Add to ORKGAbstract We use Renewal Theory for the estimation and interpretation of the flare rate from the Geostationary Operational Environmental Satellite (GOES) soft X-ray flare catalogue. It is found, that in addition to the flare rate variability with the solar cycles, a much faster variation occurs. The fast variation on time scales of days and hours down to minute scale appears to be comparable with time intervals between two successive flares (waiting times). The detected fast non-stationarity of the flaring rate is discussed in the framework of the previously published stochastic models of the waiting time dynamics
<p>Solar flares are known to originate in sunspot groups, with increasingly complex magnetic structu...
The temporal recurrence of micro-flare events is studied in a time interval before and after of majo...
The nature of quasi-periodic pulsations (QPP) in solar flares is poorly constrained, and critically ...
Context. The existence of time-energy correlations in flare occurrence is still an open and much deb...
Context. The existence of time-energy correlations in flare occurrence is still an open and much deb...
We have recognized an anomaly on the solar activity cycle, while we researching on the question that...
In this paper we describe the statistical properties of the EUV solar flux sudden variation. The sol...
Extended version of the paperIn this paper we describe the statistical properties of the EUV solar ...
Introducing thresholds to analyze time series of emission from the Sun enables a new and simple defi...
Introducing thresholds to analyze time series of emission from the Sun enables a new and simple defi...
International audienceWaiting-time distributions of solar flares and coronal mass ejections (CMEs) e...
A statistical analysis of almost 50 000 soft X-ray (SXR) flares observed by GOES during the period 1...
The results of a statistical study of hard x-ray solar flares are presented in this dissertation. Tw...
Waiting-time distributions allow us to distinguish at least three different types of dynamical syste...
Energy incident from the Sun is the chief deriving force responsible for all physical process existi...
<p>Solar flares are known to originate in sunspot groups, with increasingly complex magnetic structu...
The temporal recurrence of micro-flare events is studied in a time interval before and after of majo...
The nature of quasi-periodic pulsations (QPP) in solar flares is poorly constrained, and critically ...
Context. The existence of time-energy correlations in flare occurrence is still an open and much deb...
Context. The existence of time-energy correlations in flare occurrence is still an open and much deb...
We have recognized an anomaly on the solar activity cycle, while we researching on the question that...
In this paper we describe the statistical properties of the EUV solar flux sudden variation. The sol...
Extended version of the paperIn this paper we describe the statistical properties of the EUV solar ...
Introducing thresholds to analyze time series of emission from the Sun enables a new and simple defi...
Introducing thresholds to analyze time series of emission from the Sun enables a new and simple defi...
International audienceWaiting-time distributions of solar flares and coronal mass ejections (CMEs) e...
A statistical analysis of almost 50 000 soft X-ray (SXR) flares observed by GOES during the period 1...
The results of a statistical study of hard x-ray solar flares are presented in this dissertation. Tw...
Waiting-time distributions allow us to distinguish at least three different types of dynamical syste...
Energy incident from the Sun is the chief deriving force responsible for all physical process existi...
<p>Solar flares are known to originate in sunspot groups, with increasingly complex magnetic structu...
The temporal recurrence of micro-flare events is studied in a time interval before and after of majo...
The nature of quasi-periodic pulsations (QPP) in solar flares is poorly constrained, and critically ...