Works matching IS 17439213 AND DT 2017 AND VI 13 AND IP S335
Results: 85
IAU volume 13 issue S335 Cover and Back matter.
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- Proceedings of the International Astronomical Union, 2017, v. 13, n. S335, p. b1, doi. 10.1017/S1743921318000777
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IAU volume 13 issue S335 Cover and Front matter.
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- Proceedings of the International Astronomical Union, 2017, v. 13, n. S335, p. f1, doi. 10.1017/S1743921318000765
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The Space Weather through a Multidisciplinary Scientific Approach.
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- Proceedings of the International Astronomical Union, 2017, v. 13, n. S335, p. 280, doi. 10.1017/S1743921318000741
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Analysis of Magnetic Field Variations Produced by Equatorial Electro-Jets.
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- Proceedings of the International Astronomical Union, 2017, v. 13, n. S335, p. 125, doi. 10.1017/S1743921318000662
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METU Data Driven Forecast Models: From the Window of Space Weather IAU Symposium 335.
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- Proceedings of the International Astronomical Union, 2017, v. 13, n. S335, p. 328, doi. 10.1017/S1743921318000613
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Numerical Short-Term Solar Activity Forecasting.
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- Proceedings of the International Astronomical Union, 2017, v. 13, n. S335, p. 243, doi. 10.1017/S1743921318000534
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Challenges and Strategic Research Plans for Earth and Heliosphere: Research Infrastructures, Projects and Initiatives.
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- Proceedings of the International Astronomical Union, 2017, v. 13, n. S335, p. 219, doi. 10.1017/S1743921318000571
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A Behavioural Model of the Solar Magnetic Cycle.
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- Proceedings of the International Astronomical Union, 2017, v. 13, n. S335, p. 94, doi. 10.1017/S174392131800056X
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Four-Spacecraft Magnetic Curvature Analysis on Kelvin-Helmholtz Waves in MHD Simulations.
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- Proceedings of the International Astronomical Union, 2017, v. 13, n. S335, p. 132, doi. 10.1017/S1743921318000522
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Data Handling and Assimilation for Solar Event Prediction.
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- Proceedings of the International Astronomical Union, 2017, v. 13, n. S335, p. 344, doi. 10.1017/S1743921318000510
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Acceleration of Solar Wind Particles Passing through the 3D Heliospheric Current Sheet.
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- Proceedings of the International Astronomical Union, 2017, v. 13, n. S335, p. 54, doi. 10.1017/S1743921318000443
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Re-Acceleration of Energetic Particles in Large-Scale Heliospheric Magnetic Cavities.
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- Proceedings of the International Astronomical Union, 2017, v. 13, n. S335, p. 75, doi. 10.1017/S1743921318000285
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SWERTO: a Regional Space Weather Service.
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- Proceedings of the International Astronomical Union, 2017, v. 13, n. S335, p. 348, doi. 10.1017/S1743921318000054
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The Ionosphere Prediction Service.
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- Proceedings of the International Astronomical Union, 2017, v. 13, n. S335, p. 352, doi. 10.1017/S174392131800025X
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The MOTH II Doppler-Magnetographs and Data Calibration Pipeline.
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- Proceedings of the International Astronomical Union, 2017, v. 13, n. S335, p. 335, doi. 10.1017/S1743921318000029
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Geomagnetic Consequences of Interacting CMEs of June 13-14, 2012.
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- Proceedings of the International Astronomical Union, 2017, v. 13, n. S335, p. 65, doi. 10.1017/S1743921317010857
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Towards Estimating the Solar Meridional Flow and Predicting the 11-yr Cycle Using Advanced Variational Data Assimilation Techniques.
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- Proceedings of the International Astronomical Union, 2017, v. 13, n. S335, p. 183, doi. 10.1017/S1743921317010754
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Monitor and Prediction of Near-Earth Radiation Environment in the Frame of Space Monitoring Data Center at Moscow State University.
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- Proceedings of the International Astronomical Union, 2017, v. 13, n. S335, p. 232, doi. 10.1017/S1743921317010456
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Variability of the Vertical Total Electron Content, from GPS data, during 2 to 8 November 2015, Using Oukaimeden and Rabat Stations in Morocco.
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- Proceedings of the International Astronomical Union, 2017, v. 13, n. S335, p. 159, doi. 10.1017/S1743921318000078
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Effects of ICMEs on High Energetic Particles as Observed by the Global Muon Detector Network (GMDN).
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- Proceedings of the International Astronomical Union, 2017, v. 13, n. S335, p. 69, doi. 10.1017/S1743921318000066
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How does the Sun Influence the Magnetospheres of Jupiter and Saturn?
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- Proceedings of the International Astronomical Union, 2017, v. 13, n. S335, p. 109, doi. 10.1017/S1743921317011620
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Physics-Based Modeling Activity from the Solar Surface to the Earth's Atmosphere Including Magnetosphere and Ionosphere at NICT.
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- Proceedings of the International Astronomical Union, 2017, v. 13, n. S335, p. 284, doi. 10.1017/S1743921317011668
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High Speed Solar Wind Forecast Model from the Solar Surface to 1AU Using Global 3D MHD Simulation.
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- Proceedings of the International Astronomical Union, 2017, v. 13, n. S335, p. 272, doi. 10.1017/S1743921317011607
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Spatial Inhomogeneity in Solar Faculae.
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- Proceedings of the International Astronomical Union, 2017, v. 13, n. S335, p. 17, doi. 10.1017/S174392131701136X
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A New Technique to Provide Realistic Input to CME Forecasting Models.
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- Proceedings of the International Astronomical Union, 2017, v. 13, n. S335, p. 258, doi. 10.1017/S1743921317011048
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The Coronal Solar Magnetism Observatory.
