Contributed Posters - Abstracts

All POSTERS are concurrent but are labeled according the session numbers for topical interest. POSTERS may apply to more than one session but they are only listed once and all have a unique poster number (7.N.M).

 
• Session II
  • II: Spectral/time characteristics of radio precursors of solar flares
  • II/III/IV/V: The Coherent Large-Scale Clusters On The Solar Surface
  • II/VII: Latitudinal and temporal distribution of the solar photospheric magnetic flux periodicities during 1975 - 200 years
• Session III
  • III: Global asymmetry of the Sun observed in the extreme ultraviolet radiation
  • III: Solar Total and X-ray irradiance variations
  • III: Center-to-limb-variation of Facular Contrast, Derived from Hawaii RISE/PSPT Full Disk Images
  • III: Absolute Radiometric Measurements in Space, ARMS
  • III: Study of Solar and Spectral Irradiance Variations via MDI and VIRGO on SOHO
  • III: Photospheric Energy Budgets
  • III: PREMOS - a satellite experiment to monitor the solar irradiance at selected wavelength
  • III/VI: Non Periodic Variations of the Solar Diameter
  • III/VI: The New Instrument for Solar Diameter Measurements at Rio de Janeiro
  • III/IX: Short-term and long-term variability of solar ultraviolet Irradiances in recent years: Association with ionospheric parameters and stratospheric ozone
  • III/IV: Is F10.7 a Good Proxy for Solar EUV Flux?
  • III/IV: Calcium II Monitoring Program at the National Solar Observatory
  • III/I: The EOS Solar Radiation and Climate Experiment (SORCE) Mission
  • III/I: Solar Extreme Ultraviolet Measurements from the NASA TIMED Satellite
  • III: Operational solar irradiance and E10.7 forecasts from SOLAR2000
  • III: Draft ISO solar irradiance standard WD 21348
  • III/IV/VI: High Resolution Solar Spectral Variability Near Mg II Measured by HRTS
  • III/IV: Study of Solar Irradiance Variability Using PSPT Observations Ground-based Study of Solar Irradiance Variability Using the RISE/PSPT
  • III/VIII: The Total Irradiance Monitor for Future Solar Measurements
  • III/VII: Solar Continuum and Magnetic Field Observations by the MDI Instrument
  • III/V: Scrutinizing five years of the EUV Sun
  • III: Monitoring Solar Activity From SWAN/SOHO Lyman Alpha Interplanetary Background Images
• Session IV
  • IV: Dependence of contrast/area function on the sunspot area databases
  • IV: Improved Modeling of the Solar FUV Irradiance Using the Mg II C/W Index
  • IV: Solar Irradiance and Magnetic Field Variations from Solar Cycles 21 to 23
  • IV: Variations in Solar EUV Flux as Measured by SOHO/ CELIAS/ SEM
  • IV: Solar Irradiance Variability at Short and Long Wavelengths
  • IV/VI/VII: Variability of Chromospheric Features and Implications on UV Irradiance Variability
  • IV/VI/VII: Variability of CaII K Emission Flux Over the Solar Cycle
  • IV: Effective Sunspot Temperatures from Solar Light Curves: a Starspot Modeling Approach to the Sun
  • IV/VIII: Irradiance and solar Radius variations
  • IV/VI: Intensity Distribution of Small Magnetic Features from Minimum to Maximum
  • IV/VII: Temporal variability of YOHKOH SXT X-ray spectral irradiance
  • IV/VII: Active region associated 5303 A emission
  • IV/VI: Effective Sunspot Temperatures Derived from VIRGO Data: Applying a Starspot Modeling Approach to the Sun
  • IV/VII: Heliospheric Magnetic Field Modulation in the Last Centuries: Validation from Measurements of the Cosmogenic Ti-44 in Meteorites
• Session V
  • V: The April 15 and 18, 2001 Solar Energetic Particle Events recorded by the LION instrument on SOHO, and associated Ground Level Events recorded at medium latitudes
  • V: Temporal evolution of 1.68 y periodicity in cosmic rays
  • V: Nonstationary electrojets in the solar corona
  • V: Coronal/Interplanetary Disturbances Relating to Strong Solar Proton Events
  • V: Acceleration of Coronal Mass Ejections and Association with Surface Activity
  • V: Effective space weather forecasts/warnings with observations of active-region evolution
  • V: Solar Synoptic Charts for Solar Cycle Studies
  • V: Physical conditions of prominences before/during eruption
  • V: Neutral Atom Diffusion in a Partially Ionized Prominence Plasma
  • V: Successive CMEs and Transient Flow Systems
  • V: Predicting Proton Storms from Solar Flare X-rays
  • V: Cosmic Rays and Space Weather, 1. On-line Search of the Start of Great Flare Energetic Particle Events
  • V: Cosmic Rays and Space Weather, 2. On-line Determination of Flare Energetic Particle Spectrum
  • V: Title: Cosmic Rays and Space Weather, 3. Automatically Determination of Diffusion Coefficient in the Interplanetary Space and Energy Spectrum in Source
