Preliminary Program
Monday August 27
10:30-12:30 Session 1: Solar dynamo and activity cycles: observations, theories and simulations. I.
10:30-11:00 Multi-scale nature of solar magnetism and cyclicity of magnetic activitySami Solanki (Germany)
11:00-11:30 Helioseismic Measurements of Differential Rotation and Meridional Flows
Junwei Zhao (USA)
11:30-12:00 Observations of magnetic and kinetic helicity proxies
Hongqi Zhang (China)
12:00-12:30 Sunspot properties and the solar dynamo
Aimee Norton (Australia)
14:00-15:30 Session 2: Solar dynamo and activity cycles: observations, theories and simulations. II.
14:00-14:30 Flux-transport and mean-field dynamo theories of solar cyclesArnab Choudhuri (India)
14:30-15:00 Solar-cycle precursors and predictions
Jie Jiang (China)
15:00-15:30 Poster introductions 1 (1 min each) - chair Axel Brandenburg
16:00-18:00 Session 3: Solar and
stellar dynamos
and cycles
Svetlana Berdyugina (Germany)
16:30-16:45 Model of poleward magnetic field streams from sunspot butterflies
Nadezhda Zolotova (Russia)
16:45-17:00 Solar magnetic field reversals and the role of dynamo families
Allan Sacha Brun (France)
17:00-17:15 Magnetic helicity as a probe of magnetic flux-tube dynamics in the solar interior
Takashi Sakurai (Japan)
17:15-17:30 Magnetic network elements in solar cycle 23
Chunlan Jin (China)
17:30-18:00 Poster introductions 2 (1 min each) - chair Arnab Rai Choudhuri
Tuesday August 28
10:30-12:30 Session 4: Local dynamo: ubiquitous small-scale magnetic fields and "hidden magnetism"10:30-11:00 Discovery of ubiquitous small-scale fields
Saku Tsuneta (Japan)
11:00-11:30 New spectropolarimetric diagnostics of unresolved magnetic fields
Natalia Schukina (Ukraine) & Javier Trujillo Bueno (Spain)
11:30-12:00 Links between the local and global dynamos
Jan Stenflo (Switzerland)
12:00-12:15 Convective mechanism of amplification and structuring of magnetic fields
Alexander Getling (Russia)
12:15-12:30 On the origin of quiet-Sun magnetic fields revealed with Hinode
Ryohko Ishikawa (Japan)
14:00-15:30 Session 5:
Magnetoconvection and local dynamo
Manfred Schuessler (Germany)
14:30-15:00 Fractal multi-scale nature of solar/stellar magnetic fields
Valentina Abramenko (USA)
15:00-15:30 Poster introductions 3 (1 min each) - chair Kristof Petrovay
16:00-18:00 Session 6: Coronal activity: driving mechanisms, and role in the dynamo process
16:00-16:30 Helicity transport from the convection zone to interplanetary spaceMei Zhang (China)
16:30-17:00 Driving mechanisms of magnetic energy release phenomena, flares and CME at various stages of solar/stellar cycles
Kazunari Shibata (Japan)
17:00-17:30 Magnetic helicity ejections and coronal activity
Alexander Nindos (Greece)
17:30-18:00 Poster introductions 4 (1 min each) -chair Yihua Yan
Wednesday August 29
8:30-10:00 Plenary Session - Keynote talk: "The Origin and
Evolution of Cosmic Magnetism”
Bryan Gaensler (Australia)
10:30-12:30 Session 7: Magnetic self-organization of solar/stellar plasma
10:30-11:00 Starspot detection and propertiesIgor Savanov (Russia)
11:30-12:00 Mechanisms of formation of solar pores and spots
Irina Kitiashvili (USA)
12:00-12:30 Poster introductions 5 (1 min each) - chair Elisabete de Gouveia Dal Pino
14:00-15:30 Session 8: Poster viewing
session
16:00-16:30 Mechanisms of planetary and stellar dynamos
Emmanuel Dormy (France)
16:30-17:00 Complexes of activity ("active longitudes") and their role in dynamo
Maarit Mantere (Finland)
17:00-17:15 Magnetic field generation in an accretion disk of close binary star
Dmitry Bisikalo (Russia)
17:15-17:30 Modeling the grand minima of solar activity using a flux transport dynamo model
Binay Bidya Karak (India)
17:30-17:45 The vigorous activity of young solar-type stars
Benjamin Brown (USA)
17:45-18:00 Dynamo in subsurface convective layers
Matteo Cantiello (USA)
Thursday August
30
11:00-11:30 Magnetic fields in our Milky Way and nearby galaxies
Jinlin Han (China)
11:30-12:00 Interstellar and intergalactic dynamos
Michal Hanasz (Poland)
12:00-12:30 Key physical processes in the galactic dynamos
Anvar Shukurov (UK)
Friday August 31
8:30-10:00 Session 11: Critical physical ingredients for dynamos: turbulence and instabilities
8:30-9:00 Stellar and interstellar turbulenceBlakesley Burkhard (USA)
9:00-9:30 Interlinks between MHD turbulence and dynamos
Elisabete Dal Pino (Brazil)
9:30-9:45 On MHD Turbulence and Angular Momentum Transport in Accretion Disk Boundary Layers
Martin Pessah (Denmark)
9:45-10:00 Topological restrictions in magnetic field dynamics and reconnection
