© 2016. The American Astronomical Society. All rights reserved.. Solar activity undergoes a variation over timescales of several months known as Rieger-type periodicity, which usually occurs near maxima of sunspot cycles. An early analysis showed that the periodicity appears only in some cycles and is absent in other cycles. But the appearance/absence during different cycles has not been explained. We performed a wavelet analysis of sunspot data from the Greenwich Royal Observatory and the Royal Observatory of Belgium during cycles 14-24. We found that the Rieger-type periods occur in all cycles, but they are cycle dependent: shorter periods occur during stronger cycles. Our analysis revealed a periodicity of 185-195 days during the weak cy...
The solar dynamo is the exotic dance of the sun's two major magnetic field components, the poloidal ...
Aims. Studying the long term evolution of the solar acoustic oscillations is necessary for understan...
Aims. Studying the long term evolution of the solar acoustic oscillations is necessary for understan...
Solar activity undergoes a variation over timescales of several months known as Rieger-type periodic...
Context. Total solar irradiance allows for the use of the Sun as a star for studying observations of...
Eleven-year Schwabe cycle in solar activity is not yet fully understood despite of its almost two ce...
Context. Total solar irradiance allows for the use of the Sun as a star for studying observations of...
Context. A Rieger-type periodicity of 150–180 days (six to seven times the solar rotation period) ha...
Context. A Rieger-type periodicity of 150–180 days (six to seven times the solar rotation period) ha...
Helioseismic data have revealed a 1.3-year periodicity in the solar rotation rate near the bottom of...
Helioseismic data have revealed a 1.3-year periodicity in the solar rotation rate near the bottom of...
International audienceTwo fundamental properties of stellar magnetic fields have been determined by ...
The Rieger periods are solar cycles with a time scale of months, which are present in both flaring a...
Context. Solar magnetic activity exhibits variations with periods between 1.5 and 4 years, the so-ca...
Several recent studies utilizing different helioseismic methods have confirmed the presence of large...
The solar dynamo is the exotic dance of the sun's two major magnetic field components, the poloidal ...
Aims. Studying the long term evolution of the solar acoustic oscillations is necessary for understan...
Aims. Studying the long term evolution of the solar acoustic oscillations is necessary for understan...
Solar activity undergoes a variation over timescales of several months known as Rieger-type periodic...
Context. Total solar irradiance allows for the use of the Sun as a star for studying observations of...
Eleven-year Schwabe cycle in solar activity is not yet fully understood despite of its almost two ce...
Context. Total solar irradiance allows for the use of the Sun as a star for studying observations of...
Context. A Rieger-type periodicity of 150–180 days (six to seven times the solar rotation period) ha...
Context. A Rieger-type periodicity of 150–180 days (six to seven times the solar rotation period) ha...
Helioseismic data have revealed a 1.3-year periodicity in the solar rotation rate near the bottom of...
Helioseismic data have revealed a 1.3-year periodicity in the solar rotation rate near the bottom of...
International audienceTwo fundamental properties of stellar magnetic fields have been determined by ...
The Rieger periods are solar cycles with a time scale of months, which are present in both flaring a...
Context. Solar magnetic activity exhibits variations with periods between 1.5 and 4 years, the so-ca...
Several recent studies utilizing different helioseismic methods have confirmed the presence of large...
The solar dynamo is the exotic dance of the sun's two major magnetic field components, the poloidal ...
Aims. Studying the long term evolution of the solar acoustic oscillations is necessary for understan...
Aims. Studying the long term evolution of the solar acoustic oscillations is necessary for understan...