  • V: Cosmic Rays and Space Weather, 4. Cosmic Ray Using for Forecasting of Major Geomagnetic Storms Accompanied by Forbush-Effects
  • V: Variability of Galactic Cosmic Radiation Impacting the Earth: 1600-2000
  • V: Solar Variability as Deduced from 400 Years of Large Fluence Solar Proton events
  • V/VII: On the possible association of CME to spikes observed at submm-waves
  • V/VIII: Solar Cycle Studies of Sudden Ionospheric Disturbances
  • V/IX: Forecasting geomagnetic storm with the feature of interplanetary energetic particles
• Session VI
  • VI/VII: PSPT measurement of the supergranular intensity contrast
  • VI: The Sun-Earth Connection Event during July 14-16, 2000: from the Sun to the Earth
  • VI: Flare Index of Ascending Branch of Cycle 23
  • VI: Variability of the total solar irradiance as a new index of the cyclicity of the solar activity
  • VI: Reversals of the solar global magnetic field
  • VI: Analytical Expressions of Basic physical parameters of N. dimensional isothermal symmetrical polytrops
  • VI: The possible model of energy sources of the solar activity cycles of 11-years and quasi-biannual periodicity
  • VI: Solar variability as it is seen in helioseismology and biomedicine
  • VI/VII: Variability of the solar magnetic field, neutrino flux, diameter and solar activity indexes
  • VI/VII: Large-Scale Magnetic Field Evolution in Different Time Scales
  • VI/VII: The variability of the solar polar magnetic fields
  • VI/VII: Streamers structure and solar magnetic field
  • VI: Acoustic oscillations, their origin and power variation from minimum to maximum of solar activity
  • VI/VII: Long Term Variations of the Poloidal to Toroidal Solar Magnetic Flux Amplification Factor and Associated Solar Terrestrial
  • VI/VII: Solar Synoptic Observing Programs
• Session VII
  • VII: Magnetic Reconnection driven by Surface Alfven Waves in Chromospheric Current Sheets: Lower Coronal Loops Heating
  • VII: Theoretical plasma model for intracloud lightning
  • VII: Rossby Waves and Vortices in the Solar and Terrestrial Atmospheres
  • VII: Increase in sun's magnetic field intensity for Solar Cycles 16 -21
  • VII: Total Solar Irradiance and Coronal Index of Solar Activity
  • VII: Radio and X-Ray Emissions from Termination Shocks During the November 25, 2000, 09:08 UT Flare
  • VII: Evolution of the magnetic field of the active region NOAA 7978 during five disk passages
  • VII: White-light eclipse corona and magnetic field connections during the solar cycle
  • VII: Magnetic-Flux Emergence into the Solar Corona
  • VII: Do Changes in Solar UV Flux Influence a Major Mode of Atmospheric Variability?
  • VII: Solar Cycle 23: Variation of the Solar Corona in the Ultraviolet from Solar Minimum to Solar Maximum
  • VII: The 88-Year Cycle in the Modulation of the 11-year Solar Cycle Intensity
  • VII/III: On relevance of the coronal FeXIV 530.3 nm emission line intensity for studying the cyclic and evolutionary solar processes
  • VII/VIII: The Solar Activity Maximum For Cycle 23
• Session VIII
  • VIII: NOAA Electron Climatology: A Space Weather Model of Electron Precipitation
  • VIII: The Low Cloud - Cosmic Ray Flux Correlation Revisited
  • VIII/IX: Global Magnetic Field of the Sun and Long-term Variations of Galactic Cosmic Rays
  • VIII/IX: Evaluation of the ozone sensitivity to the variation of spectral solar flux
  • VIII/IX: Measurement Of Solar Radiation at a High Altitude Observatory, Hanle
  • VIII/IX: Current-carrying Production of Nitrogen Oxide NO
  • VIII/IX: Solar Cycle Effects on the Winter Rainfall Variations in INDIA
  • VIII/I/II: Tree Ring Growth and Geomagnetic Disturbances
  • VIII: Interactions between the 11-year solar cycle and the QBO in a zonally averaged two-dimensional dynamical-photochemical model
  • VIII: Galactic cosmic rays, particle formation, natural variability of global cloud properties, and climate implications
  • VIII/VI: Persistence of the Gleissberg (88-yr) Solar Cycle over the Last 10,000 Years: Evidence from Cosmogenic Isotopes
  • VIII: Possible Solar Modulation of the Equatorial QBO: Additional Statistical Evidence
• Session IX
  • IX: New Evidence of Space Weather Impact on the Terrestrial Weather and Climate in the Earth's Southern Hemisphere
  • IX: Coronal Mass Ejections, Central axial field direction in magnetic clouds and Geomagnetic Storms
  • IX: Effect of solar activity on the Earth's environment
  • IX: Some Aspects of Recent Studies in Solar-Terrestrial Relations
  • IX: Secular and cycle variations of the IMF Bz component and some associated geophysical effects