Simon Candelaresi (Sweden)
10:30-12:30 Session 12: Advances in dynamo theories, simulations and experiments
10:30-11:00 Advances in mean-field dynamo theoriesValery Pipin (Russia)
11:00-11:30 Non-linear and chaotic dynamo regimes
Axel Brandenburg (Sweden)
11:30-12:00 Theory of differential rotation and meridional circulation
Leonid Kitchatinov (Russia)
12:00-12:15 Experimental realization of dynamo action: present status and prospects
Andre Giesecke (Germany)
12:15-12:30 Global numerical simulations of solar convection and differential rotation
Gustavo Guerrero (USA)
14:00-15:30 Session 13: Current and new observing programs from the ground and space
14:00-14:30 Synthesis of high-resolution and global-Sun observations of solar magnetism and dynamicsGianna Cauzzi (Italy)
14:30-15:00 Observational methods for stellar magnetism: from detection to cartography
Klaus Strassmeier (Germany)
15:00-15:30 Prospect on intergalactic magnetic field measurements with gamma-ray instruments
Helene Sol (France)
16:00-18:00 Session 14: New frontiers in understanding the origins of cosmic magnetism
16:00-16:30 Dynamo seed fields in proto-galaxies and dynamo action in young galaxiesJennifer Schober (Germany)
16:30-16:45 Turbulent pumping of magnetic flux reduces the memory of the solar cycle
Dibyendu Nandy (India)
16:45-17:00 How the knowledge of stellar activity is needed for the exoplanetary field
(and how the exoplanetary research helps the stellar dynamo understanding)
Isabelle Boisse (Portugal)
17:00-17:15 Measuring magnetic fields in interstellar gas, in the Milky Way, and beyond
Bryan Gaensler (Australia)
17:15-18:00 Summary
Alexander Kosovichev (USA), Yihua Yan (China),
Lidia van Driel-Gesztelyi (France), Elisabete de Gouveia Dal Pino (Brazil)
Posters
Group 1
Nonlinear feedback and the Solar DynamoCameron Robert, cameron@mps.mpg.de, MPS, Germany
RHESSI and SDO/AIA observations of the chromospheric and coronal plasma parameters during a solar flare
Kontar Eduard, eduard@astro.gla.ac.uk, University of Glasgow United Kingdom
Battaglia Marina, University of Applied Sciences and Arts Northwestern, Switzerland
Evolution of Coronal Bright Points in different regions of Solar Atmosphere
Sattarov Isroil, isattar@astrin.uz, Astronomical Institute AS of Uzbekistan
Karachik Nina, Tashkent state pedagogical university
Sherdanov Chori, Astronomical institute AS of Uzbekistan
Minenko Ekaterina, Astronomical Institute AS of Uzbekistan
Tillaboev Azlarkhon, Tashkent state pedagogical university
On the magnetic field diffusion in the partially ionized plasma
Tsap Yuri, yur@crao.crimea.ua, Crimean Astrophysical Observatory
Flows in the Photosphere and in the Interior in Two Active Regions
Liu Yang, yliu@sun.stanford.edu, Stanford University, United States
Zhao Junwei, Stanford University
Schuck Peter, NASA
Radio Imaging-Spectroscopy Observations of the Sun in Decimetric Wavelengths
Yan Yihua, yyh@nao.cas.cn, Key Lab of Solar Activity, NAOC, China
Wang Wei, Key Lab of Solar Activity, NAOC
Liu Fei, Key Lab of Solar Activity, NAOC
Geng Lihong, Key Lab of Solar Activity, NAOC
Chen Zhijun, Key Lab of Solar Activity, NAOC
Zhang Jian, Department of Astronomy, Peking University
Modelling stellar activity cycles using deep-seated dynamos and surface flux transport
Isik Emre, e.isik@iku.edu.tr, Istanbul Kultur University, Turkey
Solar Cycle and Quasi-biennial Variations in Helioseismic Frequencies
Tripathy Sushanta, stripathy@nso.edu, National Solar Observatory, Tucson, USA
Jain Kiran, jain@nso.edu, National Solar Observatory, Tucson, USA
Simoniello Rosaria, rosaria.simoniello@pmodwrc.ch, CEA/DSM/IRFU/SAp-AIM, CE Saclay, France
Hill Frank, fhill@nso.edu, National Solar Observatory, Tucson, USA
Turck-Chieze Sylvain, sylvaine.turck-chieze@cea.fr, CEA/DSM/IRFU/SAp-AIM, CE Saclay, France
Two successive filament eruptions accompanying a flare
Bi Yi, biyi@ynao.ac.cn, Yunnan Astronomical Observatory
Hong Junchao, hjcsolar@ynao.ac.cn, Yunnan Astronomical Observatory, China
A small-scale EUV jet in the quiet Sun region
Hong Junchao, hjcsolar@ynao.ac.cn, Yunnan Astronomical Observatory China
Solar initiative at Oukaimeden Observatory
Benkhaldoun Zouhair, zouhair@ucam.ac.ma, Oukaimeden Observatory, Cadi Ayyad University, Morocco
Makela Jonathan, jmakela@illinois.edu, Department of Electrical and Computer Engineering University of Illinois
Meriwether John W., meriwether@ces.clemson.edu, Clemson University, Clemson, SC (USA)
Phase relationship between polar faculae and sunspot numbers
Deng Lin-hua, Yunnan Astronomical Observatory, Chinse Academy of Sciences.
