Scintigraphic studies on the etiology of Ampulla Cardiomyopathy

SummaryBackgroundAlthough there are many reports on Ampulla Cardiomyopathy, its etiologic mechanisms are not well known.AimEtiology of Ampulla Cardiomyopathy was investigated by myocardial scintigraphy with various nuclear tracers.Subjects and methodsIn nine patients with Ampulla Cardiomyopathy, myocardial scintigraphy was performed at acute, subacute and chronic phases. Total defect score (TDS) of tallium-201 (Tl) or technetrium-99m sestamibi (MIBI) myocardial perfusion and iodine-123-beta-methyl-p-iodophenyl penta-decanoic acid (BMIPP) scintigraphies was calculated. Cardio-mediastinal ratio (H/M) and washout rate (WR) of early and delayed images of iodine-123-meta-iodobenzylguanidine (MIBG) scintigraphy were also calculated. The patients in whom TDS of myocardial perfusion scintigraphy at acute phase was 0, were classified into group N (n=5) and those with TDS≥1 into group D (n=4).ResultsTDS of BMIPP at acute, subacute and chronic phases was higher in D than in N; 28.8±10.3 vs. 7.2±4.7 (p=0.0039), 15.5±2.1 vs. 1.0±0.8 (p<0.0001) and 2.7±1.2 vs. 0 (p=0.05), respectively. WR of MIBG at acute phase was also higher in D (50.3±5.7% vs. 36.6±10.5%, p=0.05). H/M (dH/M) on the delayed images and WR at chronic phase were not different between the two groups. H/M (eH/M) on the early images was lower in D. Blood noradrenaline (ng/ml) at acute phase was higher in D than in N (1.21±0.55 vs. 0.45±0.33, p<0.05). Left ventricular ejection fraction (LVEF) was decreased in both at acute phase but it was lower in D than in N (48.1±3.7% vs. 69.9±9.7%, p<0.05) at subacute phase.ConclusionThese findings suggest that the etiology of Ampulla Cardiomyopathy is neurologically stunned myocardium induced by coronary microcirculatory disorder.Due to the significant amount of time that was necessary for normalization of wall motion in the D group, myocardial scintigraphy is believed to be also useful in assessment of severity

Near-IR imaging polarimetry toward a bright-rimmed cloud: Magnetic field in SFO 74

We have made near-infrared (JHKs) imaging polarimetry of a bright-rimmed cloud (SFO 74). The polarization vector maps clearly show that the magnetic field in the layer just behind the bright rim is running along the rim, quite different from its ambient magnetic field. The direction of the magnetic field just behind the tip rim is almost perpendicular to that of the incident UV radiation, and the magnetic field configuration appears to be symmetric as a whole with respect to the cloud symmetry axis. We estimated the column and number densities in the two regions (just inside and far inside the tip rim) and then derived the magnetic field strength, applying the Chandrasekhar-Fermi method. The estimated magnetic field strength just inside the tip rim, ~90 ?G, is stronger than that far inside, ~30 ?G. This suggests that the magnetic field strength just inside the tip rim is enhanced by the UV-radiation-induced shock. The shock increases the density within the top layer around the tip and thus increases the strength of the magnetic field. The magnetic pressure seems to be comparable to the turbulent one just inside the tip rim, implying a significant contribution of the magnetic field to the total internal pressure. The mass-to-flux ratio was estimated to be close to the critical value just inside the tip rim. We speculate that the flat-topped bright rim of SFO 74 could be formed by the magnetic field effect

X-Ray Analysis Literatures 2010

本総説は，2010年に学術雑誌に掲載されたX線分析関連の論文において，注目すべき論文を厳選し紹介する．調査した学術雑誌は19件（和雑誌2件含む）であり，X線分析の発展に寄与しているものを対象としているが，分析化学の分野だけでなく，分光学や物理学の分野も網羅している．各雑誌に関して，X 線分析手法や測定された試料の傾向，分析技術や要素開発に関するトピックスの他に，特筆すべき論文には論評も記している．日本工業規格（JIS）におけるX線分析関連の規格の制定や改訂についてまとめている．X線関連メーカーのウェブサイトを紹介し，掲載している技術レポートの情報も得られる．　In this article, the interesting X-ray analysis-related literatures, which are published on academic journals during the year 2010, are summarized. The number of the researched journals is 19, including two Japanese journals, which contribute the advance of the X-ray analysis in the field not only of analytical chemistry but also of spectroscopy and physics. In every journal, the trend of the X-ray analysis methods and of the measured specimens, the topics of analytical technique and of the developed components of the X-ray analysis apparatus, and the comments for the nortable articles are mentioned. The constitution and revision of standards of X-ray analysis on Japanease Industrial Standard (JIS) are shown. The websites of the company related with X-ray tools or X-ray apparatus are also shown, and the information on technical reports is available

