Description: Theoretical light curve of the 1999 total solar eclipse. The model includes a fit of the middle-edge variation of the visual intensity of the apparent solar disk. The brightness during totality is set to approx. 1/20000 of the full sunlight, the observed brightness during totality.
Source: Theoretical model calculated with own software and plotted with Gnuplot
Beschreibung: Theoretische Lichtkurve der Sonnenfinsternis 1999 durch numerische Integration der Leuchtintensität der partiell bedeckten Sonnenscheibe. Helligkeit in relativen Einheiten der unverdeckten Sonnenhelligkeit L0. Helligkeit in der Totalität auf 1/20000 gesetzt, gemäß verschiedener Amateurbeobachtungen.
Quelle: Selbst erzeugt mit Gnuplot und eigener Software
Permission is granted to copy, distribute and/or modify this document under the terms of the GNU Free Documentation License, Version 1.2 or any later version published by the Free Software Foundation; with no Invariant Sections, no Front-Cover Texts, and no Back-Cover Texts. A copy of the license is included in the section entitled GNU Free Documentation License.http://www.gnu.org/copyleft/fdl.htmlGFDLGNU Free Documentation Licensetruetrue
to share – to copy, distribute and transmit the work
to remix – to adapt the work
Under the following conditions:
attribution – You must give appropriate credit, provide a link to the license, and indicate if changes were made. You may do so in any reasonable manner, but not in any way that suggests the licensor endorses you or your use.
share alike – If you remix, transform, or build upon the material, you must distribute your contributions under the same or compatible license as the original.
This licensing tag was added to this file as part of the GFDL licensing update.http://creativecommons.org/licenses/by-sa/3.0/CC BY-SA 3.0Creative Commons Attribution-Share Alike 3.0truetrue
Captions
Add a one-line explanation of what this file represents