Flare-associated Type III Radio Bursts and Dynamics of the EUV Jet from SDO/AIA and RHEISS Observations
Chen NAI-HWA, d949001@astro.ncu.edu.tw, Graduate institute of Astronomy Taiwan, China
Ip Wing-Huen, wingip@astro.ncu.edu.tw, Graduate institute of Astronomy
Innes Davina, innes@mps.mpg.de, Max-Planck-Institut fuer Sonnensystemforschung
Radiative Hydrodynamic Silumation of He 10830
Cheng Jianxia, jxcheng@nju.edu.cn, School of Astronomy & Space Science, Nanjing University
Ding Mingde, School of Astronomy & Space Science, Nanjing University
Fang Cheng, School of Astronomy & Space Science, Nanjing University
On the compatibility of a flux transport dynamo with a fast tachocline scenario
Karak Bidya Binay, bidya_karak@physics.iisc.ernet.in, Department of Physics, Indian Institute of Science, Bangalore 560012, India
Petrovay Kristof, K.Petrovay@astro.elte.hu, Budapest, Hungary
A developed method for filament automatic detection and statistical studies
Hao Qi, hq_turtle@163.com, Nanjing University, China
Fang Cheng, Nanjing University
Chen P.F., Nanjing University
Evolution and DEM analysis of Early Structures of Coronal Mass Ejections by SDO-AIA
Cheng Xin, Nanjing University
Zhang Jie, George Mason University
Ding Ming-de, Nanjing University
SDO/AIA and Hinode/EIS Observations of Interaction between EUV wave with nearby Active Region Loops
Yang Liheng, Key Laboratory of Solar Activity, National Astronomical Observatories
Zhang Jun, Key Laboratory of Solar Activity, National Astronomical Observatories
Li Ting, Key Laboratory of Solar Activity, National Astronomical Observatories
3D MHD Simulation of Non-convective Spruit's Dynamo - Application to Polar Field Amplification in the Sun -
Masada Youhei, ymasada@harbor.kobe-u.ac.jp, Department of Computational Science, Kobe University, Japan
Impact of MHD Turbulence on Thermal Wind Balance in the Sun
Masada Youhei, ymasada@harbor.kobe-u.ac.jp, Department of Computational Science, Kobe University Japan
The helicity, induced electric field and the Poynting flux of AR 11158 and their relationship with the X-class flare
Liu Jihong, liujh@bao.ac.cn, Shijiazhuang University China
Su jiangtao, National Astronomical Observatories
Zhang hongqi, National Astronomical Observatories
The Stellar Rotation - Activity Relationship and the Evolution of Stellar Dynamos
Wright Nicholas, nwright@cfa.harvard.edu, Harvard-Smithsonian Center for Astrophysics, United States
Drake Jeremy, Harvard-Smithsonian Center for Astrophysics
Mamajek Eric, University of Rochester
Henry Gregory, Tennessee State University
3-D Perspectives of Solar Activity Using Modern Solar and Heliospheric Imaging
Rouillard Alexis, arouillard@irap.omp.eu, Institut De Recherche En Astrophysique et Planetologie
A quest for activity cycles in low mass stars
Krisztian Vida, vidakris@konkoly.hu, Konkoly Observatory Hungary
New Magnetic Measurements of T Tauri Stars with CRIRES
Yang Hao, haoyang@phy.ccnu.edu.cn, Central China Normal University China
Johns-Krull Christopher M., Rice University
CrH molecule: new diagnostic tool for measuring magnetic fields in ultra-cool dwarfs
Kuzmychov Oleksii, oleksii.kuzmychov@kis.uni-freiburg.de, Kiepenheuer-Institut fur Sonnenphysik, Germany
Berdyugina Svetlana, sveta@kis.uni-freiburg.de, Kiepenheuer-Institut fur Sonnenphysik
Group 2
Galactic spirals and dynamo action: Slaved non-axisymmetric modesChamandy Luke, lchamandy@gmail.com, Inter-University Centre for Astronomy and Astrophysics, India
Subramanian Kandaswamy, kandu@iucaa.ernet.in, Inter-University Centre for Astronomy and Astrophysics
Shukurov Anvar, anvar.shukurov@newcastle.ac.uk, University of Newcastle
Optical Flares and Dark-Spot Activity of Red-Dwarf Close Binary Stars
Zhu Liying, zhuly@ynao.ac.cn, Yunnan Astronomical Observatory China
Qian Shengbang, qsb@ynao.ac.cn, Yunnan Astronomical Observatory
Liu Liang, Yunnan Astronomical Observatory
He Jiajia, Yunnan Astronomical Observatory
Zhao Ergang, Yunnan Astronomical Observatory
Wang Jingjing, Yunnan Astronomical Observatory
Jiang Linqiao, Yunnan Astronomical Observatory
Calibration and data analysis for CSRH
Wang Wei,, wwang@nao.cas.cn National Astronomical Observatories, CAS China
Yan Yihua, yyh@nao.cas.cn,, National Astronomical Observatories, CAS
Liu Donghao, dhliu@nao.cas.cn, National Astronomical Observatories, CAS
Geng Lihong, genglh@nao.cas.cn, National Astronomical Observatories, CAS
Chen Zhijun, zjchen@nao.cas.cn, National Astronomical Observatories, CAS
Chen Linjie, ljchen@nao.cas.cn, National Astronomical Observatories, CAS
Su Cang, csu@nao.cas.cn, National Astronomical Observatories, CAS
Observation of Interplanetary Scintillation in China
Liu Lijia, ljliu@nao.cas.cn, NAOC China
Self-cancellation of ephemeral regions in the quiet Sun
Yang Shuhong, shuhongyang@nao.cas.cn, NAOC China
Zhang Jun, zjun@nao.cas.cn, NAOC
Li Ting, liting@nao.cas.cn, NAOC
Liu Yang, yliu@quake.stanford.edu, Stanford University
Rotating stellar models of low-mass, pre-main sequence stars with an imposed magnetic field
Mendes Luiz, luizt@cpdee.ufmg.br, Departamento de Eng. Eletronica, Universidade Federal de Minas Gerais, Brazil
Landin Natalia, nlandin@ufv.br, Departamento de Fisica, Universidade Federal de Vicosa
Vaz Luiz, vaz@fisica.ufmg.br, Departamento de Fisica, Universidade Federal de Minas Gerais
Binary and multiple magnetic Ap/Bp stars
Rastegaev Denis, leda@sao.ru, SAO RAS Russian Fed
Large scale magnetic helicity flux estimated from MDI magnetic synoptic charts over the 23rd solar cycle
Shangbin Yang, yangshb@bao.ac.cn, National Astronomical Observatories, Chinese Academy of Sciences China
Zhang Hongqi, hzhang@bao.ac.cn, National Astronomical Observatories, Chinese Academy of Sciences
NIR polarimetry as a probe of the large-scale structure of the Galactic Magnetic Field
