Solar Seminar (Zasshikai) Home Page (FY2017)


Solar Seminar (13:00-15:00 Monday, Room 504 5th floor building 4) Access

News
The next seminar will start from 13:00 on Oct. 23rd (Mon).
We have main talk at 13:00-14:00 and short talk at 14:00-14:30.
  • Useful webpage list for solar observers.
  • See also Ishii-san's Webpage and Webpage of Kwasan and Hida Observatories.
  • Next presenters

    Date Name Title Abstract File
    2017-10-23
    main
    A.Tei
    upload or download
    2017-10-23
    short
    T.Sakaue
    upload or download

    For Speakers
    Presentation time for speaker is
    main : 40 minutes as a guide, and 20 minutes discussion.
    short : 20 minutes as a guide, and 10 minutes discussion.
    Contents of talk are
    main : about your study
    short : review of recent interesting paper and share information of recent study of the Sun.
    Language of slide and talks
    Master cource students : Language of slide and talk could be Japanese
    Doctor cource students and over : Slide must be English, and talking language could be Japanese
    (If those who could not understand Japanese attend the seminar, it is preferable that you talk in English)
    Title and Abstract
    Please send the title and abstract of your presentation by the day before.
    Presentation files
    Please upload your presentation files by the start of the seminar.
    If the presentation file is very big, please zip the file before uploading.
    For Audiences
    Honoring speakers
    Plase clap your hands as a closure of a presentation to express your respection to a speaker.
    For everyone
    Publication sharing
    Please send a copy of the submitted version of any paper on which they are working to the zasshikai mailing list just after submission

    Upcoming

    #DateNameTitle Abstract

    Main speaker
    Shibata, Ichimoto, Nagata, Ueno, Asai, Ishii, Nishida, Otsuji, Anan, Isobe,
    Tamazawa, Kawamura, Takeshige, Notsu, Hirose, Denis, Kou, Sakaue, Tei,
    Nakamura, Namekata, Ninomiya, Seki, Machida, Okada, Tokuda
    Short speaker
    Shibata, Ichimoto, Nagata, Ueno, Asai, Ishii, Nishida, Otsuji, Anan, Isobe,
    Tamazawa, Kawamura, Takeshige, Notsu, Hirose, Denis, Kou, Sakaue, Tei,
    Nakamura, Namekata, Ninomiya, Seki, Machida, Okada, Tokuda

    Presentations in this semester

    Date Name Title Abstract File
    10-02
    short
    S.Ueno introduction of some examples of recent Indian group's studies using long-term Kodaikanal full-disk CaII K digitized data References:

    "A BUTTERFLY DIAGRAM AND CARRINGTON MAPS FOR CENTURY-LONG Ca II K SPECTROHELIOGRAMS FROM THE KODAIKANAL OBSERVATORY"
    Subhamoy Chatterjee, Dipankar Banerjee, and B. Ravindra
    2016, ApJ 827, 87

    "Association of Plages with Sunspots: A Multi-Wavelength Study Using Kodaikanal CaII K and Greenwich Sunspot Area Data"
    Sudip Mandal, Subhamoy Chatterjee, and Dipankar Banerjee
    2017, ApJ 835, 158

    "Long-term Variations in the Intensity of Plages and Networks as Observed in Kodaikanal Ca-K Digitized Data"
    Muthu Priyal, Jagdev Singh, Ravindra Belur, Somasundaram Kameshwaran Rathina
    2017, Sol.Phys. 292, 85

    "Variation of Supergranule Parameters with Solar Cycles: Results from Century-long Kodaikanal Digitized CaII K Data"
    Subhamoy Chatterjee, Sudip Mandal, and Dipankar Banerjee
    2017, ApJ 841, 70

    "ASSOCIATION OF SUPERGRANULE MEAN SCALES WITH SOLAR CYCLE STRENGTHS AND TOTAL SOLAR IRRADIANCE"
    SUDIP MANDAL, SUBHAMOY CHATTERJEE, DIPANKAR BANERJEE
    2017, ApJ, accepted on May 31
    10-02
    Guest
    P.Heinzel
    10-16
    short
    A.Asai introduction of a just published paper "Variation of the Solar Microwave Spectrum in the Last Half Century"
    by M. Shimojo, K. Iwai, A. Asai, S. Nozawa, T. Minamidani, and M. Saito
    2017, Astrophysical Journal, Vol. 828, Number 1, id 62
    DOI: https://doi.org/10.3847/1538-4357/aa8c75
    pptx
    10-16
    main
    A.Machida
    • Determination of the wave property in the quiescent prominence
    • Study about the velocity field of the Arch Filament System
    • From the spectroscopic observation with Domeless Solar Telescope at Hida Observatory, we found a wave in Doppler velocity and temperature of a prominence. I will discuss the possible property of the wave.
    • We are now applying Becker's cloud model (the code was developed by Otsuji-san) to Arch Filament Systems in order to calculate the velocity field. I will introduce this study and discuss the relation between the velocity field and the geometry of the AFS.
    pdf
    10-23
    short
    T.Sakaue
    10-23
    main
    A.Tei
    10-30
    short
    S.Nagata
    10-30
    main
    K.Otsuji
    11-13
    Guest
    Y.Rahul
    11-27
    short
    H.Isobe
    11-27
    main
    D.Seki
    ...
    short
    ...
    ...
    main
    ...



    Previous presentations

    2017-1st Zasshikai Website
    Go to Zasshikai 2017-1st
    2016 Zasshikai Website
    Go to Zasshikai 2016
    2015 Zasshikai Website
    Go to Zasshikai 2015
    All of 2014
    2014 Archive (tar.gz file, 1.9Gbyte)
    All of 2013
    2013 Archive (tar.gz file, 2.4Gbyte)
    All of 2012
    2012 Archive (tar.gz file, 780Mbyte)
    All of 2011
    2011 Archive (tar.gz file, 780Mbyte)
    All of 2010
    2010 Archive (tar.gz file, 625Mbyte)



    If there are any mistakes or errors in this webpage,
    please send e-malis to the organizer, Huang Y.W (kouui_at_kwasan.kyoto-u.ac.jp).