Near-Infrared Imaging Polarimetry of the Serpens Cloud Core: Magnetic Field Structure, Outflows, and Inflows in A Cluster Forming Clump

We made deep NIR imaging polarimetry toward the Serpens cloud core. The polarization vector maps enable us to newly detect 24 small IR reflection nebulae with YSOs. Polarization measurements of NIR point sources indicate an hourglass-shaped magnetic field, of which symmetry axis is nearly perpendicular to the elongation of the C18O (J=1-0) or submillimeter continuum emission. The bright part of C18O (J=1-0), submillimeter continuum cores as well as many class 0/I objects are located just toward the constriction region of the hourglass-shaped magnetic field. Applying the CF method, the magnetic field strength was estimated to be ~100 muG, suggesting that the ambient region of the Serpens cloud core is moderately magnetically supercritical. These suggest that the Serpens cloud core first contracted along the magnetic field to be an elongated cloud, which is perpendicular to the magnetic field, and that then the central part contracted cross the magnetic field due to the high density in the central region of the cloud core, where star formation is actively continuing. Comparison of this magnetic field with the previous observations of molecular gas and large-scale outflows suggests a possibility that the cloud dynamics is controlled by the magnetic field, protostellar outflows and gravitational inflows. This appears to be in good agreement with the outflow-driven turbulence model and implies the importance of the magnetic field to continuous star formation in the center region of the cluster forming region.Comment: 36 pages, 11 figures, 2 tables, accepted for publication in the Astrophysical Journa

Bilateral Renal Cell Carcinoma and its Treatment

A report is presented on two cases of bilateral renal cell carcinoma together with a review of the literature. Bilateral renal cell carcinoma is rare and there is much controversy concerning its treatment. Our current experience supports conservative therapy for bilateral renal cell carcinoma

Detection of p53 Gene Mutations and Their Protein Overexpression in Fine-needle Biopsy Specimens with False-negative Diagnoses in Breast Cancer

To achieve a more accurate diagnosis in the first aspiration biopsy from breast tumor, p53 gene mutations were detected by PCR-SSCP analysis in aspira-tion biopsy specimens taken from 26 patients with breast tumors. Of 26 aspirat-ed cell specimens from breast tumors that were all initially diagnosed as being cytologically benign, 2 point mutations of the p53 gene were detected and were subsequently proved to be cancer cells. Further, the p53 protein expression was also examined in the initial aspirated specimens and in the resected tumors that were rediagnosed as being malignant as a result of the second biopsy. Conse-quently, these p53 gene mutations did not appear to correlate with their protein overexpression in the aspiration biopsy specimens (all cases were negative), how-ever, the specimens from 2 resected tumors that showed p53 gene mutations were positive. In addition, a positive ER level and DNA aneuploidy status were also found only in these two p53 gene mutation cases. Therefore, detection of p53 mutations in aspiration biopsy specimens may prove to be a useful method for detecting breast cancers

Exploring deuterium beam operation and the behavior of the co-extracted electron current in a negative-ion-based neutral beam injector

The achievements of the deuterium beam operation of a negative-ion-based neutral beam injector (N-NBI) in the large helical device (LHD) are reported. In beam operation in LHD-NBIs, both hydrogen (H) and deuterium (D) neutral beams were generated by changing the operation gas using the same accelerator. The maximum accelerated deuterium negative-ion current () reaches 46.2 A from two beam sources with the averaged current density being 190 A m−2 for 2 s, and the extracted electron to accelerated ion current ratio () increases to 0.39 using 5.6 V high bias voltage in the first deuterium operation in 2017. An increase of electron density in the vicinity of the plasma grid (PG) surface, which is considered the main reason for the increase of co-extracted electrons in a beam, is confirmed by the half-size research negative-ion source in the neutral beam test stand at the National Institute for Fusion Science (NIFS). The deuterium negative-ion density is also larger than the hydrogen negative-ion density in the vicinity of the PG surface using the same discharge conditions. In the latest experimental campaign in 2018, increases to 55.4 A with the averaged current density being 233 A m−2 for 1.5 s using the shot extraction gap length. The low of 0.31 can be maintained by using high discharge power. The various parameters mentioned above are defined in detail below