Pavel Michael, pavelmi@bu.edu, Boston University, United States
Simulations of Prominece Formation in the Magnetized Solar Corona by Chromospheric Heating
Xia Chun, School of Astronomy and Space Science, Nanjing University
Chen Pengfei, School of Astronomy and Space Science, Nanjing University
Keppens Rony ,Centre for Plasma Astrophysics, K.U. Leuven
Flares and Magnetic Non-potentiality of NOAA AR 11158
Song Qiao, qsong@nao.cas.cn, NAOC China
Zhang Jun, NAOC
Yang Shuhong, NAOC
Liu Yang Stanford University
Bcool
Marsden Stephen, stephen.marsden@jcu.edu.au, Centre for Astronomy, James Cook University, Australia
Petit Pascal, Institut de Recherche en Astrophysique et Planetologie
Jeffers Sandra, Institut fur Astrophysik Gottingen
Jardine Moira, University of St. Andrews
Dintrans Boris, Institut de Recherche en Astrophysique et Planetologie
Bouvier Jerome, Laboratoire d'Astrophysique de Grenoble
Konstantinova-Antova Renada, Bulgarian Academy of Sciences
do Nascimento Jose Dias, Universidade Federal do Rio Grande do Norte
Morin Julien, Institut fur Astrophysik Gottingen
Tests and Applications of Nonlinear Force-Free Field Extrapolations in the Spherical Geometry
Guo Yang, guoyang@nju.edu.cn, School of Astronomy and Space Science, Nanjing University China
Ding Mingde, dmd@nju.edu.cn, School of Astronomy and Space Science, Nanjing University
Fundamental properties and Seismological Analysis of three Kepler stars
liu kang, liukangscorpio@live.cn, Beijing Normal University China
Bi Shaolan, Beijing Normal University
Effect of Magnetic Fields on Lithium Depletion of Solar-type Stars
Li Tanda, litanda@hotmail.com, Beijing Normal University
Bi Shaolan, Bejing Normal University
Magnetic activity and solar-like pulsations in X-ray sources in the Kepler field of view
MOLENDA-ZAKOWICZ JOANNA, molenda@astro.uni.wroc.pl, University of Wroclaw, Poland
Frasca Antonio, antonio.frasca@oact.inaf.it, INAF - Osservatorio Astrofisico di Catania
Froehlich Hans-Erich HEF,roehlich@aip.de, AIP Potsdam, Germany
Bonanno Alfio, abo@oact.inaf.it, INAF - Osservatorio Astrofisico di Catania
Busa Innocenza, Innocenza.Busa@oact.inaf.it, INAF - Osservatorio Astrofisico di Catania
Catanzaro Giovanni, Giovanni.Catanzaro@oact.inaf.it, INAF - Osservatorio Astrofisico di Catania
Covey Kevin, kcovey@astro.cornell.edu, Lowell Observatory
Corsaro Enrico, eco@oact.inaf.it, INAF - Osservatorio Astrofisico di Catania
Metcalfe Travis, travis@ucar.edu, High Altitude Observatory
Marilli Ettore, Ettore.Marilli@oact.inaf.it, INAF - Osservatorio Astrofisico di Catania
Biazzo Katia, kbiazzo@na.astro.it, INAF - Osservatorio Astrofisico di Napoli
Leone Francesco, fleone@oact.inaf.it, INAF - Osservatorio Astrofisico di Catania
Development of the Super High Angular Resolution Principle for X-ray imaging
Chen Zhang, chzhang@bao.ac.cn, National Astronomical Observatories, Chinese Academy of Sciences, China
Zhang Shuang Nan, zhangsn@ihep.ac.cn, Institute of High Energy Physics , Chinese Academy of Sciences
The gap of differential rotation in early F-type stars
Ammler-von Eiff Matthias, ammler@tls-tautenburg.de, Thueringer Landessternwarte Tautenburg, Germany
Reiners Ansgar, Institute for Astrophysics Goettingen
On the behavior stellar rotation in the solar neighbourhood
de Freitas Daniel Brito, danielbrito@dfte.ufrn.br, DFTE/UFRN
De Medeiros Jose Renan, DFTE/UFRN
A nonextensive approach for the angular momentum loss rate in low-mass stars
de Freitas Daniel Brito, danielbrito@dfte.ufrn.br, DFTE/UFRN
De Medeiros Jose Renan, DFTE/UFRN
Numerical Study of Morphology of Turbulent Convection
Tian Chunlin, chunlin.tian@helsinki.fi, Department of Physics, Univseristy of Helsinki, Finland
Petrovay Kristof, Department of Astronomy, ELTE
The formations and eruptions of a filament
Zhou Guiping, gpzhou@nao.cas.cn, Key Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences
Tsuneta S., National Astronomical Observatory, Mitaka, Tokyo 181-8588, Japan
Wang Jingxiu, wangjx@nao.cas.cn, Key Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences
Two Types of Magnetic Reconnection in Coronal Bright Points and the Corresponding Magnetic Configuration
Zhang Qingmin, zhangqm@nju.edu.cn, School of Astronomy and Space Science, Nanjing University
Chen Pengfei, chenpf@nju.edu.cn, School of Astronomy and Space Science, Nanjing University
Guo Yang, guoyang@nju.edu.cn, School of Astronomy and Space Science, Nanjing University
Fang Cheng, fcheng@nju.edu.cn, School of Astronomy and Space Science, Nanjing University
Ding Mingde, dmd@nju.edu.cn, School of Astronomy and Space Science, Nanjing University
Non-collisional pitch angle scattering and hard X-ray observations of solar flares
Burge Christina, c.burge@astro.gla.ac.uk, University of Glasgow, United Kingdom
Kontar Eduard, University of Glasgow
The Butterfly Diagram Leopard Skin Pattern
Ternullo Maurizio, mternullo@oact.inaf.it, INAF - Osservatorio Astrofisico di Catania, Italy
Five-Element Digital Corrector Receiver for the Chinese Spectral Radioheliograph
Zhao An, azhao@nao.cas.cn, National Astronomical Observatories of Chinese Academy of Sciences, China
Yan Yihua, National Astronomical Observatories of Chinese Academy of Sciences
Accuracy analysis and application of extrapolation of force-free fields in solar active and quiet regions
Liu Suo, lius@nao.cas.cn, National Astronomical Observatory, Chinese Academy of Sciences, Beijing, China
Zhang Hongqi, hzhang@nao.cas.cn, National Astronomical Observatory, Chinese Academy of Sciences, Beijing, China
Su Jiangtao, sjt@nao.cas.cn, National Astronomical Observatory, Chinese Academy of Sciences, Beijing, China
Song Mutao, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing, China
Group 3
