> > the 8" telescope pointing opposite the max elevation azimuth > > and at a complementary elevation (23 deg). > > Why did you do that procedure? Perhaps you could explain it? > To be able to follow the object using RA motion (almost) solely. This was discussed in Feb., (and some times 1998 and 1999?) See: http://www2.satellite.eu.org/seesat/Feb-2000/0361.html http://www2.satellite.eu.org/seesat/Feb-2000/0364.html http://www2.satellite.eu.org/seesat/Feb-2000/0366.html http://www2.satellite.eu.org/seesat/Feb-2000/0367.html ... -- bjorn.gimle@tietotech.se (office) -- -- b_gimle@algonet.se (home) http://www.algonet.se/~b_gimle -- -- COSPAR 5919, MALMA, 59.2615 N, 18.6206 E, 33 m -- -- COSPAR 5918, HAMMARBY, 59.2985 N, 18.1045 E, 44 m -- -- SeeSat-L / Visual Satellite Observer Home Page found at -- -- http://www.satellite.eu.org/satintro.html -- ----------------------------------------------------------------- Unsubscribe from SeeSat-L by sending a message with 'unsubscribe' in the SUBJECT to SeeSat-L-request@lists.satellite.eu.org http://www2.satellite.eu.org/seesat/seesatindex.html
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