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Remotely sensed interplanetary scintillation (IPS) data from the Institute for Space-Earth Environmental Research (ISEE), Japan, allows a determination of solar-wind parameters throughout the inner heliosphere. We show the 3D analysis technique developed for these data sets that forecast plasma velocity, density, and component magnetic fields at Earth, as well at the other inner heliospheric planets and spacecraft. One excellent coronal mass ejection (CME) example that occurred on the 10 March 2022 was viewed not only in the ISEE IPS analyses, but also by the spacecraft near Earth that measured the CME arrival at one AU. Solar Orbiter, that was nearly aligned along the Earth radial at 0.45 AU, also measured the CME in plasma density, velocity, and magnetic field. BepiColombo at 0.42 AU was also aligned with the STEREO A spacecraft, and viewed this CME. The instruments used here from BepiColombo include: 1) the European-Space-Agency Mercury-Planetary-Orbiter magnetic field measurements; 2) the Japan Aerospace Exploration Agency Mio spacecraft Solar Particle Monitor that viewed the CME Forbush decrease, and the Mercury Plasma Experiment/Mercury Electron Analyzer instruments that measured particles and solar-wind density from below the spacecraft protective sunshield covering. This article summarizes the analysis using ISEE, Japan real-time data for these forecasts: it provides a synopsis of the results and confirmation of the CME event morphology after its arrival, and discusses how future IPS analyses can augment these results. [ABSTRACT FROM AUTHOR]

Background and Aim: The risks of peptic ulcer complications increase in association with low-dose aspirin (LDA) use. The endoscopic findings and clinical features of gastroduodenal ulcer have not been thoroughly investigated in patients taking LDA.Method: We classified 1,041 gastroduodenal ulcer patients into three groups [patients taking LDA (group A), patients taking nonaspirin nonsteroidal anti-inflammatory drug (NSAID) (group N), and patients taking neither aspirin nor nonaspirin NSAID (group C)] and 241 bleeding gastroduodenal ulcer patients into three corresponding groups (groups a, n, and c). We investigated the clinical features, endoscopic characteristics, and endoscopic treatment of the hemorrhagic lesion in the gastroduodenal ulcer patients taking LDA and compared them with those of the other groups.Results: The frequency of bleeding events such as hematemesis, melena, and anemia was significantly higher in group A and N than in group C. The percentage of ulcers located in the antrum was higher in group A and N than in group C, and also higher in group a and n than in group c. The percentage of ulcers located in the body, fundus, and cardia was significantly higher in the bleeding patients than in all gastroduodenal ulcer patients. The percentage of cases that required additional endoscopic treatment in group a was higher than in group c. Duration of hospitalization of group a was significantly longer than that of group c.Conclusion: These results indicate that it is very important to prevent LDA-induced gastroduodenal ulcer complications, including bleeding. [ABSTRACT FROM AUTHOR]

The Jupiter Icy Moons Explorer (JUICE) is a science mission led by the European Space Agency, being developed for launch in 2023. The Ganymede Laser Altimeter (GALA) is an instrument onboard JUICE, whose main scientific goals are to understand ice tectonics based on topographic data, the subsurface structure by measuring tidal response, and small-scale roughness and albedo of the surface. In addition, from the perspective of astrobiology, it is imperative to study the subsurface ocean scientifically. The development of GALA has proceeded through an international collaboration between Germany (the lead), Japan, Switzerland, and Spain. Within this framework, the Japanese team (GALA-J) is responsible for developing three receiver modules: the Backend Optics (BEO), the Focal Plane Assembly (FPA), and the Analog Electronics Module (AEM). Like the German team, GALA-J also developed software to simulate the performance of the entire GALA system (performance model). In July 2020, the Proto-Flight Models of BEO, FPA, and AEM were delivered from Japan to Germany. This paper presents an overview of JUICE/GALA and its scientific objectives and describes the instrumentation, mainly focusing on Japan's contribution. [ABSTRACT FROM AUTHOR]