Ages of open clusters NGC 6791 and NGC 6819 using the asterseismic isochrones fittingNing Gai, ning_gai@163.com, Department of Physics, Dezhou University
Probing the cores of RGB Bump stars with asteroseismic l=1 modes
Ning Gai, ning_gai@163.com, Department of Physics, Dezhou University
The simulation of imaging capabilities for the Chinese Spectral Radioheligraph
Du Jing, National Astronomical Observatories, Chinese Academy of Sciences
Yan Yihua, National Astronomical Observatories, Chinese Academy of Sciences
Wang Wei, National Astronomical Observatories, Chinese Academy of Sciences
The Morphologic Properties of Magnetic networks over the Solar Cycle 23
Huang Chong, chuang@nao.cas.cn, Key Laboratory of Solar Activity,National Astronomical Observatories, Chinese Academy of Sciences China
Yan Yihua, Key Laboratory of Solar Activity,National Astronomical Observatories, Chinese Academy of Sciences
Zhang Yin, Key Laboratory of Solar Activity,National Astronomical Observatories, Chinese Academy of Sciences
Tan Baolin, Key Laboratory of Solar Activity,National Astronomical Observatories, Chinese Academy of Sciences
Solar Flares During Deep Solar Minimum as Observed Simultaneously by SphinX and RHESSI
Mrozek Tomasz, mrozek@astro.uni.wroc.pl, Solar Physics Division, Space Research Centre, Polish Academy of Sciences, Poland
Gburek Szymon, Solar Physics Division, Space Research Centre, Polish Academy of Sciences
Siarkowski Marek, Solar Physics Division, Space Research Centre, Polish Academy of Sciences
Sylwester Barbara, Solar Physics Division, Space Research Centre, Polish Academy of Sciences
Sylwester Janusz, Solar Physics Division, Space Research Centre, Polish Academy of Sciences
Gryciuk Magdalena, Solar Physics Division, Space Research Centre, Polish Academy of Sciences
Kepa Anna, Solar Physics Division, Space Research Centre, Polish Academy of Sciences
Research on the extrapolating method of solar coronal magnetic field
Wang Rui, ray@nao.cas.cn, National Astronomical Observatories of China, China
Yan Yihua, yyh@nao.cas.cn, National Astronomical Observatories of China
The characters of energetic electron transportation during solar flares
Huang Jing, National Astronomical Observatories, Chinese Academy of Sciences
Yan YiHua, National Astronomical Observatories, Chinese Academy of Sciences
Statistic Analysis of Zebra Pattern Structures at 2.6-3.8GHz in an X3.4 Solar Flare
Yu Sijie, sjyu@nao.cas.cn, National Astronomical Observatories, Chinese Academy of Sciences
Yan Yihua, yyh@nao.cas.cn, National Astronomical Observatories, Chinese Academy of Sciences
Tan Baoling, bltan@nao.cas.cn, National Astronomical Observatories, Chinese Academy of Sciences
Construction of Digital Image Database of 44-year Synoptic Observation of Solar Chromosphere in Kyoto University
Kitai Reizaburo, kitai@kwasan.kyoto-u.ac.jp, Kyoto University
Ueno Satoru, Kyoto University
Katoda Miwako, Kyoto University
Hada Yuko, Kyoto University
Hayashi Hiroo, Kyoto University
Asai Ayumi, Kyoto University
Helicity characteristics of sunspot umbra and penumbra
Hao Juan, haojuan@nao.cas.cn, National Astronomical Observatories, Chinese Academy of Sciences, China
Zhang Mei, zhangmei@nao.cas.cn, National Astronomical Observatories, Chinese Academy of Sciences
Interaction Between Global EUV Wave and Coronal Hole
Xue Zhike, zkxue@ynao.ac.cn, Yunnan Astronomical Observatory, China
Qu Zhongquan, Yunnan Astronomical Observatory
Yan Xiaoli, Yunnan Astronomical Observatory
Negative effective magnetic pressure in turbulent convection
Kapyla Petri, petri.kapyla@helsinki.fi, University of Helsinki, Finland
Mantere Maarit, maarit.mantere@helsinki.fi, University of Helsinki
Brandenburg Axel, brandenb@nordita.org, NORDITA
Rogachevskii Igor, gary@bgu.ac.il, Ben-Gurion University of the Negev
Kleeorin Nathan, nat@bgu.ac.il, Ben-Gurion University of the Negev
Study of Ribbon Separation and Magnetic Reconnection Rates
Xie Wenbin, wb_xie@bao.ac.cn, Department of Physics, Jilin Normal University
Zhang Hongqi, National Astronomical Observatories, Chinese Academy of Sciences China
Lin Jun YunNan, Astronomical Observatory, Chinese Academy of Sciences
Wang Haimin, New Jersey Institute of Technology
Recent observations from solar radio spectrometers of Huairou, China
Tan Chengming, tanchm@nao.cas.cn, National Astronomical Observatories, Chinese Academy of Sciences, China
Solar Interior Zonal and Meridional Flows Obtained from Time-Distance Helioseismology Analysis
Zhao Junwei, junwei@sun.stanford.edu, Stanford University, United States
Bogart Rick, Stanford University
Kosovichev Alexander, Stanford university
Duvall Tom, NASA Goddard Flight Center
Growth rate of magnetic field during star burst phase in a galaxy
Ko Chung-Ming, cmko@astro.ncu.edu.tw, Institute of Astronomy, National Central University, Taiwan Taiwan, China
The geometrical information of the Sun
Wang Xiaofan, wxf@nao.cas.cn, National Astronomical Observatories, Chinese Academy of Sciences
Sigismondi Costantino, sigismondi.costantino@gmail.com, ICRA and Sapienza University of Rome
A Statistical Study on Photospheric Active-Region Magnetic Nonpotentiality and Associated Flares During Solar Cycles 22-23
YANG Xiao, yangx@nao.cas.cn, Key Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences China
ZHANG HongQi, Key Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences
GAO Yu, Key Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences
GUO Juan, Key Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences
LIN GangHua, Key Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences
Simulation of a CME-driven shock by multiple scattering angular distributions
Wang Xin, wangxin@nao.cas.cn, National Astronomical Observatories, Chinese Academy of Sciences, China
Yan Yihua, National Astronomical Observatories, Chinese Academy of Sciences
