27 research outputs found

    Cosmic ray acceleration by stellar wind. Simulation for heliosphere

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    The solar wind deceleration by the interstellar medium may result in the existence of the solar wind terminal shock. In this case a certain fraction of thermal particles after being heated at the shock would obtain enough energy to be injected to the regular acceleration process. An analytical solution for the spectrum in the frame of a simplified model that includes particle acceleration at the shock front and adiabatic cooling inside the stellar wind cavity has been derived. It is shown that the acceleration of the solar wind particles at the solar wind terminal shock is capable of providing the total flux, spectrum and radial gradients of the low-energy protons close to one observed in the interplanetary space

    Synthesis, Structure, and Magnetic Properties of an Al2O3/Ge-p/Al2O3/Co Thin-Film System

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    Abstractβ€”Structural and magnetic measurements are made of an Al2O3/Ge-p/Al2O3/Co thin-film system. The structure is synthesized via ion-plasma deposition and can be used as a tunnel heterostructure. The dependences of the magnetic properties of cobalt on the rate of its deposition and the rates of deposition of preceding layers are established

    The role of the semiconductor layer in the exchange-bias film structure of CoNi / Si / FeNi / Si with a spin spring effect

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    CoNi / Si / FeNi / Si structures were synthesized by ion-plasma sputtering. A negative hysteresis loop bias was detected at the thickness of the silicon layer was less than 2 nm and the temperature was less than 100 K. A positive hysteresis loop bias was detected at the thickness of the silicon layer was more than 2 nm and the temperature greater than 100K

    Effect of the Semiconductor Spacer on Positive Exchange Bias in the CoNi/Si/FeNi Three-Layer Structure

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    ВСкст ΡΡ‚Π°Ρ‚ΡŒΠΈ Π½Π΅ публикуСтся Π² ΠΎΡ‚ΠΊΡ€Ρ‹Ρ‚ΠΎΠΌ доступС Π² соотвСтствии с ΠΏΠΎΠ»ΠΈΡ‚ΠΈΠΊΠΎΠΉ ΠΆΡƒΡ€Π½Π°Π»Π°.Films consisting of a hard magnetic ferromagnet CoNi and a soft magnetic ferromagnet FeNi interacting through a nonmagnetic Si semiconductor spacer are experimentally studied. The temperature and field dependences of the magnetic properties of film structures with different silicon thicknesses are examined. It is found that the multilayer structure has the properties inherent in magnetic springs and exhibits positive exchange bias as a function of the silicon thicknes

