokUplatneniVysledku
n8:2007
n3:tvurceVysledku
Elbra, T. Šlechta, Stanislav Kohout, Tomáš Pesonen, L. J. Schnabl, Petr
n3:typAkce
n15:EUR
n3:zahajeniAkce
2007-05-23+02:00
n3:zamer
n7:AV0Z30130516
s:issn
0358-2981
s:numberOfPages
5
n17:hasPublisher
Geofysiikan seura