Frequency And Time Properties Of Decimeter Narrowband Spikes In Solar Flares
Wang Shujuan, wsj@nao.ac.cn,, National Astronomical Observatories, Chinese Academy of Sciences
Polar jet kinetics and energetics analysed from STEREO/COR data
Feng Li, Purple Mountain Observatory, CAS, China
Inhester Bernd, Max Planck Institute for Solar System Research, Germany
Gan Weiqun, wqgan@pmo.ac.cn, Purple Mountain Observatory, CAS, China
A complex active-region filament eruption: the event on 2000 February 9
Defang Kong, Yunan Astronomical Observatory
Observations and Magnetic Field Modeling of the Solar Flare/CME Event on 2010 April 8
Su Yingna, ynsu@head.cfa.harvard.edu, Harvard-Smithsonian Center for Astrophysics, United States
Kliem Bernhard, Institute for Physics and Astronomy, University Potsdam
van Ballegooijen Adriaan, Harvard-Smithsonian Center for Astrophysics
Surges Vicent, Harvard-Smithsonian Center for Astrophysics
Deluca Edward, Harvard-Smithsonian Center for Astrophysics
Golub Leon, Harvard-Smithsonian Center for Astrophysics
Magnetic helicity transported by flux emergence and shuffling motions in Solar Active Region NOAA 10930
Zhang Yin,, zhangyin@bao.ac.c,n NAOC
Kitai R Kwasan and Hida Observatories, Kyoto University, Yamashina-ku, Kyoto 607-8471
Takizawa Kan, Kwasan and Hida Observatories, Kyoto University, Yamashina-ku, Kyoto 607-8471
Automatic Identification of Solar Granules and Magnetic Bright PointsAutomatic Identification of Solar Granules and Magnetic Bright Points
Safari Hossein, safari@znu.ac.ir, Department of Physics, University of Zanjan, Iran
Javaherian Mohsen, m_javaherian@znu.ac.ir, Department of Physics, University of Zanjan
An Automatic Method for Identification of Solar Coronal Loops
Safari Hossein, safari@znu.ac.ir, Department of Physics, University of Zanjan, Zanjan, Iran
Taran Somayeh, Department of Physics, University of Zanjan, Zanjan, Iran
Space Environment during Solar Minimum of CS-23
Hady Ahmed, Abdel aahady@yahoo.com, Cairo University
Group 4
The relationship between nu_max and age t of stars from MSTang Yanke, Department of Physics, Dezhou University
First year results and challenges from the Heliometer at Obsevatorio Nacional, Rio de Janeiro
Andrei Alexandre Humberto, oat1@on.br (1) ON/MCTI; (2) OATo/INAF; (3) SYRTE/OP; (4) OV/UFRJ Italy
D'Avila Victor Amorim, victor@on.br, ON/MCTI
Reis Neto Eugenio, eug.reis@gmail.com, MAST/MCTI
Penna Jucira Lousad, jucira@on.br ON/MCTI
Boscardin Sergio Calderari, sergio.boscardin@on.br, ON/MCTI
Coletti Alissandro, sandroac34@gmail.com, Azeheb/FACC
Oliveira Luiz Carlos, loveira2@bol.com.br, NGC51
Sigismondi Costantino, costantino.sigismondi@gmail.com, Sapienza University of Rome
Ejections of magnetic structures above a spherical wedge driven by a convective dynamo with differential rotation
Warnecke Joern, joern@nordita.org, Nordita, Sweden
Kapyla Petri, Department of Physics, Helsinki University
Mantere Maarit, Department of Physics, Helsinki University
Brandenburg Axel, Nordita
Solar Microwave Quasi-periodic Pulsations with Multi-timescale and Fine Structures
Tan Baolin, bltan@nao.cas.cn, NAOC
Magnetic helicity injection in NOAA 11261 associated with flares
Xu Haiqing, xhq@bao.ac.cn, National Astronomical Observatories, Chinese Academy of Sciences China
Zhang Hongqi, hzhang@bao.ac.cn, National Astronomical Observatories, Chinese Academy of Sciences
Su Jiangtao, sjt@bao.ac.cn, National Astronomical Observatories, Chinese Academy of Sciences
Ruan Guiping, Shandong Provincial Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment, School of Space Science and Physics,Shandong, University at Weihai
Liu Jihong, Department of physics electrical engineering department of information, Shi Jiazhuang University
Magnetic Helicity in Emerging Active Regions: A Statistical Study
Liu Yang, yliu@sun.stanford.edu, Stanford University, United States
Team HMI, Stanford University
The flow helicity in quasi-ordered cellular convection
Getling Alexander V., a.getling@mail.ru, Institute of Nuclear Physics, Lomonosov Moscow State University, Moscow, 119991Russia
Stable magnetic fields in stars
Reisenegger Andreas, areisene@astro.puc.cl, Pontificia Universidad Catolica de Chile Chile
Akgun Taner, akgun@astro.cornell.edu, Barcelona Supercomputing Center
Marchant Pablo, pimarcha@uc.cl, Pontificia Universidad Catolica de Chile
Armaza Cristobal, cyarmaza@uc.cl, Pontificia Universidad Catolica de Chile
Mastrano Alpha, alpham@unimelb.edu.au, University of Melbourne
Chromospheric Activity of Late-type Stars
Zhang Liyun, liy_zhang@hotmail.com, Guizhou University
The Doppler imaging of active star Sigma Gem in 2011
Gu Sheng-hong, shenghonggu@ynao.ac.cn, Yunnan Observatory, China
Telting John, Nordic Optical Telescope
Collier Cameron Andrew, St. Andrews University
Changing Photospheric Vector Magnetic Fields Associated with a B4.2-class Solar Flare
Su Jiangtao, National Astronomical Observatories, Chinese Academy of Sciences
Liu Yu, National Astronomical Observatories, Yunnan observatory, Chinese Academy of Sciences
Shen Yuandeng , National Astronomical Observatories, Yunnan observatory, Chinese Academy of Sciences
An extreme ultraviolet wave associated with a failed eruption observed by the Solar Dynamics Observatory
zheng ruisheng, zhrsh@ynao.ac.cn, Yunnan Astronomical Observatory, China
Modeling the solar cycles 12-20 with a realistic Babcock-Leighton flux transport dynamo
Jiang Jie, jiejiang@nao.cas.cn, NAOC, China
Cameron Robert, MPS
Isik Emre, Department of Physics, Faculty of Science & Letters, Istanbul Culture University
CoRot observation of a young Sun-like star
GONDOIN Philippe, pgondoin@rssd.esa.nl, European Space Agency ,Netherlands
Gandolfi Davide, dgandolf@rssd.esa.nl, European Space Agency
Generation of magnetic structures in stratified turbulence.
