Chapter 4D Ray-Space and Ultra-Wide Area FTV

Ultra-wide area FTV is an FTV with very wide viewing zone where motion parallax is realized. 4D orthogonal ray-space is analyzed and applied to ultra-wide area FTV. Ray-space of “a group of rays through one point” is derived in 4D orthogonal ray-space. It is extended to obtain ray-space captured by linear arrangement cameras. View generation of ultra-wide area FTV needs rays that are not captured by real cameras. These rays are synthesized by interpolating the captured ray-space so that the intersections of the captured ray-space and the ray-space of rays emitted from a light source have the same color

A Cost Information System as Applied to a Solar Cell Development Project

As part of national R&D program of new energy resources named Sunshine Project, R&D efforts have been made on solar photovoltaic conversion system since 1974. It is the point for practical use of the conversion system, to establish the production process of low-cost silicon solar cells. In this paper we present a Cost Information System which has been developed to evaluate the production cost of solar cells for several conceptual production lines designed in the New Energy Development Organization, Japan.To be presented at IFORS \u278

A Comprehensive Study of Repetitive Transcranial Magnetic Stimulation in Parkinson's Disease

The clinical benefits of repetitive transcranial magnetic stimulation (rTMS) for Parkinson's disease (PD) remain controversial. We performed a comprehensive study to examine whether rTMS is a safe and effective treatment for PD. Twelve PD patients received rTMS once a week. The crossover study design consisted of 4-week sham rTMS followed by 4-week real rTMS. The Unified Parkinson's Disease Rating Scale (UPDRS), Modified Hoehn and Yahr Stage, Schwab and England ADL Scale, Actigraph, Mini-Mental State Examination, Hamilton Depression Scale, Wechsler Adult Intelligence Scale-revised, and cerebral blood flow (CBF) and cerebrospinal fluid (CSF) examinations were used to evaluate the rTMS effects. Under both drug-on and drug-off conditions, the real rTMS improved the UPDRS scores significantly, while the sham rTMS did not. There were no significant changes in the results of the neuropsychological tests, CBF and CSF. rTMS seems to be a safe and effective therapeutic option for PD patients, especially in a wearing-off state

Evidence for Spin–Orbit Alignment in the TRAPPIST-1 System

In an effort to measure the Rossiter–McLaughlin effect for the TRAPPIST-1 system, we performed high-resolution spectroscopy during transits of planets e, f, and b. The spectra were obtained with the InfraRed Doppler spectrograph on the Subaru 8.2 m telescope, and were supplemented with simultaneous photometry obtained with a 1 m telescope of the Las Cumbres Observatory Global Telescope. By analyzing the anomalous radial velocities, we found the projected stellar obliquity to be λ = 1 ± 28° under the assumption that the three planets have coplanar orbits, although we caution that the radial-velocity data show correlated noise of unknown origin. We also sought evidence for the expected deformations of the stellar absorption lines, and thereby detected the "Doppler shadow" of planet b with a false-alarm probability of 1.7%. The joint analysis of the observed residual cross-correlation map including the three transits gave λ = 19_(-15)^(+13)°. These results indicate that the the TRAPPIST-1 star is not strongly misaligned with the common orbital plane of the planets, although further observations are encouraged to verify this conclusion

Planet(esimal)s Around Stars with TESS (PAST) III: A Search for Triplet He I in the Atmospheres of Two 200 Myr-old Planets

