• 한국자기학회지
• /
• 제14권1호
• /
• pp.33-37
• /
• 2004

Cu$_{0.1}$Fe$_{0.9}$Cr$_2$S$_4$에 대하여 x-선 회절기(XRD), 진동 시료 자화율 측정기(VSM), Mossbauer 분광기, 자기저항(Magnetoresistance;MR)법을 이용하여 시료의 결정학적 및 자기적 특성을 연구하였다. 결정구조는 cubic spinel 구조이며, 격자 상수는 a$_{0}$=9.9880 $\AA$이었다. 자기저항(MR)실험 결과 110 K 이하에서는 반도체적 거동을, 100 K 이상에서는 도체적인 거동을 보인다. VSM 실험결과 100 Oe 인가 자장 하에서 zero-field-cooling(ZFC)와 field-cooling(FC) 사이에 커다란 비가역적 첨점 형태가 관측되었다. 5 kOe인가 자장 하에서 포화자화값이 온도 상승과 더불어 110 K 까지 증가되는 현상이 관측되었다. 15 K∼300 K의 온도 범위에 걸쳐서 Mossbauer스펙트럼을 분석한 결과 전기사중극자 분열치가 Neel온도 이하에서 나타나기 시작하여 온도가 하강하면서 점차 증가하고 공명선의 선폭이 비대칭적으로 굵어짐을 볼 수 있었다. 이것은 동적 Jahn-Teller뒤틀림이 일어나고 있는 것으로 해석된다. Fe 이온의 전하상태는 +2이며, 초미세 자기장은 온도가 상승함에 따라 극저온에서 100 K 부근까지 증가하다가 감소하는 현상이 나타났다. 이것은 반대방향의 orbital current field(H$_{L}$)와 Fermi contact field(H$_{C}$) 사이의 상쇄효과로 해석된다.

• 한국진공학회:학술대회논문집
• /
• 한국진공학회 2012년도 제42회 동계 정기 학술대회 초록집
• /
• pp.81-81
• /
• 2012

XMCD (X-ray Magnetic Circular Dichroism)는 원형 편광 X-선의 helicity 방향이 시료의 자화 방향과 평행, 또는 반평행할 때 시료의 색이 바뀌는 현상, 즉 흡수율이 달라지는 현상이다. XMCD측정이 가지는 장점은 첫째, 이 실험이 특정 원소의 흡수선에서 이루어지기 때문에 시료 전체에서 특정 원소에 의한 자기적 성질을 분리해서 측정할 수 있을 뿐만 아니라, 같은 원소라 하더라도 다른 화학적 환경에 있는 원자들의 자기적 성질의 분리가 가능하다는 점이다. 이러한 성질로 인해 XMCD는 다른 원소들로 이루어진 다층 박막(GMR, TMR 등의 자기저항박막 구조물)의 층별 자기적 성질 연구 및 신자성물질의 자기적 성질의 고유성 연구에 많이 이용되었다. XMCD가 가지는 두 번째 장점은 sum rule을 통하여 자기 모멘트의 두 가지 성분인 궤도 모멘트(orbital moment)와 스핀 모멘트(spin moment)의 구별이 가능하다는 점이다. 이러한 장점은 수직자기 메모리 연구 및 스핀과 격자 간의 상호작용이 중요한 역할을 하는 다강체 등의 연구에 많이 이용되어 왔다. XMCD 측정이 또 다른 장점이 될 수 있는 것은 표면에 대단히 민감하다는 점이다. VSM, SQUID 등의 측정방법으로는 시료의 체적이 대단히 작은 수 ${\AA}$ 정도의 초박막에 대해서는 충분한 민감도를 가질 수 없다. 그러나, XMCD의 측정 깊이는 수십 ${\AA}$ 정도로 표면에 민감하기 때문에 이러한 초박막에 대해서도 충분한 민감도를 가질 수 있어서 SMOKE(Surface Magneto-Optical Kerr Effect)와 표면 자성연구에 있어서 독보적인 장치로 이용되어 왔다. 이러한 장점으로 인해 XMCD는 1990년대 이후 분광학적으로 활발히 이용되어 왔을 뿐만 아니라, 대단히 빠르고 신호가 큰 현상이기 때문에 최근 들어서는 자구(magnetic domain) 관찰 등을 목적으로 한 자기 현미경 및 자기현상의 동역학 연구에도 많이 응용되고 있다. 이 강연에서는 이러한 X-선 자기 원형 이색성 현상의 원리 및 실험 방법 등을 설명하겠다. 또한 몇 가지 X-선 자기 원형 이색성을 이용한 최근 몇 가지 연구도 소개하려 한다.

