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 Mees Solar Obs., Haleakala, HI, USA J. Pasachoff, B. Babcock, Muzhou Lu B (450 nm)
2 Mobile station, Hokkaido, Japan N. Thouvenin, M. Imai, T. Fukuhara V (535 nm)
3 Moondara Obs., Mount Isa, QLD, Australia F. Braga-Ribas, L. Fulham I (760 nm)
4 Tien Shan Obs., Kazakhstan F. Colas, F. Vachier B
5 Lowell Obs., AZ, USA W. Sheehan V
6 Lowell Obs., AZ, USA P. Tanga V
7 Taiohae, Nuku Hiva, Marquesas Is. C. Veillet R (607 nm)
8 Mobile station, Svalbard Is., Norway J. Berthier, T. Widemann I
9 Udaipur Obs., India P. Machado, A. Ambastha R
All filters have a 10 nm FWHM. "R" and "V" correspond to SODISM filters (on Picard) while "I" is similar to one of the filters for the HST observations.

Additional sites, with their own instruments:
A Khurel Togoot Obs., Ulaanbaatar, Mongolia S. Bouley, L. Maquet  
B Hauriou solar station, China C. Sigismondi  
Topic revision: r15 - 03 Jul 2012, PaoloTanga
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