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- Proceedings of the International Astronomical Union, 2017, v. 13, n. S335, p. 359, doi. 10.1017/S1743921317011334
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Forecasting Solar Energetic Particle Events and Associated False Alarms.
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- Proceedings of the International Astronomical Union, 2017, v. 13, n. S335, p. 324, doi. 10.1017/S1743921317011036
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Excitation and Evolution of Transverse Loop Oscillations by Coronal Rain.
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- Proceedings of the International Astronomical Union, 2017, v. 13, n. S335, p. 36, doi. 10.1017/S1743921317011024
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Application of Test Particle Simulations to Solar Energetic Particle Forecasting.
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- Proceedings of the International Astronomical Union, 2017, v. 13, n. S335, p. 268, doi. 10.1017/S1743921317011012
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Statistical Analysis of Extreme Electron Fluxes in the Radiation Belts.
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- Proceedings of the International Astronomical Union, 2017, v. 13, n. S335, p. 128, doi. 10.1017/S1743921317011000
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Simulating the Dynamics of Coronal Plasma Condensations.
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- Proceedings of the International Astronomical Union, 2017, v. 13, n. S335, p. 23, doi. 10.1017/S1743921317010997
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Pursuing Forecasts of the Behavior and Arrival of Coronal Mass Ejections through Modeling and Observations.
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- Proceedings of the International Astronomical Union, 2017, v. 13, n. S335, p. 58, doi. 10.1017/S1743921317010882
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Reinforcing a Double Dynamo Model with Solar-Terrestrial Activity in the Past Three Millennia.
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- Proceedings of the International Astronomical Union, 2017, v. 13, n. S335, p. 211, doi. 10.1017/S1743921317010912
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The Response of the Martian Atmosphere to Space Weather.
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- Proceedings of the International Astronomical Union, 2017, v. 13, n. S335, p. 114, doi. 10.1017/S1743921317010924
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On the Evolution of Pre-Flare Patterns of a 3-Dimensional Model of AR 11429.
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- Proceedings of the International Astronomical Union, 2017, v. 13, n. S335, p. 294, doi. 10.1017/S1743921317010432
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Geomagnetopause Position and Shape Dependence on Solar Wind Plasma and IMF Parameters: Analytic Model Comparison with Observations and 3-D MHD Runs.
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- Proceedings of the International Astronomical Union, 2017, v. 13, n. S335, p. 121, doi. 10.1017/S1743921317010420
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The Mexican Early Warning System for Space Weather.
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- Proceedings of the International Astronomical Union, 2017, v. 13, n. S335, p. 236, doi. 10.1017/S1743921317010158
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CCMC Modeling of Magnetic Reconnection in Electron Diffusion Region Events.
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- Proceedings of the International Astronomical Union, 2017, v. 13, n. S335, p. 142, doi. 10.1017/S1743921317010845
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Principal Component Analysis of Geomagnetic Activity: New Information on Solar Wind.
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- Proceedings of the International Astronomical Union, 2017, v. 13, n. S335, p. 197, doi. 10.1017/S1743921317010146
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The Aging Solar Wind: a Break in Wind Evolution at Older Ages?
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- Proceedings of the International Astronomical Union, 2017, v. 13, n. S335, p. 98, doi. 10.1017/S1743921317010134
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Structure of the Power Spectral Density of Galactic Cosmic Ray Variation during 1953-2016.
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- Proceedings of the International Astronomical Union, 2017, v. 13, n. S335, p. 82, doi. 10.1017/S1743921317010122
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Determining the Polar Cusp Longitudinal Location from Pc5 Geomagnetic Field Measurements at a Pair of High Latitude Stations.
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- Proceedings of the International Astronomical Union, 2017, v. 13, n. S335, p. 139, doi. 10.1017/S174392131701002X
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On the Dynamics of the Largest Active Region of the Solar Cycle 24.
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- Proceedings of the International Astronomical Union, 2017, v. 13, n. S335, p. 32, doi. 10.1017/S1743921317008924
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Hard X-Ray Emission of Solar Flares Measured by Lomonosov Space Mission.
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- Proceedings of the International Astronomical Union, 2017, v. 13, n. S335, p. 29, doi. 10.1017/S1743921317008821
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The Belgian Space Weather Observatory in Dourbes.
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- Proceedings of the International Astronomical Union, 2017, v. 13, n. S335, p. 355, doi. 10.1017/S1743921317008353
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PFSS-Based Solar Wind Forecast and the Radius of the Source-Surface.
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- Proceedings of the International Astronomical Union, 2017, v. 13, n. S335, p. 307, doi. 10.1017/S1743921317009875
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Forecasting Solar Energetic Particle Fluence with Multi-Spacecraft Observations.
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- Proceedings of the International Astronomical Union, 2017, v. 13, n. S335, p. 298, doi. 10.1017/S1743921317008936
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Electron Acceleration in Collapsing Magnetic Traps during the Solar Flare on July 19, 2012: Observations and Models.
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- Proceedings of the International Astronomical Union, 2017, v. 13, n. S335, p. 90, doi. 10.1017/S1743921317008912
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Comparison and Time Evolution of the Geomagnetic Cutoff at the ISS Position: Internal vs External Earth's Magnetic Field Models.
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- Proceedings of the International Astronomical Union, 2017, v. 13, n. S335, p. 105, doi. 10.1017/S1743921317009863
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The Relationship between Long-Duration Gamma-Ray Flares and Solar Cosmic Rays.
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- Proceedings of the International Astronomical Union, 2017, v. 13, n. S335, p. 49, doi. 10.1017/S1743921317009681
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