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(1968)Stud. Geophys. Geod. Ceskoslov. Accad. Ved. 12,108.Kurat G., Koeberl C., Presper T., Brandstätter F., Maurette M. (1994) Petrology and 289 geochemistry of Antarctic micrometeorites, Geochimica et Cosmochimica Acta 58, 38793904, doi:10.1016/0016-7037(94)90369-7.Kuropatenko V.F., Kovalenko G.V., Kuznetsova V.I., Mikhaylova G.I., Sapozhnikova G.N.(1988a), “VOLNA” program system and nonuniform difference method for calculations ofnonsteady motion of compressible continua.
Part 1: Nonuniform difference method,Questions of Nuclear Science and Technology. Series of Methods and Programs ofNumerical Solution for Problems of Mathematical Physics 2, 9-18.Kuropatenko V.F., Es’kova T.E., Kovalenko G.V., Kuznetsova V.I., Mikhaylova G.I., PotapkinB.K., Sapozhnikova G.N. (1988b) “VOLNA” program system and nonuniform differencemethod for calculations of nonsteady motion of compressible continua. Part 2:Architecture. General Organization, Questions of Nuclear Science and Technology. Seriesof Methods and Programs of Numerical Solution for Problems of Mathematical Physics 2,19-25.Kyte F.T., and Wasson J.T. (1986) Accretion rate of extraterrestrial matter: Iridium deposited 33to 67 million years ago, Science 232, 1225-1229.Langenhorst F., Pesonen L.J., Deutsch A., Hernemann U. (1999) Shock experiments on diabase:microstructural and magnetic properties, Lunar and Planetary Science Conference XXX,abs.1241.Langlais B., Purucker M.
E., and Mandea M. (2004) Crustal magnetic field of Mars, Journalof Geophysical Research 109, E02008, doi:10.1029/ 2003JE002048.Langlais B., Lesur V., Purucker M.E., Connerney J.E.P., Mandea M. (2010) Crustal magneticfields of terrestrial planets, Space Science Reviews, doi:10.1007/s11214-009- 9557-y.Lawrence K., Johnson C., Tauxe L., Gee J. (2008) Lunar paleointensity measurements:Implications for lunar magnetic evolution, Physics of the Earth Planetary Interiors 168,71–877.Lee T., Shu F.H., Shang H., Glassgold A.E., Rehm K.E.
(1998) Protostellar cosmic rays andextinct radioactivities in meteorites, Astrophysical Journal 506, 898-912.Linford N., Jackson M., Marvin J. (2002) Seahenge, Susceptibility and more ways to be wrong,The IRM Quarterly (Spring 2002), 12(1), 1&10-11.Louzada K.L., Stewart S.T., Weiss B.P. (2007) Effect of shock on the magnetic properties ofpyrrhotite, the Martian crust, and meteorites, Geophysical Research Letters 34, L05204,doi:10.1029/2006GL027685.Louzada K.L., Weiss B.P., Maloof A.C., Stewart S.T., Swanson-Hysell N.L., Soule A.
(2008)Paleomagnetism of Lonar impact crater, India, Earth and Planetary Science Letters 275,308-319, doi:10.1016/j.epsl.2008.08.025. 290 Louzada K.L., Stewart S.T. (2009) Effects of planet curvature and crust on the shock pressurefield around impact basins, Geophysical Research Letters 36,doi:10.1029/2009 GL037869.Louzada K.L., Stewart S.T., Weiss B.P., Gattacceca J., Bezaeva N.S. (2010) Shock and staticpressure demagnetization of pyrrhotite and implications for the Martian crust, Earth andPlanetary Science Letters 290(1-2), 90-101.Love S.G., Brownlee D.E. (1993) A Direct Measurement of the Terrestrial Mass Accretion Rateof Cosmic Dust, Science 262(5133), 550-553, doi: 10.1126/science.262.5133.550.Mang C., Kontny A., Fritz J., Schneider R.
(2013) Shock experiments up to 30 GPa and theirconsequences on microstructure and magnetic properties in pyrrhotite, GeochemistryGeophysics Geosystems 14(1), 64-85, doi:10.1029/2012GC004242.Martelli G., and Newton G. (1977) Hypervelocity cratering and impact magnetisation of basalt,Nature 269, 478 – 480.Martin R.J., Noel J.S. (1988) The influence of stress path on thermoremanent magnetization,Geophysical Research Letters 15, 507–510.Matuyama M.(1929) Proceedings of the Japan Academy 5, 203.Matzka J., Krasa D., Schult A., Peterson N. (2003) Magnetic state of 10-40 Ma old oceanbasalts and its implications for natural remanent magnetization, Earth and PlanetaryScience Letters 206, 541-553.McClelland E., Goss C.
