Miscellaneous

19 January 2009 - A few weeks ago, the Royal Meteorological Institute of Belgium (RMI) published the results of its study on the climate evolution in Belgium. "Eye on the Climate" covers the period 1833-2007 and is a well-balanced and thorough report on the various climate parameters and the possible factors that can influence the climate in Belgium. There does not seem to be an English version of this report, but it is highly recommended to take that French dictionary and read the entire text!

Probably the most important conclusions concerning the weather parameters are:

Most important remarks concerning the climate factors are:

On climate models:

New topics (at least to me):


Evolution of polar faculae number: Observed vs. Seeing-corrected

The polar faculae (PF) I observed the last 10 years were done from 2 different locations: From mid-1996 till mid-2000 from Texas, USA (average seeing Q=4), and for the other years from Belgium (average seeing Q=3). The number of PF seen is heavily influenced by the seeing. This is readily apparent when determining the ratio R between PF as deduced from SOHO-images with my own PF-numbers for a certain Q-value (see table underneath).

Best fit is found for the formula R = (Q-2,15)/(Q-2,85). It was decided to rescale the observed PF-numbers in order to get comparable values where Q = 3,5 all the time, i.e. PF-numbers where Q > 3,5 will be reduced, and PF-numbers where Q < 3,5 get increased. This however resulted in overcorrections during the wintermonths of 2000-2003 in Belgium, where average seeing approaches 2,85 (correction approaches infinity!). For the smoothed period May 2000 - August 2003, R = (Q-2)/(Q-2,7) was applied. The 2,7-limit gives more margin during the Belgian wintermonths, but keeping at the same time a good fit with the ratio SOHO / JJ. The original and seeing-adjusted PF-evolution can be found underneath.

It may be clear that the current PF-numbers are steadily increasing, but are still far from the activity-levels during the previous solar cycle. This implies that solar minimum may be further away than is general believed (2007 in stead of late 2006), or the PF-maximum may be lower than the previous maximum, which -according to the solar dynamo model- could mean that the upcoming solar cycle may be lower than SC23.

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