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Sample pictures from Lowell Observatory (P. Tanga, W. Sheehan, K. Brausch, W. Burke, J. Roberts) Very good transparency, but bad seeing and wind disturbing the ob...
The Venus Twilight Experiment Refraction and scattering phenomena during the transit of Venus on June 5 6, 2012 Planetary transits are a powerful method for disc...
Test results Solar observation on 27/12/2011 : The three images below are the result of the addition of 20 images taken in a 2 second stream. Light wavelet proce...
Why a coronograph? We plan to image Venus when it is close to the solar limb, around the transit event occuring on June 5 6, 2012, when twilight phenomena become ...
Coronagraph placement Venus TEx Coronographs map here The following table indicates the sites, the observer(s) and the associated filters for each of them: 1 ...
Preparing coronagraphs and the transit 05.Jun.12 Kazakhstan expedition, coronagraph #4 Few hours of Transit somewhere in Kazakhstan (Observers : François Col...
Press conference in Paris On May 15th, scientists from OCA and OBSPM collaboration have given one last press conference at the Observatory of Paris. Starting wit...
Main.JenniferP 23 May 2012 In May 15th, scientists from OCA and OBSPM collaboration have given one last press conference at the Observatory of Paris. Starting wit...
The transit and related science Venus is one of the most intriguing bodies in the Solar System. It is almost the same size as the Earth and apparently has a simil...
Collaborators A tentative list, including observers and observing sites / instruments. Ashok Ambastha Udaipur Obs. India John Briggs HUT Observatory, C...
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Science team Paolo Tanga Laboratoire Lagrange, Observatoire de la Côte d'Azur, Nice, France Thomas Widemann LESIA UMR 8109, Observatoire de Paris / Université...
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