(1993)Self-reversal of chemical remanent magnetization on thetransformation of maghemite to haematite, Geophysical Journal International 112, 517532.McSween H.Y. and Treiman A.H. (1998) Martian meteorites, in Planetary Materials, Rev.Mineral., . 36(6), 1 – 53, Mineral. Soc. of Am., Washington, D. C.Melosh H. J. (1989) Impact cratering: A geologic process, New York: Oxford University Press,253p.Merrill R. Grommé C.S. (1969) Non-reproducible self-reversal of magnetization in diorite,Journal of Geophysical Research 74, 2014 -2019Merill R., McElhinny M.W., McFadden P.L. (1998) The Magnetic Field of the Earth:Paleomagnetism, the Core, and the Deep Mantle, San Diego: Academic Press, 244p.Mitchell D.L., Halekas J., Lin R.P., Frey S., Hood L.L., Acuña M.H., Binder A.B. (2008) Globalmapping of lunar crustal magnetic fields by Lunar Prospector, Icarus 194, 401–409.Moh G.H. and Taylor L.A. (1971) Laboratory techniques in experimental sulfidepetrology, Neues Jahrbuch für Mineralogie, Monatshefte, 10, 450-459.Moskowitz B.M., Jackson M., Kissel C.
(1998) Low-temperature magnetic behavior oftitanomagnetites, Earth and Planetary Science Letters 157, 141-149. 291 Nagata T., Akimoto S., Uyeda S. (1951) Reverse thermoremanent magnetism, Proceedings ofthe Japan Academy 27, 643-645.Nagata T., Uyeda S., Akimoto S. (1951) Self-reversal of thermoremanent magnetization ofigneous rocks, Journal of Geomagnetism and Geoelectricity 4, 22-38.Nagata T., Uyeda S., Akimoto S. (1952) Journal of Geomagnetism and Geoelectricity 42, 22 35.Nagata T.
(1953) Self-reversal of thermoremanent magnetization of igneous rocks, Nature 172,850-852.Nagata T., Uyeda S. (1959) Exchange Interaction as a Cause of Reverse Thermo-RemanentMagnetism, Nature 184, 890-891.Nagata T., (1966) Main characteristics of piezo-magnetization and their qualitativeinterpretation, Journal of Geomagnetism and Geoelectricity 18, 81–97.Nagata T., Fisher R.M., Schwerer F.C. (1972) Lunar rock magnetism, The Moon 4, 170–196.Néel L. (1948) Propriétés magnétiques des ferrites : ferrimagnétisme et antiferromagnétisme,Annales de Physique (Paris), 3, 137-198 (Имеется перевод: сборник «Антиферромагнетизм», Москва: ИЛ, 1956).Néel L. (1951) L’inversion de l’aimantation permanente des roches, Annales de Géophysique,7(2), 90-102.Néel L.
(1952) Théorie du traînage magnétique de diffusion, Journal de Physique et le Radium13, 249-263.Néel L. (1955) Some theoretical aspects of rock magnetism, Phil. Mag. Suppl. Adv. Phys. 4,191-243.Néel L., Pauleve J., Pauthenet R., Laugier J., Dautreppe A. (1964) Magnetic Properties of anIron-Nickel Single Crystal Ordered by Neutron Bombardment, Journal of AppliedGeophysics 35, 873-876.Nikolaev A.Yu., Kozlov E.A., Yusupov D.T., Sidorov K.S., Klenov A.I., Petukhov E.A.,Yurchenko O.S., Smachnaya O.V., Lysenko O.V., Sedova O.V.
(2015) ChemicalComposition and Shock Compression of Basalt from the Vicinity of a Natural MeteoriticCrater, Proceeding of International Conference XVII Khariton’s Topical ScientificReadings. Extreme states of substance. Detonation. Shock waves, 161.Nishida J., Sasajima S. (1974) On the self-reversal of TRM in a highly oxidized submarinebasalts, Rock Magn. Palaeogeophys. 2 5-9.Nishioka I., Funaki M., Toshimori S.
