A comparison of dust concentration with high resolution analysis and visible strata in the Holocene and Last Glacial Maximum periods from the Dome Fuji ice core, East Antarctica

第3回極域科学シンポジウム　横断セッション「海・陸・氷床から探る後期新生代の南極寒冷圏環境変動」11月26日（月）、27日（火） ２階ラウン

Climatic and atmospheric histories over the past 700,000 years from the Dome Fuji deep ice core, Antarctica

第3回極域科学シンポジウム　横断セッション「海・陸・氷床から探る後期新生代の南極寒冷圏環境変動」11月26日（月） 国立国語研究所 ２階講

Ice Core Records of Antarctic Warming Events in the Last Glacial Period

第3回極域科学シンポジウム　横断セッション「海・陸・氷床から探る後期新生代の南極寒冷圏環境変動」11月26日（月） 国立国語研究所 ２階講

General tendencies of stable isotopes and major chemical constituents of the Dome Fuji deep ice core (scientific paper)

Stable isotope compositions of water and major chemical constituents of the Dome Fuji ice core are analyzed and the data sets over the entire depth of the 2503-m core are presented in appropriate time resolution as consecutive series of average value in definite terms. These results based on the first stage analyses allow a temporal climatic dividing of the three glacial-interglacial cycles present in the records. A Comparison of the climatic and environmental characteristics of these climate stages is presented

Optical and Near-Infrared Photometry of Nova V2362 Cyg : Rebrightening Event and Dust Formation

We present optical and near-infrared (NIR) photometry of a classical nova, V2362 Cyg (= Nova Cygni 2006). V2362 Cyg experienced a peculiar rebrightening with a long duration from 100 to 240 d after the maximum of the nova. Our multicolor observation indicates an emergence of a pseudophotosphere with an effective temperature of 9000 K at the rebrightening maximum. After the rebrightening maximum, the object showed a slow fading homogeneously in all of the used bands for one week. This implies that the fading just after the rebrightening maximum ( less or equal 1 week ) was caused by a slowly shrinking pseudophotosphere. Then, the NIR flux drastically increased, while the optical flux steeply declined. The optical and NIR flux was consistent with blackbody radiation with a temperature of 1500 K during this NIR rising phase. These facts are likely to be explained by dust formation in the nova ejecta. Assuming an optically thin case, we estimate the dust mass of 10^(-8) -- 10^(-10) M_solar, which is less than those in typical dust-forming novae. These results support the senario that a second, long-lasting outflow, which caused the rebrightening, interacted with a fraction of the initial outflow and formed dust grains.Comment: 6 pages, 4 figures, 2010, PASJ, 62, 1103--1108, in pres

Development of ethnographic digital collections

Περιέχει το πλήρες κείμενοΟι λαογραφικές συλλογές αποτελούν πολύτιμη πηγή μελέτης, εξερεύνησης και αξιολόγησης των εθνικών στερεοτύπων των διαφόρων διαμερισμάτων μιας χώρας, δεδομένου ότι στις συλλογές είναι καταχωρημένα ανόθευτα και πηγαία τα εγχώρια εθνοχαρακτηριστικά τους. Κατά κύριο λόγο η λαογραφία αναφέρεται στους μύθους, τα τραγούδια, τη μουσική, τα έθιμα, τη χειροτεχνία, την ενδυμασία, την αρχιτεκτονική και την προφορική παράδοση μιας κοινότητας. Η ιδιαιτερότητα και η ποικιλία ενός τομέα όπως της λαογραφίας δικαιολογεί απόλυτα την ύπαρξη συλλογών και υπο-συλλογών σύνθετης δομής και σημασιολογίας, όπως αυτές που αναφέρουμε παραπάνω. Επομένως η ανάπτυξη ψηφιακών συλλογών απαιτεί τη διατήρηση των στοιχείων που χρειάζονται για: (α) την περιγραφή του περιεχομένου της κάθε συλλογής χωριστά και (β) τη σωστή απεικόνιση της δομής των αντικειμένων στο εσωτερικό αυτής. Στόχος της εργασίας αυτής είναι η παρουσίαση μιας μεθοδολογίας για την ανάπτυξη ενός περιγραφικού μοντέλου μεταδεδομένων για λαογραφικές συλλογές. Το μοντέλο θα αποτελέσει βασικό εργαλείο για την περιγραφή του ψηφιοποιημένου λαογραφικού υλικού, την πρόσβαση σε αυτό από κατανεμημένους χρήστες και φυσικά την επικοινωνία του με άλλα συστήματα. Επιπλέον θα συμβάλλει στη διασύνδεση σύνθετων συλλογών και των αντικειμένων που περιλαμβάνουν είτε σημασιολογικά, είτε χρονικά, είτε θεματικά είτε με οποιονδήποτε άλλο τρόπο απαιτεί η φύση των συλλογών και οι ανάγκες των χρηστών

