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事なかれ主義のニック・キャラウェイ : 『グレート・ギャツビー』の主人公兼語り手に関する一考察
No full textArticle信州大学教育学部研究論集 12:107-114(2018)departmental bulletin pape
下関唐戸地区における観光地開発の周辺地域・住民への影響
No full textArticle国立大学法人信州大学 教育学部自然地理学研究室『2016年度地理学野外実習報告書Ⅸ 下関』(2018)p.36-44research repor
南風泊水産加工団地及び『下関ふく』ブランド発信の課題
No full textArticle国立大学法人信州大学 教育学部自然地理学研究室『2016年度地理学野外実習報告書Ⅸ 下関』(2018)p.64-72research repor
知的障害の理解についての新しい方向性（1） : 知的障害概念に影響を及ぼした福祉制度を中心に
No full textArticle信州大学教育学部研究論集 12:187-209(2018)departmental bulletin pape
長野県大町市，大峰帯中部地域の下部更新統の層序と大規模火砕流堆積物の再堆積性砕屑物
No full textThe Omine Belt is located in the western margin of the Northern Fossa Magna. Western limit of the Omine Belt is the Itoigawa-Sizuoka Tectonic Line and the eastern limit is the Otari-Nakayama Fault. In the central Omine Belt, Omine Group is interbedded with six volcaniclastic beds from lower to upper stratigraphic following order, Nyunomi Formation, Sonehara Formation,Takagariyama TuffI Member,Takagariyama TuffII Member,Reishoji TuffMember and Omine Formation. After Takagariyama Tuff I Member (1.76 Ma) and Takagariyama Tuff II Member (1.75 Ma) emplaced, the denudation and resedimentation systems have been developed.The systems reflect solidification degree of these pyroclastic flow deposits. Nyukawa Pyroclastic Flow Deposit (Takagariyama TuffI Member)is mostly composed of welded tuff, and Ebisutoge Pyroclastic Deposit (Takagariyama TuffII Member) is composed of nonwelded tuff. Clastic materials derived from Ebisutoge Pyroclastic Deposit are found only at a slightly upper level of the Takagariyama TuffII Member.On the other hand, clastic materials derived from Nyukawa Pyroclastic Flow Deposit are found many horizons in upper beds of the Takagariyama TuffI Member and II.It might be stated that resedimentaion system for the Nyukawa Pyroclastic Flow Deposit continued for a long time because of its welding properties and denudation difficulty.ArticleJournal of the Faculty of Science Shinshu University 47 : 9-24(2018)departmental bulletin pape
New determinant expressions of multi-indexed orthogonal polynomials in discrete quantum mechanics
No full textMulti-indexed orthogonal polynomials (the Meixner, little q-Jacobi (Laguerre), (q-) Racah, Wilson, and Askey-Wilson types) satisfying second-order difference equations were constructed in discrete quantum mechanics. They are polynomials in sinusoidal coordinates eta(x) (x is the coordinate of the quantum system) and are expressed in terms of Casorati determinants whose matrix elements are functions of x at various points. By using shape-invariance properties, we derive various equivalent determinant expressions, especially those whose matrix elements are functions of the same point x. Except for the (q-) Racah case, they can be expressed in terms of eta only, without explicit x-dependence.ArticlePROGRESS OF THEORETICAL AND EXPERIMENTAL PHYSICS. 5:053A01 (2017)journal articl
AVERAGE SPATIAL DISTRIBUTION OF COSMIC RAYS BEHIND THE INTERPLANETARY SHOCK-GLOBAL MUON DETECTOR NETWORK OBSERVATIONS
No full textWe analyze the galactic cosmic ray (GCR) density and its spatial gradient in Forbush Decreases (FDs) observed with the Global Muon Detector Network (GMDN) and neutron monitors (NMs). By superposing the GCR density and density gradient observed in FDs following 45 interplanetary shocks (IP-shocks), each associated with an identified eruption on the Sun, we infer the average spatial distribution of GCRs behind IP-shocks. We find two distinct modulations of GCR density in FDs, one in the magnetic sheath and the other in the coronal mass ejection (CME) behind the sheath. The density modulation in the sheath is dominant in the western flank of the shock, while the modulation in the CME ejecta stands out in the eastern flank. This east-west asymmetry is more prominent in GMDN data responding to similar to 60 GV GCRs than in NM data responding to similar to 10 GV GCRs, because of the softer rigidity spectrum of the modulation in the CME ejecta than in the sheath. The geocentric solar ecliptic-y component of the density gradient, G(y), shows a negative (positive) enhancement in FDs caused by the eastern (western) eruptions, while G(z) shows a negative (positive) enhancement in FDs caused by the northern (southern) eruptions. This implies that the GCR density minimum is located behind the central flank of IP-shocks and propagating radially outward from the location of the solar eruption. We also confirmed that the average Gz changes its sign above and below the heliospheric current sheet, in accord with the prediction of the drift model for the large-scale GCR transport in the heliosphere.ArticleASTROPHYSICAL JOURNAL. 825(2):100 (2016)journal articl
