KnowraSolar magnetic fieldLinked fromLinked fromThe 17 pages that link to Solar magnetic field, each with the reason it gives.All 17Broader topic 2Related 11Narrower topic 4Solar cycleRelated: Its deep structure and evolution cannot be measured directly, limiting cycle theory.Fraunhofer linesRelated: Magnetic fields split and polarize selected spectral lines through the Zeeman effect.SunspotRelated: Concentrated magnetic fields in sunspots hinder the upward flow of hot plasma.Solar prominenceNarrower topic: Its structure provides the forces that suspend and shape prominence material.HelioseismologyRelated: Magnetic forces alter wave propagation, complicating the interpretation of oscillations in active regions.George Ellery HaleNarrower topic: Hale’s observations established that sunspots are sites of strong solar magnetism.Coronal heating problemRelated: Magnetic energy is a leading candidate source for heating the corona.Interplanetary magnetic fieldNarrower topic: The interplanetary field is the outward-carried portion of this larger solar field.Stellar magnetic fieldBroader topic: The Sun provides the best-observed example of a stellar magnetic field.Solar physicsRelated: Its changing configurations govern much of the Sun’s visible activity.Solar stormNarrower topic: Stored and rearranged magnetic energy powers flares and many coronal mass ejections.HeliophysicsRelated: Its changing structure powers flares, coronal mass ejections, and the solar cycle.Astrophysical electromagnetic fieldsBroader topic: Its changing structure drives sunspots, flares, and much of solar-wind behavior.Hale's lawRelated: Its large-scale polarity reverses along with the orientation specified by Hale’s law.Polarization in astronomyRelated: Solar spectropolarimetry infers its strength and orientation from Zeeman-sensitive signals.Solar activity and climateRelated: Its changing structure underlies solar cycles and many proposed climate pathways.Solar phenomenaRelated: Its changing structure drives many active regions and eruptions.
KnowraSolar magnetic fieldLinked fromLinked fromThe 17 pages that link to Solar magnetic field, each with the reason it gives.All 17Broader topic 2Related 11Narrower topic 4Solar cycleRelated: Its deep structure and evolution cannot be measured directly, limiting cycle theory.Fraunhofer linesRelated: Magnetic fields split and polarize selected spectral lines through the Zeeman effect.SunspotRelated: Concentrated magnetic fields in sunspots hinder the upward flow of hot plasma.Solar prominenceNarrower topic: Its structure provides the forces that suspend and shape prominence material.HelioseismologyRelated: Magnetic forces alter wave propagation, complicating the interpretation of oscillations in active regions.George Ellery HaleNarrower topic: Hale’s observations established that sunspots are sites of strong solar magnetism.Coronal heating problemRelated: Magnetic energy is a leading candidate source for heating the corona.Interplanetary magnetic fieldNarrower topic: The interplanetary field is the outward-carried portion of this larger solar field.Stellar magnetic fieldBroader topic: The Sun provides the best-observed example of a stellar magnetic field.Solar physicsRelated: Its changing configurations govern much of the Sun’s visible activity.Solar stormNarrower topic: Stored and rearranged magnetic energy powers flares and many coronal mass ejections.HeliophysicsRelated: Its changing structure powers flares, coronal mass ejections, and the solar cycle.Astrophysical electromagnetic fieldsBroader topic: Its changing structure drives sunspots, flares, and much of solar-wind behavior.Hale's lawRelated: Its large-scale polarity reverses along with the orientation specified by Hale’s law.Polarization in astronomyRelated: Solar spectropolarimetry infers its strength and orientation from Zeeman-sensitive signals.Solar activity and climateRelated: Its changing structure underlies solar cycles and many proposed climate pathways.Solar phenomenaRelated: Its changing structure drives many active regions and eruptions.