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