We report a search for excess absorption in the 1083.2 nm line of ortho (triplet) helium during transits of TOI-1807b and TOI-2076b, 1.25 and 2.5R$_{\rm Earth}$ planets on 0.55- and 10.4-day orbits around nearby $\sim$200~Myr-old K dwarf stars. We limit the equivalent width of any transit-associated absorption to $<$4 and $<$8 mA, respectively. We limit the escape of solar-composition atmospheres from TOI-1807b and TOI-2076b to $\lesssim$1 and $\lesssim$0.1M$_{\rm Earth}$ Gyr$^{-1}$, respectively, depending on wind temperature. The absence of a H/He signature for TOI-1807b is consistent with a measurement of mass indicating a rocky body and the prediction by a hydrodynamic model that any H-dominated atmosphere would be unstable and already have been lost. Differential spectra obtained during the transit of TOI-2076b contain a He I-like feature, but this closely resembles the stellar line and extends beyond the transit interval. Until additional transits are observed, we suspect this to be the result of variation in the stellar He I line produced by rotation of active regions and/or flaring on the young, active host star. Non-detection of escape could mean that TOI-2076b is more massive than expected, the star is less EUV-luminous, the models overestimate escape, or the planet has a H/He-poor atmosphere that is primarily molecules such as H$_2$O. Photochemical models of planetary winds predict a semi-major axis at which triplet He I observations are most sensitive to mass loss: TOI-2076b orbits near this optimum. Future surveys could use a distance criterion to increase the yield of detections.Comment: Accepted to MNRA

Limits on the Spin-Orbit Angle and Atmospheric Escape for the 22 Myr-old Planet AU Mic b

We obtained spectra of the pre-main sequence star AU Microscopii during a transit of its Neptune-sized planet to investigate its orbit and atmosphere. We used the high-dispersion near-infrared spectrograph IRD on the Subaru telescope to detect the Doppler "shadow" from the planet and constrain the projected stellar obliquity. Modeling of the observed planetary Doppler shadow suggests a spin-orbit alignment of the system ($\lambda=-4.7_{-6.4}^{+6.8}$ degrees), but additional observations are needed to confirm this finding. We use both the IRD data and spectra obtained with NIRSPEC on Keck-II to search for absorption in the 1083 nm line of metastable triplet He I by the planet's atmosphere and place an upper limit for the equivalent width of 3.7 m\AA at 99 $\%$ confidence. With this limit and a Parker wind model we constrain the escape rate from the atmosphere to $<0.15-0.45\, M_{\oplus}$ Gyr$^{-1}$, comparable to the rates predicted by an XUV energy-limited escape calculation and hydrodynamic models, but refinement of the planet mass is needed for rigorous tests.Comment: 10 pages, 5 figures, accepted for publication in ApJ Letter

Cross-talk between TLR3 and TNF-α or IFN-γ Signaling in Induction of CXCL8/IL-8 and CXCL10/IP-10 Expression in Airway Epithelial Cells

CXCL8/IL-8 is a chemoattractant for neutrophils and mast cells, and regulates inflammatory cell recruitment in allergy, infection, and other neutrophil-related diseases. Interferon (IFN) -γ-inducible protein 10 (CXCL10/IP-10) is a chemokine that attracts mononuclear cells, Th1 cells, and natural killer cells. We investigated the levels of CXCL8/IL-8 and CXCL10/IP-10 expression by airway epithelial cells after exposure to the inflammatory cytokines tumor necrosis factor (TNF) -α and IFN-γ, and to poly I:C, a synthetic analog of double-stranded RNA that is a ligand of Toll-like receptor 3 (TLR3). Poly I:C, TNF-α, IFN-γ, and combinations of poly I:C with TNF-α or IFN-γ were used to stimulate the airway epithelial cell line BEAS-2B. Following stimulation, we determined CXCL8/IL-8 and CXCL10/IP-10 mRNA levels by real-time PCR and protein levels by ELISA. Poly I:C treatment upregulated mRNA and protein expression for both CXCL8/IL-8 and CXCL10/IP-10. The addition of TNF-α, but not IFN-γ, to poly I:C further increased the expression of CXCL8/IL-8 mRNA and protein. The addition of either TNF-α or IFN-γ to the poly I:C treatment further increased CXCL10/IP-10 mRNA and protein expression. Cross-talk between TLR3 signaling and inflammatory cytokines regulates the expression of CXCL8/IL-8 and CXCL10/IP-10 in airway epithelial cells. From our results, TNF-α and IFN-γ produce different effects on TLR3 signaling