The 2006 November outburst of EG Aquarii: the SU UMa nature revealed

We report time-resolved CCD photometry of the cataclysmic variable EG Aquarii during the 2006 November outburst During the outburst, superhumps were unambiguously detected with a mean period of 0.078828(6) days, firstly classifying the object as an SU UMa-type dwarf nova. It also turned out that the outburst contained a precursor. At the end of the precursor, immature profiles of humps were observed. By a phase analysis of these humps, we interpreted the features as superhumps. This is the second example that the superhumps were shown during a precursor. Near the maximum stage of the outburst, we discovered an abrupt shift of the superhump period by ${\sim}$ 0.002 days. After the supermaximum, the superhump period decreased at the rate of $\dot{P}/P$=$-8.2{\times}10^{-5}$, which is typical for SU UMa-type dwarf novae. Although the outburst light curve was characteristic of SU UMa-type dwarf novae, long-term monitoring of the variable shows no outbursts over the past decade. We note on the basic properties of long period and inactive SU UMa-type dwarf novae.Comment: 9 pages, 7 figures, accepted for PAS

Multiple transcripts of Ca 2ϩ channel ␣ 1 -subunits and a novel spliced variant of the ␣ 1C -subunit in rat ductus arteriosus

3 H]thymidine incorporation, suggesting that L-and T-type Ca 2ϩ channels are involved in smooth muscle cell proliferation in the DA. Third, we found that a novel alternatively spliced variant of the ␣ 1C-isoform was highly expressed in the neointimal cushion of the DA, where proliferating and migrating smooth muscle cells are abundant. The basic channel properties of the spliced variant did not differ from those of the conventional ␣1C-subunit. We conclude that multiple VDCC subunits were identified in the DA, and, in particular, ␣ 1C-and ␣1G-subunits were predominant in the DA. A novel spliced variant of the ␣1C-subunit gene may play a distinct role in neointimal cushion formation in the DA. alternative spliced; development; gene expression; fetal circulation THE DUCTUS ARTERIOSUS (DA) is a fetal arterial connection between the pulmonary artery and the descending aorta. After birth, the DA closes immediately, in accordance with its smooth muscle contraction. An increase in oxygen tension and a dramatic decline in circulating prostaglandins are the most important triggers of DA contraction (5). Generally, vascular smooth muscle contraction is induced by Ca 2ϩ / calmodulin-dependent phosphorylation of the regulatory myosin light chain, which is mediated by an increase in intracellular Ca 2ϩ . Ca 2ϩ influx through voltage-dependent Ca 2ϩ channels (VDCCs) and Ca 2ϩ release from intracellular stores are major sources of this increase (8, 26). Thus VDCCs must play an important role in vascular myogenic reactivity and tone of the DA. VDCCs are classified, according to their distinct electrophysiological and pharmacological properties, into low (Ttype) and high (L-, N-, P-, Q-, and R-type) VDCCs (20, In addition to their role in determining contractile state, a growing body of evidence has demonstrated that VDCCs play an important role in regulating differentiation and remodeling of vascular smooth muscle cells (SMCs) (14, In the present study, we identified multiple VDCC subunits in the DA by semiquantitative and quantitative RT-PCR and immunodetection. In particular, ␣ 1C -and ␣ 1G -subunits were predominant in the DA. Furthermore, we will demonstrate the identification of a novel spliced variant of the ␣ 1C -subunit gene that may play a role in neointimal cushion formation of the DA