Final Program

Monday August 27

10:30-12:30 Session 1: Solar dynamo and activity cycles: observations, theories and simulations. I.
                    Chair: Cheng Fang

10:30-11:00 Multi-scale nature of solar magnetism and cyclicity of magnetic activity
                        Sami 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.
                    Chair: Axel Brandenburg

14:00-14:30 Flux-transport and mean-field dynamo theories of solar cycles
                       Arnab 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
                    Chair: Arnab Choudhuri

16:00-16:30 Magnetic activity cycles across the HR-diagram
                       Svetlana Berdyugina (Germany)
16:30-16:45 The vigorous activity of young solar-type stars
                        Mark Miesch (USA)
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"
                        Char: Jingxiu Wang

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
                    Chair: Kristof Petrovay

14:00-14:30 Physics of solar 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
                    Chair: Yihua Yan

16:00-16:30 Helicity transport from the convection zone to interplanetary space
                        Mei 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
                    Chair: Elisabete de Gouveia Dal Pino

10:30-11:00 Starspot detection and properties
                        Igor Savanov (Russia)
11:00-11:30 Mechanisms of formation of solar pores and spots
                        Irina Kitiashvili (USA)
11:30-11:45 Ejections of magnetic structures above a spherical wedge driven by
                    a convective dynamo with differential rotation
                        Joern Warnecke (Sweden)
11:45-12:00 Current Helicity of in Solar Active Regions as a Tracer of Solar Dynamo
                        Dmitry Sokoloff  (Russia)

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

16:00-18:00 Session 9: Stellar and planetary dynamos
                        Chair: David Webb

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  Model of poleward magnetic field streams from sunspot butterflies
                        Nadezhda Zolotova (Russia)
17:45-18:00  Dynamo in subsurface convective layers
                        Matteo Cantiello (USA)

Thursday August 30

10:30-12:30 Session 10: Interstellar and galactic dynamos

10:30-11:00 Magnetic fields in our Milky Way and nearby galaxies
                        Jinlin Han (China)
11:00-11:30 Interstellar and intergalactic dynamos
                        Michal Hanasz (Poland)
11:30-12:00 Dynamo seed fields in proto-galaxies and dynamo action in young galaxies
                        Jennifer Schober  (Germany)
12:00-12:30  Measuring magnetic fields in interstellar gas, in the Milky Way, and beyond
                       Bryan Gaensler (Australia)

Friday August 31

8:30-10:00 Session 11: Critical physical ingredients for dynamos: turbulence and instabilities

8:30-9:00 Stellar and interstellar turbulence
                    Blakesley Burkhart (USA)
9:00-9:30 Interlinks between MHD turbulence and dynamos
                    Elisabete de Gouveia Dal Pino (Brazil)
9:30-9:45   On MHD Turbulence and Angular Momentum Transport in Accretion Disk Boundary Layers
                    Chan Chi-kwan  (Sweden)
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 theories
                        Valery 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 dynamics
                        Gianna Cauzzi (Italy)
14:30-15:00 Observational methods for stellar magnetism: from detection to cartography
                        Klaus Strassmeier (Germany)
15:00-15:15 Bcool
                         Stephen Marsden (Australia)
15:15-15:30 Radio Imaging-Spectroscopy Observations of the Sun in Decimetric Wavelengths
                         Yihua Yan  (China)

16:00-18:00 Session 14: New frontiers in understanding the origins of cosmic magnetism

16:00-16:15 Negative effective magnetic pressure in turbulent convection
                        Petri Kapyla (Finland)
16:15-16:30 Turbulent pumping of magnetic flux reduces the memory of the solar cycle
                       Dibyendu Nandy (India)
16:30-16:45 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)
16:45-17:15  Prospect on intergalactic magnetic field measurements with gamma-ray instruments
                       Helene Sol (France)

17:15-18:00 Discussion and 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 Dynamo
    Cameron 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
   
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 Simulation 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
   
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 modes
    Chamandy 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
   
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 fitting
    Ning 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
       
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 MS
    Tang 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
   
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
   
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
   
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
   
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
   
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
   
Not Much Helicity is Needed to Drive Large Scale Dynamos
Jonathan Pietarila Graham, jpietarilagraham@mailaps.org, Los Alamos National Laboratory, USA
Eric Blackman, University of Rochester, USA
Pablo Mininni, NCAR, USA
Annick Pouquet NCAR, USA