We investigate the nature of monthly sunspot numbers and solar flux F10.7 by employing the linear and multiple regression techniques. We observed a brilliant correlation between monthly mean sunspot number and F10.7. We observed that even in deep solar minimum there exist some magnetic activities. We obtained the coefficient of determination R2 to be 0.9533. We estimated the correlation coefficient for solar flux F10.7 and sunspot number to be 0.97. We extrapolated the F10.7 back to the year 1700 and observed a good correspondence between the modelled F10.7 and sunspot nature. We also found a very good correspondence between the modelled and observed solar flux F10.7
Here, we compare the sunspot counts and the number of sunspot groups (SGs) with variations of tot...
The Sun shows a global magnetic field cycle traditionally best visible in the photosphere as a chang...
In this study, the relationship between the monthly mean values of the Quasi Biennial Oscillation (Q...
We investigate the nature of monthly sunspot numbers and solar flux F10.7 by employing the linear an...
Abstract Background: Several recent studies indicated possible long‐term variations of physical prop...
It is shown that the monthly smoothed sunspot number (SSN) or its rate of decrease during the final...
The F10.7cm radio flux and the Sunspot Number are the most widely used long-term indices of solar ac...
A statistical study of formulas for predicting the sunspot number several years in advance is report...
Monthly averages of the Helsinki Ak-values have been reduced to the equivalent aa-indices to extend...
Power spectral densities computed from low-latitude horizontal intensity of the Earth's magnetic fie...
Here we study the prediction of even and odd numbered sunspot cycles separately, thereby taking into...
We analyze the monthly sunspot number (SSN) data from January 1749 to June 2013. We use the Average ...
We perform two statistical studies of monthly mean sunspots one of them by considering the Daubechie...
The Sun exhibits a well-observed modulation in the number of spots on its disk over a period of abou...
We analyze the yearly mean sunspot-number data covering the period 1700 to 2012. We show that the ye...
Here, we compare the sunspot counts and the number of sunspot groups (SGs) with variations of tot...
The Sun shows a global magnetic field cycle traditionally best visible in the photosphere as a chang...
In this study, the relationship between the monthly mean values of the Quasi Biennial Oscillation (Q...
We investigate the nature of monthly sunspot numbers and solar flux F10.7 by employing the linear an...
Abstract Background: Several recent studies indicated possible long‐term variations of physical prop...
It is shown that the monthly smoothed sunspot number (SSN) or its rate of decrease during the final...
The F10.7cm radio flux and the Sunspot Number are the most widely used long-term indices of solar ac...
A statistical study of formulas for predicting the sunspot number several years in advance is report...
Monthly averages of the Helsinki Ak-values have been reduced to the equivalent aa-indices to extend...
Power spectral densities computed from low-latitude horizontal intensity of the Earth's magnetic fie...
Here we study the prediction of even and odd numbered sunspot cycles separately, thereby taking into...
We analyze the monthly sunspot number (SSN) data from January 1749 to June 2013. We use the Average ...
We perform two statistical studies of monthly mean sunspots one of them by considering the Daubechie...
The Sun exhibits a well-observed modulation in the number of spots on its disk over a period of abou...
We analyze the yearly mean sunspot-number data covering the period 1700 to 2012. We show that the ye...
Here, we compare the sunspot counts and the number of sunspot groups (SGs) with variations of tot...
The Sun shows a global magnetic field cycle traditionally best visible in the photosphere as a chang...
In this study, the relationship between the monthly mean values of the Quasi Biennial Oscillation (Q...