Not exact matches
The mean insolation at Earth orbit is about 1366 W / m ^ 2; the peak - to - peak variation
over the 11 year
solar cycle is about 3 W / m ^ 2; the authors discuss two running averages derived from different satellite
data sets and analysis derived by Willson and Mordvinov (2003) and Frohlich and Lean (1998) respectively.
I mean since there is no clear trend (upward or downward) in cosmic ray flux
over the period we've been able to measure them directly; and since we do not see a significant difference in climate
over the 11 year
solar cycle between Solar Max and Solar Min (and this modulation is much larger than the one Svensmark is talking about); and since it is not clear how important the ionization from GCR is in cloud formation; and since the anthropogenic ghg mechanism does just fine reproducing the data, exactly how do you foresee implementing this «effect&ra
solar cycle between
Solar Max and Solar Min (and this modulation is much larger than the one Svensmark is talking about); and since it is not clear how important the ionization from GCR is in cloud formation; and since the anthropogenic ghg mechanism does just fine reproducing the data, exactly how do you foresee implementing this «effect&ra
Solar Max and
Solar Min (and this modulation is much larger than the one Svensmark is talking about); and since it is not clear how important the ionization from GCR is in cloud formation; and since the anthropogenic ghg mechanism does just fine reproducing the data, exactly how do you foresee implementing this «effect&ra
Solar Min (and this modulation is much larger than the one Svensmark is talking about); and since it is not clear how important the ionization from GCR is in cloud formation; and since the anthropogenic ghg mechanism does just fine reproducing the
data, exactly how do you foresee implementing this «effect»?
A linear regression fit to your smoothed
data in the graph sampled every 3 years or so gives a downward trend with a value of about 7 % of the size of a
solar cycle over the 40 - year span observed.
The mean insolation at Earth orbit is about 1366 W / m ^ 2; the peak - to - peak variation
over the 11 year
solar cycle is about 3 W / m ^ 2; the authors discuss two running averages derived from different satellite
data sets and analysis derived by Willson and Mordvinov (2003) and Frohlich and Lean (1998) respectively.
Similar conclusions were reached by Agee et al. (2012), who examined ISCCP
data over the recent
solar minimum (between
solar cycles 23 and 24), during which time high levels of CR were recorded, and yet no corresponding cloud changes were observed to suggest a connection to
solar activity.