• Bulletin of the Korean Chemical Society
• /
• 제31권6호
• /
• pp.1704-1710
• /
• 2010

The structure of a 2D grid-like copper(II) complex [Cu$(NCO)_2$(pyz)](pyz=pyrazine) (1) consists of 1D chains of Cu-pyz units connected by double end-on (EO) cyanato bridges. Each Cu(II) ion has a distorted octahedral coordination, completed by the four EO cyanato and two pyrazine ligands. Magnetic interactions through EO cyanato and pyrazine bridges in 1 are discussed on the basis of DFT broken-symmetry calculations at the B3LYP level. For model dicopper(II) complexes I (bridged by cyanato) and II (bridged by pyrazine), electronic structure calculations reproduce very well the experimental couplings for the S = 1/2 ferromagnetic and antiferromagnetic exchange-coupled 2D system: the calculated exchange parameters J are +1.25 $cm^{-1}$ and -3.07 $cm^{-1}$ for I and II, respectively. The $\sigma$ orbital interactions between the Cu $x^2-y^2$ magnetic orbitals and the nitrogen lone-pair orbitals of pyrazine are analyzed from the viewpoint of through-bond interaction. The energy splitting of 0.106 eV between two SOMOs indicates that the superexchange interaction should be antiferromagnetic in II. On the other hand, there are no bridging orbitals that efficiently connect the two copper(II) magnetic orbitals in I because the HOMOs of the basal-apical NCO bridge do not play a role in the formation of overlap interaction pathway. The energy separation in the pair of SOMOs of I is calculated to be very small (0.054 eV). This result is consistent with the occurrence of weakly ferromagnetic properties in I.

• 천문학논총
• /
• 제15권spc1호
• /
• pp.93-102
• /
• 2000

We have reviewed the magnetic activity in close binaries. Solar like magnetic activity indicators such as photometric spots, chromo spheric emission, coronal X-ray and radio emission, and flare activity are commonplace in many cool stars with convective envelopes. Using the UV spectra we confirmed the strength of stellar activity increases with more rapid rotation and later spectral types which corresponds to the increasing depth of the star's convective envelope. Apart from very young stellar objects such as T Tauri stars, the stars with the highest levels of activity are close binary systems composed of cool stars, i.e., the chromospherically active binaries such as RS CVn, BY Dra, W UMa and related systems. The IUE low and high dispersion spectra of V711 Tau, VW Cep and SW Lac are used for ultraviolet photometry and for a variation study of chromospheric activity. Evidence of chromospherically activity is indicated by the intensity variation of the Mg II emission line with orbital phase.

• 항공우주기술
• /
• 제2권1호
• /
• pp.54-62
• /
• 2003

우주공간상의 위성체는 아주 미세한 크기에 불과하지만 여러 가지 원인에 의한 외부교란토크를 받는다. 외부교란토크는 위성체의 궤도 운동뿐만 아니라 위성체의 자세에도 큰 영향을 미친다. 저궤도위성의 자세동역학에 작용하는 외부교란토크는 다양하다. 이러한 것들 중 중요한 4가지 원인은 중력경도, 지구자기장, 태양복사압 및 대기저항 등을 들 수 있다. 본 연구에서는 저궤도위성과 같은 저궤도위성에 작용하는 외부교란토크를 상세히 분석하고 저궤도위성 자세동역학에 미치는 외부교란토크의 영향을 상세히 기술한다.

• 천문학회지
• /
• 제44권3호
• /
• pp.97-108
• /
• 2011

The photometric light curves of the W-type W UMa eclipsing contact binary system BB Pegasi have been found to be extremely asymmetric over all the observed 63 years in all wavelengths UBVR. The light curves have been characterized by occultation primary minima. Hence, the morphology of these light curves has been studied in view of these different asymmetric degrees. The system shows a distinct O'Connell effect, as well as depth variation. A 22.96 years of stellar dark spots cycle has been determined for the system. Almost the same cycle (22.78 yr) has been found for the depth variation of MinI and MinII. We also present an analysis of mid-eclipse time measurements of BB Peg. The analysis indicates a period decrement of $5.62{\times}10^{-8}$ day/yr, which can be interpreted in terms of mass transfer at a rate of $-4.38{\times}10^{-8}M_{\odot}$/yr, from the more to the less massive component. The O - C diagram shows a damping sine wave covering two different cycles of 17.0 yr and 12.87 yr with amplitudes equal to 0.0071 and 0.0013 day, respectively. These unequal durations show a non-periodicity which may be explained as a result of magnetic activity cycling variations due to star spots. The obtained characteristics are consistent with similar chromospherically active stars, when applying the Applegate's (1992) mechanism.

