La penombra nell'eclissi lunare e la Limb Darkening Function del Sole
Abstract
The penumbral zone during a lunar eclipse is determined by the solar Limb Darkening Function convoluted with the Earth's profile. The convolution integral is presented and a graphical solution obtained exploiting the penumbral zone cast by the solar disk with its LDF and an infinite border, present in a photo realized in purpose.
- Publication:
-
Gerbertvs, International Academic Publication on History of Medieval Science
- Pub Date:
- December 2019
- Bibcode:
- 2019Gerb...12...75S
- Keywords:
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- Penumbra;
- Lunar eclipses;
- Solar Limb Darkening Function