(2007) Shock-induced anisotropy of magneticsusceptibility: impact experiment on basaltic andesite, Earth Planets Space 59, e45–e48.Nord G.L., Lawson C.A. (1989) Order-disorder transition-induced twin domains and magnetic 292 properties in ilmenite-hematite, American Mineralogist 74, 160-176.Nyquist L.E., Bogard D.D., Shih C.Y., Stoffler D., Eugster O. (2001) Ages and geologichistories of Martian meteorites, Space science Review 96, 105-164.O’Reilly W., Banerjee S.K. (1966) Oxidation of titanomagnetites and self-reversal, Nature 211,26-28.Orlicky O. (2002) Field-reversal versus self-reversal hypothesis: Paleomagnetic properties andmagnetic mineralogy of selected Neogene hornblende pyroxene andesites of centralSlovakia (Part II) Contributions to Geophysics and Geodesy 32(1), 1-?? .Ozima M., Larson E.E. (1968)Study of Self-reversal of TRM in some Submarine Basalts,Journal of Geomagnetism and Geoelectricity, 20(4), 337-351.Ozima M., Funaki M., Hamada N., Aramaki S.
and Fujii T. (1992)Self-reversal ofthermoremanent magnetization in pyroclastics from the 1991 eruption of Mt. Pinatubo,Philippines, Journal of Geomagnetism and Geoelectricity 44, 979 -984.Ozima M., Funaki M. (2001) Magnetic properties of hemoilmenite single crystals in Harunadacite pumice revealed by the Bitter technique, with special reference to self-reversal ofthermoremanent magnetization Earth Planets Space 53, 111-119.Ozima M., Funaki M. (2003) Hemoilmenite as a carrier of SRTRM in dacitic pumice fromAkagi, Ontake and Sambre Volcanoes, Japan, Earth and Planetary Science Letters 213,311-320.Ozima M., Oshima O., Funaki M. (2003) Magnetic properties of pyroclastic rocks from the laterstage of the eruptive activity of Haruna Volcano in relation to the self-reversal ofthermoremanent magnetization, Earth Planets Space 55, 183-188Papike J.J.
(1981) The lunar regolith: significance of the chemistry of the <10 µm fraction and amodel for agglutinate formation involving fusion of the finest fraction (F3), Lunar andPlanetary Science Conference XII, 851-853.Pearce G.W. and Karson J.A. (1981) On pressure demagnetization, Geophysical ResearchLetters 8, 725 – 728.Pesonen L.J., Marcos, N., Pipping, F. (1992) Palaeomagnetism of the Lappajärvi impactstructure, western Finland, Tectonophysics 216, 123–142.Pesonen L.J., Deutsch A., Hornemann U., Langenhorst F. (1997) Magnetic properties of diabasesamples shocked experimentally in the 4.5 to 35 GPa range, Lunar and Planetary ScienceConference XXVIII, abs.1370. 293 Pieters C.M., Taylor L.A., Noble S.K., Keller L.P., Hape B., Morris R.V., Allen C.C., McKayD.S., Wentworth S. (2000) Space weathering on airless bodies: resolving a mystery withlunar samples, Meteoritics & Planetary Science 35, 1101-1107.Pilkington M., Grieve R.A.F.
(1992) The geophysical signature of terrestrial impact craters,Geophysical Review 30, 161–181.Pohl J., Bleil U., Hornemann U. (1975) Shock magnetization and demagnetization of basalt bytransient stress up to 10 kbar Geophysical Journal 41, 23-41.Pohl J., Eckstaller A. (1981) The effect of shock on remanence in multi-domain iron grains andimplications for palaeointensity measurements, Lunar and Planetary Science XII, 851–853abstract.Popova O.P., Jenniskens P., Emel’yanenko V., Kartashova A., Biryukov E., Khaibrakhmanov S.,Shuvalov V., Rybnov Y., Dudorov A., Grokhovsky V.I., Badyukov D.D., Yin Q.Z., GuralP.S., Albers J., Granvik M., Evers L.G., Kuiper J., Kharlamov V., Solovyov A., RusakovY.S., Korotkiy S., Serdyuk I., Korochantsev A.V., Larionov M.Y., Glazachev D., MayerA.E., Gisler G., Gladkovsky S.V., Wimpenny J., Sanborn M.E., Yamakawa A., VerosubK.L., Rowland D.J., Roeske S., Botto N.W., Friedrich J.M., Zolensky M.E., Le L., RossD., Ziegler K., Nakamura T., Ahn I., Lee J.I., Zhou Q., Li X.H., Li Q.L., Liu Y., TangG.Q., Hiroi T., Sears D., Weinstein I.A., Vokhmintsev A.S., Ishchenko A.V., SchmittKopplin P., Hertkorn N., Nagao K., Haba M.K., Komatsu M., and Mikouchi T.
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