Kemel Koen, koen@nordita.org, Nordita
Brandenburg Axel, Nordita
Kleeorin Nathan, Ben-Gurion University of the Negev
Mitra Dhrubaditya, Nordita
Rogachevskii Igor, Ben-Gurion University of the Negev
Comparison of Solar Activity During Last Two Minima on turn of Cycles Activity 22/23 and 23/24
Gryciuk Magdalena, mg@cbk.pan.wroc.pl, Space Research Centre, Polish Academy of Sciences, Poland
Gburek Szymon, sg@cbk.pan.wroc.pl, Space Research Centre, Polish Academy of Sciences
Siarkowski Marek, ms@cbk.pan.wroc.pl, Space Research Centre, Polish Academy of Sciences
Farnik Frantisek, Astronomical Institute of Academy of Sciences of the Czech Republic
Geomagnetic field generation due to surface destruction of the solid core
Starchenko Sergey, sstarchenko@mail.ru, IZMIRAN, Troitsk, Moscow region Russian Fed
Pushkarev Yuriy, ydcanon@rambler.ru, IPGG, St.-Petersburg, Russia
Magnetism and convection scaling laws in planets
Starchenko Sergey, sstarchenko@mail.ru, IZMIRAN, Troitsk, Moscow region Russian Fed
A nonlinear flux transport dynamo model for the Sun
Isik Emre, e.isik@iku.edu.tr, Istanbul Kultur University Turkey
Cameron Robert, cameron@mps.mpg.de Max Planck Institute for Solar System Research
Schmitt Dieter, schmitt@mps.mpg.de Max Planck Institute for Solar System Research
Delta Sunspots In Solar Cycle 22-23
Guo Juan, guojuan@bao.ac.cn, Key Laboratory of Solar Activity, National Astronomical Observatories, Beijing, China
SATURATION OF THE MAGNETOROTATIONAL INSTABILITY BY STABLE MAGNETOACOUSTIC MODES
Liverts Eduard, eliverts@bgu.ac.il, Ben Gurion University of the Negev Israel
Shtemler Yuri, yshtemler@gmail.com, Ben Gurion University of the Negev
Mond Michael, mond@bgu.ac.il, Ben Gurion University of the Negev
Umurhan Orkan, mumurhan@ccsf.edu, City College of San Francisco
Long-term temporal variations in the mean maximum size of sunspot groups
Javaraiah Javaraiah, jj@iiap.res.in, Indian Institute of Astrophysics, Bangalore-560034, India
Dependence of solar cycles duration on the magnitude of the annual module of the magnetic fields of sunspots
Krivodubskij Valery, krivod1@observ.univ.kiev.ua, Astronomical Observatory, Kiev National Taras Shevchenko University
Lozitskaja Nataly, nloz@observ.univ.kiev.ua, Observatory, Kiev National Taras Shevchenko University
On the extended 23rd solar cycle dynamo-period
Krivodubskij Valery, krivod1@observ.univ.kiev.ua, Astronomical Observatory, Kiev National Taras Shevchenko University
The Effect of Twisted Magnetic Field on the Period Ratio P1/P2 of Nonaxisymmetric MHD Waves
Karami Kayoomars, kkarami@uok.ac.ir, Department of Physics, University of Kurdistan, Pasdaran Street, Sanandaj, Iran
Bahari Karam, K.Bahari@razi.ac.ir, Physics Department, Faculty of Science, Razi University, Kermanshah, Iran
Group 5
Toward understanding the multiscale spatial spectrum of solar convection
Getling Alexander V., a.getling@mail.ru, Institute of Nuclear Physics, Lomonosov Moscow State University, Moscow, 119991Russia
Kolmychkov Vyacheslav V., ksv@keldysh.ru, Keldysh Institute of Applied Mathematics, Russian Academy of Sciences, Moscow, 125047 Russia
Mazhorova Olga S., olgamazhor@mail.ru, Keldysh Institute of Applied Mathematics, Russian Academy of Sciences, Moscow, 125047 Russia
Shcheritsa Olga V., shchery@keldysh.ru, Keldysh Institute of Applied Mathematics, Russian Academy of Sciences, Moscow, 125047 Russia
Probing the solar origin of energy build-up and release in solar energetic particles
AWASTHI ARUN KUMAR, awasthi@prl.res.in, Physical Research Laboratory, India
Jain Rajmal, rajmal@prl.res.in, Physical Research Laboratory
Bhatt Nipa, nijibhatt@hotmail.com, C. U. Shah Science College
Generalization of the Neupert effect over the Solar Flare Plasma Cooling
AWASTHI ARUN KUMAR, awasthi@prl.res.in, Physical Research Laboratory, India
Jain Rajmal, rajmal@prl.res.in, Physical Research Laboratory
Analysis of the Sunspot Observations by Gustav Sporer in 1861–1893
Diercke Andrea, Humboldt-Universitat zu Berlin
Arlt Rainer, Leibniz-Institut fur Astrophysik Potsdam
Denker Carsten, cdenker@aip.de, Leibniz-Institut fur Astrophysik Potsdam, Germany
Statistical characteristics of horizontal proper motions in the vicinity of pores
Verma Meetu, Leibniz-Institut fur Astrophysik Potsdam
Denker Carsten, cdenker@aip.de, Leibniz-Institut fur Astrophysik Potsdam, Germany
SOLAR ENERGY UTILITIES
Udayashankar Paniveni, paniveni.udayashankar@gmail.com, NIEIT, Mysore
Relative Navigation Based on Adaptive UKF Technology for Satellites Formation Flying
Jiangfei WU, wjf015@163.com, Institute of Surveying and Mapping, Information Engineering University, Zhengzhou, China
Evolution of magnetic field corresponding to X-ray brightening events in coronal holes and quiet Sun regions
Huang Zhenghua, zhu@arm.ac.uk, Armagh Observatory, United Kingdom
Madjarska Maria, Armagh Observatory
Doyle Gerry, Armagh Observatory
Lamb Derek, Southwest Research Institute
A Study of Connections between Solar Flares and Subsurface Flow Fields of Active Regions
Gao Yu, gy@bao.ac.cn, Key Laboratory of Solar Activiry, National Astronomical Observatories, Chinese Academy of Sciences
