Action et activités de l'Académie du 1er mai 2005 au 31 avril 2006
In: Bulletin de la Classe des Beaux-Arts, Band 17, Heft 1, S. 227-239
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In: Bulletin de la Classe des Beaux-Arts, Band 17, Heft 1, S. 227-239
In: Bulletin de la Classe des Beaux-Arts, Band 14, Heft 1, S. 161-174
In: Bulletin de la Classe des lettres et des sciences morales et politiques, Band 12, Heft 1, S. 56-65
In: Bulletin de la Classe des Sciences de l'Académie Royale de Sciences, des Lettres et des Beaux-Arts de Belgique, Band 8, Heft 7, S. 349-365
In: Bulletin de la Classe des Sciences de l'Académie Royale de Sciences, des Lettres et des Beaux-Arts de Belgique, Band 1, Heft 1, S. 349-357
In: Bulletin de la Classe des sciences, Band 52, Heft 1, S. 202-228
In: Bulletin de la Classe des sciences, Band 51, Heft 1, S. 699-725
In: Bulletin de la Classe des sciences, Band 49, Heft 1, S. 356-361
In: Bulletin de la Classe des sciences, Band 45, Heft 1, S. 218-238
The possible sources of the continuous (solar) spectrum of comets are discussed. Four mechanisms are considered :
1) diffuse reflection by the solid nucleus (Lambert's Law) ;
2) scattering by molecules (Rayleigh) ;
3) scattering by small solid particles (Mie) ;
4) scattering by free electrons (Thomson).
It was found that the solar continuum of comets is due in most cases to scattering by small solid particles.
An attempt has also been made to determine the continuous spectrum of comet Arend-Roland by photographic spectrophotometry.
In: Bulletin de la Classe des sciences, Band 52, Heft 1, S. 947-968
In: Bulletin de la Classe des sciences, Band 43, Heft 1, S. 171-178
The authors tried to establish a correlation between solar flares and luminosity outbursts of five comets. No definite relationship was found between the variations of visual magnitudes observed by Beyer and the flares reported in the Quarterly Bulletin on Solar Activity. The examination of 75 spectra revealed a correlation only in one case. Finally it seems impossible to prove the existence of such a relationship as long as we have no long series of monochromatic light curves of comets.