• Bulletin of the Korean Chemical Society
• /
• 제31권6호
• /
• pp.1665-1668
• /
• 2010

The spin exchange interactions of $(VO)_2(H_2O){O_3P-(CH_2)_3-PO_3}{\cdot}2H_2O$ were examined by spin dimer analysis based on extended Huckel tight binding method. The strongest spin exchange interaction occurs through the super-superexchange path $J_2$ and the second strongest spin exchange interaction occurs through the superexchange interaction path $J_1$. There are two strongly interacting spin exchange paths in $(VO)_2(H_2O){O_3P-(CH_2)_3-PO_3}{\cdot}2H_2O$. Therefore, magnetic susceptibility curve of $(VO)_2(H_2O){O_3P-(CH_2)_3-PO_3}{\cdot}2H_2O$ can be well reproduced by an alternating onedimensional antiferromagnetic chain model rather than an isolated spin dimer model.

• Current Applied Physics
• /
• 제18권11호
• /
• pp.1190-1195
• /
• 2018

By employing soft X-ray magnetic circular dichroism (XMCD), soft X-ray absorption spectroscopy (XAS), and photoemission spectroscopy (PES), we have investigated the electronic structure of the candidate zero-moment half-metallic $Mn_3Ga$. We have studied the ball-milled and annealed $Mn_3Ga$ powder samples that exhibit nearly zero magnetization. Mn 2p XAS revealed that Mn ions in $Mn_3Ga$ are nearly divalent for both of the Mn ions having the locally octahedral symmetry and those having the locally tetrahedral symmetry. The measured Mn 2p XMCD spectrum of $Mn_3Ga$ is very similar to that of ferrimagnetic $MnFe_2O_4$ having divalent Mn ions. The sum-rule analysis of the Mn 2p XMCD spectrum shows that both the spin and orbital magnetic moments of Mn ions in $Mn_3Ga$ are negligibly small, in agreement with the nearly compensated-ferrimagnetic ground state of $Mn_3Ga$. The valence-band PES spectrum of $Mn_3Ga$ agrees well with the calculated density of states, supporting the half-metallic electronic structure of $Mn_3Ga$.

• Investigative Magnetic Resonance Imaging
• /
• 제26권2호
• /
• pp.96-103
• /
• 2022

Purpose: The survival of organisms critically depends on avoidance responses to life-threatening stimuli. Information about dangerous situations needs to be remembered to produce defensive behavior. To investigate underlying brain regions to process information of danger, manganese-enhanced MRI (MEMRI) was used in olfactory fear-conditioned rats. Materials and Methods: Fear conditioning was conducted in male Sprague-Dawley rats. The animals received nasal injections of manganese chloride solution to monitor brain activation for olfactory information processing. Twenty-four hours after manganese injection, rats were exposed to electric foot shocks with odor cue for one hour. Control rats were exposed to the same odor cue without foot shocks. Forty-eight hours after the conditioning, rats were anesthetized and their brains were scanned with 9.4T MRI. Acquired images were processed and statistical analyses were performed using AFNI. Results: Manganese injection enhanced brain areas involved in olfactory information pathways in T1 weighted images. Rats that received foot shocks showed higher brain activation in the central nucleus of the amygdala, septum, primary motor cortex, and preoptic area. In contrast, control rats displayed greater signals in the orbital cortex and nucleus accumbens. Conclusion: Nasal delivery of manganese solution enhanced olfactory signal pathways in rats. Odor cue paired with foot shocks activated amygdala, the central brain region in fear, and related brain circuits. Use of MEMRI in fear conditioning provides a reliable monitoring technique of brain activation for fear learning.

• Archives of Plastic Surgery
• /
• 제50권1호
• /
• pp.54-58
• /
• 2023

Patients with Crouzon syndrome have increased risks of cerebrospinal fluid rhinorrhea and meningoencephalocele after LeFort III osteotomy. We report a rare case of meningoencephalocele following LeFort III midface advancement in a patient with Crouzon syndrome. Over 10 years since it was incidentally found during transnasal endoscopic orbital decompression, the untreated meningoencephalocele eventually led to intermittent clear nasal discharge, frontal headache, and seizure. Computed tomography and magnetic resonance imaging demonstrated meningoencephalocele in the left frontal-ethmoid-maxillary sinus through a focal defect of the anterior cranial base. Through bifrontal craniotomy, the meningoencephalocele was removed and the anterior cranial base was reconstructed with a pericranial flap and split calvarial bone graft. Secondary frontal advancement was concurrently performed to relieve suspicious increased intracranial pressure, limit visual deterioration, and improve the forehead shape. Surgeons should be aware that patients with Crouzon syndrome have the potential for an unrecognized dural injury during LeFort III osteotomy due to anatomical differences such as inferior displacement and thinning of the anterior cranial base.