Zhao Junwei, W.W. Hansen Experimental Physics Labratory
Zhang Hongqi, Key Laboratory of Solar Activiry, National Astronomical Observatories, Chinese Academy of Sciences
DYNAMICS OF THE MAGNETOSPHERE DURING THE 8 - 9 MARCH 2008 CIR/HSS DRIVEN GEOMAGNETIC STORM
Garg Shobhit, gargshobhit@ucla.edu, UCLA United States
Peroomian Vahe, vahe@igpp.ucla.edu, UCLA
El-Alaoui Mostafa, mostafa@igpp.ucla.edu, UCLA
Chemical composition of photospheres in RS CVn stars
Tautvaisiene Grazina, grazina.tautvaisiene@tfai.vu.lt, Vilnius University, Lithuania
Barisevicius Gintaras, gintaras.barisevicius@tfai.vu.lt, Vilnius University, Lithuania
Berdyugina Svetlana, sveta@kis.uni-freiburg.de, Kiepenheuer Institut fur Sonnenphysik, Germany
Ilyin Ilya, ilyin@aip.de, Astrophysical Institute Potsdam, Germany
Chorniy Yuriy, yuriy.chorniy@tfai.vu.lt, Vilnius University
Solar-cycle variation of solar structure near the surface: the adiabatic index
Rabello-Soares M. Cristina, cristina@sun.stanford.edu, Stanford University, United States
Perturbations in the wave parameters near active regions
Rabello-Soares M. Cristina, cristina@sun.stanford.edu, Stanford University, United States
Bogart Richard S., rick@sun.Stanford.EDU, Stanford University
Scherrer Philip H., phil@sun.Stanford.EDU, Stanford University
Knotty Invariants: Structure and Evolution of Magnetized Fluids.
Roth Ilan, ilan@ssl.berkeley.edu, University of California, Berkeley, United States
An intelligent observing method for solar flare.
jiaben lin, jiaben.lin@163.com, Key Laboratory of solar activity, China
yuanyong deng, Key Laboratory of solar activity
juan guo, Key Laboratory of solar activity
zhen zeng, Key Laboratory of solar activity
Magnetogasdynamic shock waves generated by a piston moving in a non-uniform self-gravitating rotational axisymmetric gas in the presence of conductive and radiative heat fluxes
Nath Gorakh, gn_chaurasia_univgkp@yahoo.in, National institute of Technology Raipur, India
Variations of the solar cycle profile in a solar dynamo with fluctuating dynamo governing parameters
Pipin Valery, valery.pipin@gmail.com, Institute solar-terrestrial physics, Irkutsk
Sokoloff Dmitry, d_sokoloff@hotmail.com, Moscow State University
Usoskin Ilya, ilya.usoskin@oulu.fi, Sodankylae Geophysical Observatory, Oulu University
On the transport of the large-scale magnetic field induced by the "helicity-vorticity" effect
Pipin Valery, valery.pipin@gmail.com, Institute solar-terrestrial physics, Irkutsk, Russian Fed
On the Source of Energy of Stars
Avagyan Slavik, slavikavagyan@yahoo.com, State Engineering University of Armenia, Gyumri Campus
Solar dynamo model with nonlocal alpha-effect and diamagnetic pumping
Kitchatinov Leonid, kit@iszf.irk.ru, Institute for Solar-Terrestrial Physics, Irkutsk, Russia
Olemskoy Sergey, osv@iszf.irk.ru, Institute for Solar-Terrestrial Physics, Irkutsk, Russia
Observational Evidence of Unwinding and Chirality Changing in Penumbral Filaments by Hinode
Su Jiangtao, sjt@bao.ac.cn, National Astronomical Observatories, Chinese Academy of Sciences
Current Helicity of in Solar Active Regions as a Tracer of Solar Dynamo
Sokoloff Dmitry, d_sokoloff@hotmail.com, Moscow State University, Russia
Znang Hongqi, hzhang@bao.ac.cn, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China
Moss David, moss@maths.man.ac.uk, School of Mathematics, University of Manchester, Manchester M13 9PL, UK
Kleeorin Nathan, nat@menix.bgu.ac.il, Department of Mechanical Engineering, Ben-Gurion University of Negev, POB 653, 84105 Beer-Sheva, Israel
Kuzanyan Kirill, kuzanyan@izmiran.ru, IZMIRAN, Troitsk, Moscow Region 142190, Russia
Rogachevskii Igor, gary@bgu.ac.il, Department of Mechanical Engineering, Ben-Gurion University of Negev, POB 653, 84105 Beer-Sheva, Israel
Yu Gao, gy@bao.ac.cn, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China
Haiqing Xu, xu@bao.ac.cn, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China
Observations of a geomagnetic SI+-SI –pair and associated solar wind fluctuations
Bisoi Susanta Kumar, bisoi.susanta@gmail.com, Physical Research Laboratory, Ahmedabad, India
Padmanabhan Janardhan, jerry@prl.res.in, Physical Research Laboratory, Ahmedabad, India
Peculiar behavior of solar polar fields during solar cycles 21-23: Correlation with meridional flow speed
Bisoi Susanta Kumar, bisoi.susanta@gmail.com, Physical Research Laboratory, Ahmedabad, India
Padmanabhan Janardhan, jerry@prl.res.in, Physical Research Laboratory, Ahmedabad, India
Inner heliospheric Interplanetary Scintillation signatures of the deepest solar minimum in the past 100 years.
Bisoi Susanta Kumar, bisoi.susanta@gmail.com, Physical Research Laboratory, Ahmedabad, India
Padmanabhan Janardhan, jerry@prl.res.in, Physical Research Laboratory, Ahmedabad, India
Asymmetries in periodicities of the photospheric magnetic field of the sun: A probe to the unusual solar minimum prior to the solar cycle 24
Bisoi Susanta Kumar, bisoi.susanta@gmail.com, Physical Research Laboratory, Ahmedabad, India
Padmanabhan Janardhan, jerry@prl.res.in, Physical Research Laboratory, Ahmedabad, India