| Preface |
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xiii | |
| Editors |
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xv | |
| Conference Photograph |
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xvii | |
| Participants |
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xviii | |
| Session 1 |
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Large-scale flows in the Sun: Characteristics and time variations |
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3 | (6) |
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22 Year Solar Magnetic Cycle and its relation to Convection Zone Dynamics |
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9 | (2) |
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Asymmetry in Solar Torsional Oscillation |
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11 | (2) |
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Lekshmi B. Dibyendu Nandy |
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Ambiguity of the Solar Meridional Flow |
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13 | (4) |
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| Session 2 |
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The new Sunspot Number: continuing upgrades and possible impacts |
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17 | (6) |
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Variations in Ca-K, line profiles and Ca-K line features as a function of latitude and solar cycle during the 20th century |
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23 | (4) |
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Un-interrupted Sun-as-a-star Helioseismic Observations over Multiple Solar Cycles |
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27 | (4) |
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Kyiv monitoring program of spectral line variations with the 11-year cycle |
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31 | (4) |
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Long-term stellar magnetic field study at the Crimean Astrophysical Observatory |
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35 | (4) |
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The long-term variation of the effective magnetic field of the active star element of Eridani |
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39 | (4) |
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Francesco Leone Manuele Gangi |
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Correlation of the New Sunspot Number and Geomagnetic as Index in the Years 1900-2013 |
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43 | (4) |
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A study on the variations in long-range dependence of solar energetic particles during different solar cycles |
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47 | (2) |
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Standard Magnetic Field Production at Huairou Solar Observing Station |
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49 | (2) |
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Long-term variations in meridional motion of sunspot groups: comparison of DPD and SOON data |
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51 | (2) |
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Energy distribution of solar flare events |
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53 | (2) |
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Flux tube model in the solar atmosphere |
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55 | (2) |
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Multivariate analysis of intermediate periodicities of the green corona |
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57 | (2) |
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Solar-Cycle variation in the photospheric mean velocity flows: GONG observations |
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59 | (2) |
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Coronal magnetic field measurements using forbidden emission lines |
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61 | (2) |
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Studying solar-cycle variation of open magnetic flux regions using coronal holes |
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63 | (2) |
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A study on universality, non-extensivity and Levy statistics of solar wind turbulence |
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65 | (2) |
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Superposed Epoch Analysis of High Latitude Ionospheric Joule Heating during Major Geomagnetic Storms over three Solar Cycles |
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67 | (2) |
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Energetics of Magnetosphere-Ionosphere system during main Phase of Intense Geomagnetic Storms over three Solar Cycles |
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69 | (2) |
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Decades of Chinese Solar and Geophysical Data |
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71 | (2) |
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Variation of the meteor count rate and echo height during solar cycle 23 and 24 |
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73 | (2) |
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Connection between Active region complexity and Solar Flare strength |
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75 | (2) |
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Search for Correlation between Solar Flare Count and Mean Solar Magnetic Field |
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77 | (2) |
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The morphological comparison and analysis of coronal green line |
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79 | (2) |
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Study of magnetic field topology of active region 12192 using an extrapolated non-force-free magnetic field |
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81 | (2) |
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Study of Interplanetary and Geomagnetic Response of Filament Associated CMEs |
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83 | (2) |
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Role of the background regimes towards the Solar Mean Magnetic Field (SMMF) |
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85 | (2) |
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A Magnetofrictional model for the solar corona |
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87 | (2) |
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Study of Stealth CMEs and associated ICMEs |
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89 | (2) |
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Synoptic Magnetic Fields Measurements of the Solar Chromosphere from SOLIS/VSM at NSO |
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91 | (4) |
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| Session 3 |
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Coronal mass ejections as a new indicator of the active Sun |
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95 | (6) |
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Automated Detection Methods for Solar Activities and an Application for Statistic Analysis of Solar Filament |
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101 | (7) |
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Long-term variations in the heliosphere |
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108 | (7) |
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The potential of Ca II K observations for solar activity and variability studies |
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115 | (6) |
