Add to ORKGThe objective of this investigation is to open a new window into the solar dynamo, convection, and magnetic reconnection through measurement of the helicity density of magnetic fields in the photosphere and tracing of large-scale patterns of magnetic helicity in the corona
Active regions on the solar surface are known to possess magnetic helicity, which is predominantly n...
The defining physical property of the Sun's corona is that the magnetic field dominates the plasma. ...
By defining an appropriate field line helicity, we apply the powerful concept of magnetic helicity t...
International audienceMounting observational evidence of the emergence of twisted magnetic flux tube...
Aims. The origin and evolution of the magnetic helicity in the solar corona are not well understood....
Magnetic helicity quantifies how the magnetic field is sheared and twisted compared to its lowest en...
A complete understanding of the physical mechanisms responsible for the solar magnetic field is yet ...
Two of the most widely observed and striking features of the Suns magnetic field are coronal loops, ...
Aims. The origin and evolution of the magnetic helicity in the solar corona are not well understoo...
The Sun, by the virtue of its proximity to Earth, serves as an excellent astrophysical laboratory fo...
The dynamics of the solar corona are dominated by the magnetic field which creates its structure. Th...
Abstract. Concept of magnetic/current helicity was introduced to solar physics about 15 years ago. E...
The central challenge in solar/heliospheric physics is to understand how the emergence and transport...
The mean value of the normalized current helicity in solar active regions is on the order of 1e-8 1/...
We demonstrate that conservation of global helicity plays only a minor role in determining the natur...
Active regions on the solar surface are known to possess magnetic helicity, which is predominantly n...
The defining physical property of the Sun's corona is that the magnetic field dominates the plasma. ...
By defining an appropriate field line helicity, we apply the powerful concept of magnetic helicity t...
International audienceMounting observational evidence of the emergence of twisted magnetic flux tube...
Aims. The origin and evolution of the magnetic helicity in the solar corona are not well understood....
Magnetic helicity quantifies how the magnetic field is sheared and twisted compared to its lowest en...
A complete understanding of the physical mechanisms responsible for the solar magnetic field is yet ...
Two of the most widely observed and striking features of the Suns magnetic field are coronal loops, ...
Aims. The origin and evolution of the magnetic helicity in the solar corona are not well understoo...
The Sun, by the virtue of its proximity to Earth, serves as an excellent astrophysical laboratory fo...
The dynamics of the solar corona are dominated by the magnetic field which creates its structure. Th...
Abstract. Concept of magnetic/current helicity was introduced to solar physics about 15 years ago. E...
The central challenge in solar/heliospheric physics is to understand how the emergence and transport...
The mean value of the normalized current helicity in solar active regions is on the order of 1e-8 1/...
We demonstrate that conservation of global helicity plays only a minor role in determining the natur...
Active regions on the solar surface are known to possess magnetic helicity, which is predominantly n...
The defining physical property of the Sun's corona is that the magnetic field dominates the plasma. ...
By defining an appropriate field line helicity, we apply the powerful concept of magnetic helicity t...