    The Study of Co-Cu Heterogeneous Alloy Thin Films by NMR Method

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    Π’ Π΄Π°Π½Π½ΠΎΠΉ Ρ€Π°Π±ΠΎΡ‚Π΅ ΠΎΠ±ΡΡƒΠΆΠ΄Π°ΡŽΡ‚ΡΡ Ρ€Π΅Π·ΡƒΠ»ΡŒΡ‚Π°Ρ‚Ρ‹, ΠΏΠΎΠ»ΡƒΡ‡Π΅Π½Π½Ρ‹Π΅ ΠΏΡ€ΠΈ исслСдовании структуры ΠΌΠ°Π³Π½ΠΈΡ‚Π½Ρ‹Ρ… слоСв Π² ΠΌΡƒΠ»ΡŒΡ‚ΠΈΡΠ»ΠΎΠΉΠ½Ρ‹Ρ… ΠΏΠ»Π΅Π½ΠΊΠ°Ρ… Co/Cu со свСрхтонкими ΠΌΠ°Π³Π½ΠΈΡ‚Π½Ρ‹ΠΌΠΈ слоями, ΠΏΡ€ΠΈΠ³ΠΎΡ‚ΠΎΠ²Π»Π΅Π½Π½Ρ‹Ρ… ΠΌΠ΅Ρ‚ΠΎΠ΄ΠΎΠΌ ΠΌΠ°Π³Π½Π΅Ρ‚Ρ€ΠΎΠ½Π½ΠΎΠ³ΠΎ ΠΈΠΎΠ½Π½ΠΎ-ΠΏΠ»Π°Π·ΠΌΠ΅Π½Π½ΠΎΠ³ΠΎ распылСния, ΠΌΠ΅Ρ‚ΠΎΠ΄ΠΎΠΌ ЯМР Π½Π° ядрах 59Co (эффСктивная Ρ‚ΠΎΠ»Ρ‰ΠΈΠ½Π° слоя Co составляла dCo β‰ˆ 3.5 ΠΈ 4.5A). НСсмотря Π½Π° ΡΡ‚ΠΎΠ»ΡŒ ΠΌΠ°Π»Ρ‹Π΅ Π·Π½Π°- чСния эффСктивной Ρ‚ΠΎΠ»Ρ‰ΠΈΠ½Ρ‹ слоСв, Π±Ρ‹Π»ΠΎ ΠΎΠ±Π½Π°Ρ€ΡƒΠΆΠ΅Π½ΠΎ, Ρ‡Ρ‚ΠΎ спСктры ЯМР прСдставляли собой ΡΡƒΠΏΠ΅Ρ€ΠΏΠΎΠ·ΠΈΡ†ΠΈΡŽ Π΄Π²ΡƒΡ… ΠΏΠΈΠΊΠΎΠ² с Ρ†Π΅Π½Ρ‚Ρ€Π°Π»ΡŒΠ½Ρ‹ΠΌΠΈ частотами f1=190βˆ’196ΠœΠ“Ρ† ΠΈ f2=208βˆ’213ΠœΠ“Ρ†, ΠΊΠΎΡ‚ΠΎΡ€Ρ‹Π΅, ΠΎΡ‡Π΅Π²ΠΈΠ΄Π½ΠΎ, соотвСтствовали Π°Ρ‚ΠΎΠΌΠ°ΠΌ ΠΊΠΎΠ±Π°Π»ΡŒΡ‚Π°, ΠΈΠΌΠ΅ΡŽΡ‰ΠΈΠΌ 0 ΠΈ 1 Π°Ρ‚ΠΎΠΌ ΠΌΠ΅Π΄ΠΈ Π² Π±Π»ΠΈΠΆΠ°ΠΉ- шСм ΠΎΠΊΡ€ΡƒΠΆΠ΅Π½ΠΈΠΈ. Π”Π°Π½Π½Ρ‹ΠΉ Ρ„Π°ΠΊΡ‚ ΡƒΠΊΠ°Π·Ρ‹Π²Π°Π΅Ρ‚ Π½Π° Ρ‚ΠΎ, Ρ‡Ρ‚ΠΎ ΠΊΠΎΠ±Π°Π»ΡŒΡ‚ Π³Π»Π°Π²Π½Ρ‹ΠΌ ΠΎΠ±Ρ€Π°Π·ΠΎΠΌ организуСтся Π² ΠΊΡ€ΡƒΠΏΠ½Ρ‹Π΅ кластСры, Π²ΠΊΠ»ΡŽΡ‡Π°ΡŽΡ‰ΠΈΠ΅ большоС число Π°Ρ‚ΠΎΠΌΠΎΠ².In the present work we discuss the structure of magnetic layer in magnetron sputtered Co/Cu multilayers with ultrathin magnetic layers ( effective layer thicknesses dCo β‰ˆ 3.5 and 4.5A) obtained by means of 59Co NMR method. In spite of such a small effective thicknesses of sputtered layers it has been found that the NMR spectra are the superposition of two peaks with central frequencies f1=190-196MHz and f2=208- 213MHz which obviously correspond to Co-atoms which have 0 and 1 Cu-atom in the nearest-neighbor shell indicating that cobalt preferably forms clusters with large number of atoms involved

    Solid-state Synthesis of Cobalt Germanides in Epitaxial Ge/Ξ±-Co(001) and Ge/Ξ²-Co(110) Nanofilms