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Long term trends in solar photospheric fields and solar wind turbulence levels: Implications to the near-Earth space |
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121 | (4) |
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Ca II K spectroheliograms for studies of long-term changes in solar irradiance |
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125 | (4) |
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Sunspot data collection of Specola Solare Ticinese in Locarno |
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129 | (4) |
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Sunspot group tilt angles from drawings for cycles 19-24 |
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133 | (4) |
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Reconstruction of solar activity according to the data of centenary observations |
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137 | (4) |
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Evolution of structures with an open magnetic flux over a hundred years |
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141 | (4) |
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Solar science at metric radio wavelengths: Coming of age |
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145 | (2) |
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Heliospheric Modulation of Cosmic Rays and Solar Activity during Solar Cycles 22-24 |
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147 | (2) |
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Solar Activities and Its Impact on Space Weather |
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149 | (2) |
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Forbush decrease caused by interacting and non-interacting passing CME |
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151 | (2) |
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On the Characteristics of Geomagnetic Storms Observed During the Past 415 Years |
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153 | (2) |
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Where do running penumbral waves emerge in chromosphere? |
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155 | (2) |
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A wavelet analysis of F2 layer critical frequency over solar cycle 23 |
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157 | (2) |
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First results from Automated Imaging Routine for Compact Arrays for Radio Sun |
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159 | (2) |
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Scaling Analysis of the Flare Index Data from Kandilli Observatory |
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161 | (2) |
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Study of solar flares associated with Geoeffective CMEs |
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163 | (2) |
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Phase analysis of solar activity indices using wavelet techniques |
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165 | (2) |
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Magnesium II Index measurements from SORCE SOLSTICE and GOES-16 EUVS |
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167 | (2) |
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The coronal green line monitoring: a traditional but powerful tool for coronal physics |
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169 | (2) |
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Automated detection of Coronal Mass Ejections in Visible Emission Line Coronagraph (VELC) on-board ADITYA-L1 |
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171 | (2) |
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Century long study of sunspot activity using the Kodaikanal white-light data |
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173 | (2) |
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Solar cycle variation of coronal mass ejections contribution to solar wind mass flux |
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175 | (2) |
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Multiple Solar Jets from NOAA AR 12644 |
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177 | (2) |
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Study of Coronal Rotation using X-ray images observed by Hinode |
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179 | (2) |
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Quantifying weak non-thermal meterwave solar emission using non-imaging techniques |
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181 | (2) |
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Magnetic field topology from non-force free extrapolation and magnetohydrodynamic simulation of its eventual dynamics |
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183 | (2) |
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Long-term variation of sunspot penumbra to umbra area ratio |
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185 | (2) |
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Properties of Coronal Holes in Solar Cycle 21-23 using McIntosh archive |
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187 | (2) |
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Migration of polar prominences in 13-24 cycles of activity |
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189 | (2) |
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Andrey Tlatov Valeriya Vasil'eva |
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Geometric and magnetic properties of coronal flux ropes associated with CMEs leading to geomagnetic storms |
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191 | (2) |
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C-1.4 class flare and an associated peculiar coronal jet |
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193 | (3) |
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An Overview of Science Results Obtained From Kodaikanal Digitized White-Light Data Archive: 1921-2011 |
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196 | (2) |
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Association of calcium network brightness with polar magnetic fields |
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198 | (5) |
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| Session 4 |
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Ultraviolet Solar Spectral Irradiance Variation on Solar Cycle Timescales |
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203 | (6) |
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Solar Activity Changes During Prolonged Sunspot Minima as Inferred from Indian Monsoon Rainfall Variations |
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209 | (4) |
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| Session 5 |
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A Stellar Perspective on the Magnetic Future of the Sun |
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213 | (4) |
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Phase difference between long-term magnetic feature activity and flare activity of solar-type stars |
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217 | (4) |
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Statistical Study of Solar White-light Flares and Comparison with Superflares on Solar-type Stars |
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221 | (104) |
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Prediction of upcoming grand episodes of solar activity |
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325 | (2) |
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A prediction of the solar cycle 25 |
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327 | (2) |
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| Author Index |
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329 | |
