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Coronal hole
Cmes, Solar Wind and Sun-Earth Connections: Unresolved Issues
Coronal Holes
Lectures 6, 7 and 8 October 8, 10 and 13 the Heliosphere
Waves and Magnetism in the Solar Atmosphere (WAMIS)
Automated Coronal Hole Identification Via Multi-Thermal Intensity
Arxiv:2101.06279V2 [Astro-Ph.SR] 3 Mar 2021 N H Rtecutro S Ihtesn Nnvme 2018, November in D Sun, Question
What Do We See on the Face of the Sun? Lecture 3: the Solar Atmosphere the Sun’S Atmosphere
Statistical Analysis and Catalog of Non-Polar Coronal Holes Covering
NASA Heliophysics: the Science of Space Weather!
UNDERSTANDING SPACE WEATHER Part III: the Sun’S Domain
Arxiv:1903.12613V1 [Astro-Ph.SR] 29 Mar 2019 4 Air Force Research Laboratory/Space Vehicles Directorate, Kirtland Air Force Base, NM, 87117, USA
The Sun's Mysteries from Space - II
Comparing Different Methods for Estimating Total Open Heliospheric Magnetic Flux
Areas of Polar Coronal Holes from 1996 Through 2010
Arxiv:1708.07169V1 [Astro-Ph.SR] 23 Aug 2017 Rdciesineic,99 Earmra,Sie10 a D San 170, Suite Road, Rim Mesa 9990 Inc., Science Predictive Riley P
Determination of Coronal Temperatures from Electron Density Profiles
Comparison of the Scaling Properties of EUV Intensity Fluctuations in Coronal Hole and Quiet-Sun Regions
The 3-D Sun and Heliosphere at Solar Maximum
Top View
Alert of Severe Earthquakes Worldwide Due to Solar Forcing of Very Weak Solar Cycle 24
Differences Between a Polar Coronal Hole and Its Equatorial Extension
Relationship Between the Low-Latitude Coronal Hole Area, Solar Wind
WHPI Solar Minimum Study
Coronal Expansion and Solar Wind
Arxiv:1712.03042V2 [Astro-Ph.SR] 28 Jan 2018
In Situ Analysis of Heliospheric Current Sheet Propagation 10.1002/2017JA024194 Jun Peng1,2 , Yong C.-M
Center for Astrophysics Harvard Collegr, Observatory and Smithsonhn Astrophysical Observatory Cambridge, Massachusetts 02 138
Solar Corona:Open Questions D H Th “S L O Bit “ Solar
Coronal Hole Boundaries Evolution at Small Scales III
Sun-To-Earth Propagation of the 2015 June 21 Coronal Mass Ejection Revealed by Optical, EUV, and Radio Observations
Dear Science Educator: Because of Its Relationship to the Sun, Solar
Ncomms8135.Pdf
Improvements on Coronal Hole Detection in SDO/AIA Images Using Supervised Classification
Arxiv:2104.04417V2 [Astro-Ph.SR] 10 Aug 2021
Multi-Channel Coronal Hole Detection with Convolutional Neural Networks? R
The Structure and Dynamics of the Corona – Heliosphere Connection
Coronal Hole Boundaries Evolution at Small Scales*
Solar Wind and Kinetic Heliophysics
Equatorial Coronal Holes and Their Relation to the High-Speed Solar Wind Streams
Heliophysics I
Correlation Between Coronal Hole and Quiet Sun Intensities: Evidence for Continuous Reconnection
The Low Solar Corona and the Stars N
Observations of the Sun's Magnetic Field During the Recent Solar Maximum
Coronal Heating and Energetics
The Spatial Relationship Between Active Regions and Coronal Holes and the Occurrence of Intense Geomagnetic Storms Throughout the Solar Activity Cycle S
History and Development of Coronal Mass Ejections As a Key Player in Solar Terrestrial Relationship N
Cosmic-Ray Picture of the Heliosphere
STEREO Observations of Interplanetary Coronal Mass Ejections and Prominence Deflection During Solar Minimum Period
Inner Heliospheric Evolution of a ”Stealth” CME Derived from Multi-View Imaging and Multipoint In–Situ Observations: I
The Solar Magnetic Activity Band Interaction and Instabilities That Shape Quasi-Periodic Variability
The Solar Corona at Totality
Sensitivity of Solar Wind Mass Flux to Coronal Temperature
19810024570.Pdf
Solar Wind Originating in Funnels: Fast Or Slow?
Introduction Modeling Heliospheric Current Sheet Modeling Coronal
Solar Corona, Solar Wind Structure and Solar Particle Events
The Structure of the Sun
Solar Wind and Interplanetary Disturbances
Physics of Space Weather Phenomena: a Review
Coronal Holes and High Speed Streams
The Properties of the Solar Corona and Its Connection to the Solar Wind
A Statistical Study of the Long-Term Evolution of Coronal Hole Properties As Observed by SDO S
Photospheric Magnetic Structure of Coronal Holes? Stefan J
Coronal Holes and Swx
Factors Affecting the Intensity of Solar Energetic Particle Events
Coronal Holes and Swx
SEARCH: Segmentation of Polar Coronal Holes
Lecture 6: Coronal Heating and Flares the Hot Corona: a Brief History
Historical Space Weather Forecasts and Synoptic Drawings Now
Plasmoid Releases in the Heliospheric Current Sheet and Associated Coronal Hole Boundary Layer Evolution