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|Date||Name||Title||Abstract||File||4/10||K.Shibata||Solar Physics in Future 2017||pptx||4/17||S.Takeshige||I will introduce a paper, titled 'Spatial Growth of Current-driven Instability in Relativistic Rotating Jets and the Search for Magnetic Reconnection', Singh et al. 2016. http://adsabs.harvard.edu/abs/2016ApJ...824...48S||4/17||A.Asai||A 3-dimensional view of a filament eruption and CMEs associated with the 2011 March 8 Solar Flare||pptx||4/24||K.Ichimoto||I will give an overview of the Solar observation projects in 2017.as usual at the beginning of the fiscal year.|
- Solar-C status
- What we do at Hida?
|5/1||Y.Notsu||"A solar-like magnetic cycle on the mature K-dwarf 61 Cygni A (HD 201091)"||
In the short talk on next Monday, I will introduce the following paper.
"A solar-like magnetic cycle on the mature K-dwarf 61 Cygni A (HD 201091)"
Boro Saikia et al. 2016, A&A, 594, 29
This paper reports the first detection of a cool star, apart from the Sun, where the magnetic cycle (polarity reversal etc) is in phase with its chromospheric cycle (Ca II intensity changes), on the basis of 8-year spectropolarimetric monitoring observations.
|5/1||S.Ueno||In the tomorrow's solar seminar, I plan to talk about the following two things. 1) Introduction of the theme of Mr. Kaiho's DST-observation in last week: According to Ishii-san, Director Shibata requested that contents of recent DST observations should be introduced in the solar seminar. So, I received Mr. Kaiho's presentation file for the seminar on Apr-25. I will briefly introduce it again for people who could not attend his seminar. 2) Report of conference about Chinese future ground-based solar telescopes: When we visited Fuxian Solar Observatory in last December, I attended the conference about Chinese future solar telescopes in Kunming. In this conference, the Chinese Giant Solar Telescope (CGST) and 2.5 m solar and stellar telescope (ISMART) were mainly treated. I will report outline of this conference.||5/8||K.Hirose||5/8||A.Kawamura||Statistical Characteristics of Solar cycle 23 & Newly Found Aurora Picture (of Solar Cycle 19)||5/15||U.Kou||Statistical Characteristics of Solar cycle 23 & Newly Found Aurora Picture (of Solar Cycle 19)||Today I will have a brief introduce of Title: Magnetic Field and Plasma Diagnostics from Coordiated Prominence Observations Author: B. Schmieder et. al Link: http://adsabs.harvard.edu/abs/2016ASPC..504..119S Abstract: This paper studies the temperature, density and flow velocities of the prominence from a statistical point of view by combining the measurements from THEMIS, IRIS, HINODE/EIS and Meudon Solar Tower. They are aiming to answer the following question: 1. what is the general direction of the magnetic field in prominences? 2. are prominences in a weak environment field dominated by gas pressure? 3. if there are substantial velocities to maintain vertical rotation structures, as has been suggested for tornado-like prominences.||5/15||S.Nagata||5/22||5/29||K.Namekata||5/29||S.Ninomiya||6/5||D.Cabezas||In tomorrow's seminar as a short talk, I will introduce the paper by Kleint et al. (2015) entitled as: "The fast filament eruption leading to the X-flare on 2014 March 29" http://adsabs.harvard.edu/abs/2015ApJ...806....9K||6/5||T.Anan||Which spectral line is good for future Japanese space missions?||I would like to talk about development of simultaneous multi-spectral windows spectropolarimetry of the Domeless Solar Telescope at Hida Observatory to select which spectral line is good for future Japanese space missions. At the end of presentation, I would like to discuss with you science objectives what you want to study using the polarimetry.||6/12||K.Otsuji||Which spectral line is good for future Japanese space missions?||In next monday's seminar as a short talk, I will introduce the papers shown below: "On HMI solar oblateness during solar cycle 24 and impact of the space environment on results" Meftah, M.; Hauchecorne, A.; Bush, R. I.; Irbah, A. Advances in Space Research, Volume 58, Issue 7, p. 1425-1440. http://ads.nao.ac.jp/abs/2016AdSpR..58.1425M||pptx||6/12||H.Isobe||gFlux rope seismology for diagnosing the eruption onset.h||The references are: Forbes 1990, JGR, 95, 11919 Isobe & Tripathi 2006, A&A, 449, L17 Isobe, Tripathi, Asai & Jain 2007, Sol. Phys. 246, 89 Pinter, Jain, Tripathi & Isobe 2008, ApJ, 680, 1560 Foullon, Verwichte, & Nakariakov 2009, ApJ, 700, 1658 Joshi et al. 2016, ApJ, 833, 243 I will also show some results of MHD simulation of flux rope oscillation with changing the parameters that control the flux ropefs (loss of) equilibrium.||pptx||6/19||H.Tamazawa||In today's seminar as as short talk, I will introduce the paper shown below, "Atmospheric impace of the strongest known solar particle storm of AD 775" Sukhodolov et al. 2017 Scientific Reports, 7, 45257||pptx||6/19||Elena Kupriyanova||6/26||S.Ninomiya||In todayfs seminar, I will introduce the paper shown below, gStatistics of convective collapse event in the photosphere and chromosphere observed with the Hinode SOTh C. E. Fischer, A. G. de Wijin, R. Centeno, B. W. Lites, and C. U. Keller A&A 504,583-588(2009) http://ads.nao.ac.jp/abs/2009A%26A...504..583F||pptx||6/26||T.Sakaue||"Numerical Experiments on the Powerful and Variable Irradiance from the Stellar Chrmosphere."||I will talk about my recent study, the title of which is "Numerical Experiments on the Powerful and Variable Irradiance from the Stellar Chrmosphere." The motivation and the current progress status are discussed in the seminar.||7/3||7/10||K.Nishida||"Next generation computer system in Kwasan Observatory"||7/10||T.Ishii||"Point like jets and surges at the emerging flux region before/during pore formation (NOAA 12660) on 2017-May-22 observed with SMART/SDDI"http://www.hida.kyoto-u.ac.jp/SMART/SDDI/event_report/2017_05/ http://www.kwasan.kyoto-u.ac.jp/~ishii/tmp/SDDI/20170522/||pptx|
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