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    ΠŸΡ€Π΅Π΄ΡΡ‚Π°Π²Π»Π΅Π½Ρ‹ ΡΠΊΡΠΏΠ΅Ρ€ΠΈΠΌΠ΅Π½Ρ‚Π°Π»ΡŒΠ½Ρ‹Π΅ Ρ€Π΅Π·ΡƒΠ»ΡŒΡ‚Π°Ρ‚Ρ‹ исслСдования Ρ‚Π²Ρ‘Ρ€Π΄ΠΎΡ„Π°Π·Π½ΠΎΠ³ΠΎ синтСза Π³Π΅Ρ€ΠΌΠ°Π½ΠΈΠ΄ΠΎΠ² ΠΊΠΎΠ±Π°Π»ΡŒΡ‚Π° Π² ΡΠΏΠΈΡ‚Π°ΠΊΡΠΈΠ°Π»ΡŒΠ½Ρ‹Ρ… Ge/Ξ±-Co(001) ΠΈ Ge/Ξ²-Co(110) Π½Π°Π½ΠΎΠΏΠ»Π΅Π½ΠΊΠ°Ρ…. Показано, Ρ‡Ρ‚ΠΎ для ΠΎΠ±Π΅ΠΈΡ… ΠΏΠΎΠ»ΠΈΠΌΠΎΡ€Ρ„Π½Ρ‹Ρ… ΠΌΠΎΠ΄ΠΈΡ„ΠΈΠΊΠ°Ρ†ΠΈΠΉ ΠΊΠΎΠ±Π°Π»ΡŒΡ‚Π° Ρ„Π°Π·Π° Co5Ge7 формируСтся ΠΏΠ΅Ρ€Π²ΠΎΠΉ ΠΏΡ€ΠΈ Ρ‚Π΅ΠΌΠΏΠ΅Ρ€Π°Ρ‚ΡƒΡ€Π΅ ~275β—¦C. Π‘ ΡƒΠ²Π΅Π»ΠΈΡ‡Π΅Π½ΠΈΠ΅ΠΌ Ρ‚Π΅ΠΌΠΏΠ΅Ρ€Π°Ρ‚ΡƒΡ€Ρ‹ ΠΎΡ‚ΠΆΠΈΠ³Π° ΠΏΡ€ΠΈ Ρ‚Π΅ΠΌΠΏΠ΅Ρ€Π°Ρ‚ΡƒΡ€Π΅ ~300β—¦C образуСтся Ρ„Π°Π·Π° CoGe2, которая Ρ€Π΅Π·ΠΊΠΎ ΡƒΠΌΠ΅Π½ΡŒΡˆΠ°Π΅Ρ‚ элСктричСскоС сопротивлСниС ΠΈ Π½Π°ΠΌΠ°Π³Π½ΠΈΡ‡Π΅Π½Π½ΠΎΡΡ‚ΡŒ ΠΎΠ±Ρ€Π°Π·Ρ†ΠΎΠ². Π Π°Π·Π»ΠΈΡ‡Π½Ρ‹Π΅ ΠΏΠΎΠ»ΠΈΠΌΠΎΡ€Ρ„Π½Ρ‹Π΅ ΠΌΠΎΠ΄ΠΈΡ„ΠΈΠΊΠ°Ρ†ΠΈΠΈ ΠΊΠΎΠ±Π°Π»ΡŒΡ‚Π° Π½Π΅ ΠΈΠ·ΠΌΠ΅Π½ΡΡŽΡ‚ ΠΏΠΎΡΠ»Π΅Π΄ΠΎΠ²Π°Ρ‚Π΅Π»ΡŒΠ½ΠΎΡΡ‚ΡŒ формирования Ρ„Π°Π· ΠΈ ΠΈΡ… Ρ‚Π΅ΠΌΠΏΠ΅Ρ€Π°Ρ‚ΡƒΡ€ инициирования.The experimental results of a study of solid-state synthesis of cobalt germanides in epitaxial Ge/Ξ±-Co(001) and Ge/Ξ²-Co(110) nanofilms are presented. For both polymorphic modifications of cobalt, it is demonstrated that the Co5Ge7 phase occurs at ~275β—¦C. When the annealing temperature increases to ~300β—¦C, the CoGe2 phase forms, which sharply reduces the electric resistance and magnetic characteristics of the samples. The order of the formation of phases and the temperatures at which the phases are formed are not changed based on the polymorphic modification of cobalt
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