Biblio
Found 55 results
Filters: Keyword is Astrophysics - Solar and Stellar Astrophysics [Clear All Filters]
Evidence for a Coronal Shock Wave Origin for Relativistic Protons Producing Solar Gamma-Rays and Observed by Neutron Monitors at Earth,
, Astrophys. J., Volume 893, p.76, (2020)
Impact of solar magnetic field amplitude and geometry on cosmic rays diffusion coefficients in the inner heliosphere,
, Journal of Space Weather and Space Climate, Volume 10, p.55, (2020)
Low Geo-Effectiveness of Fast Halo CMEs Related to the 12 X-Class Flares in 2002,
, Journal of Geophysical Research (Space Physics), Volume 125, p.e27529, (2020)
Modeling the Early Evolution of a Slow Coronal Mass Ejection Imaged by the Parker Solar Probe,
, Astrophys. J. Suppl., Volume 246, p.72, (2020)
Multi-scale observations of thermal non-equilibrium cycles in coronal loops,
, Astron. Astrophys., Volume 633, p.A11, (2020)
Relating Streamer Flows to Density and Magnetic Structures at the Parker Solar Probe,
, Astrophys. J. Suppl., Volume 246, p.37, (2020)
Spectroscopic detection of coronal plasma flows in loops undergoing thermal non-equilibrium cycles,
, Astron. Astrophys., Volume 634, p.A54, (2020)
Comprehensive Determination of the Hinode/EIS Roll Angle,
, Solar Phys., May, Volume 294, p.59, (2019)
Elemental composition in quiescent prominences,
, Astron. Astrophys., May, Volume 625, p.A52, (2019)
Feature Ranking of Active Region Source Properties in Solar Flare Forecasting and the Uncompromised Stochasticity of Flare Occurrence,
, Astrophys. J., Volume 883, p.150, (2019)
Flare forecasting and feature ranking using SDO/HMI data,
, Nuovo Cimento C Geophysics Space Physics C, Volume 42, p.30, (2019)
Measuring relative abundances in the solar corona with optimised linear combinations of spectral lines,
, Astron. Astrophys., Dec, Volume 632, p.A20, (2019)
Searching for g modes. II. Unconfirmed g-mode detection in the power spectrum of the time series of round-trip travel time,
, Astron. Astrophys., Apr, Volume 624, p.A106, (2019)
Which Photospheric Characteristics Are Most Relevant to Active-Region Coronal Mass Ejections?,
, Solar Phys., Volume 294, p.130, (2019)
Active Region Photospheric Magnetic Properties Derived from Line-of- Sight and Radial Fields,
, Solar Phys., Volume 293, (2018)
Connecting Coronal Mass Ejections to Their Solar Active Region Sources: Combining Results from the HELCATS and FLARECAST Projects,
, Solar Phys., Apr, Volume 293, p.60, (2018)
The Coronal Monsoon: Thermal Nonequilibrium Revealed by Periodic Coronal Rain,
, Astrophys. J., Volume 853, (2018)
Forecasting Solar Flares Using Magnetogram-based Predictors and Machine Learning,
, Solar Phys., Volume 293, (2018)
IRIS Observations of Spicules and Structures Near the Solar Limb,
, Solar Phys., Volume 293, (2018)
On the Occurrence of Thermal Nonequilibrium in Coronal Loops,
, Astrophys. J., Volume 855, (2018)
Photospheric Shear Flows in Solar Active Regions and Their Relation to Flare Occurrence,
, Solar Phys., Volume 293, p.114, (2018)
Searching for g modes. I. A new calibration of the GOLF instrument,
, Astron. Astrophys., Volume 617, p.A108, (2018)
Statistical Analysis of Solar Events Associated with Storm Sudden Commencements over One Year of Solar Maximum During Cycle 23: Propagation from the Sun to the Earth and Effects,
, Solar Phys., Volume 293, (2018)
Testing and Improving a Set of Morphological Predictors of Flaring Activity,
, Solar Phys., Volume 293, p.96, (2018)
Asymptotic g modes: Evidence for a rapid rotation of the solar core,
, Astron. Astrophys., Volume 604, (2017)