Satgen 555 Track RS13 SubHorizon by GM4IHJ (BID SGEN555) 1999-11-13 While the present rise in solar output does not seem likely to reach the heights attained in the previous cycle 88/89 ( Sunspots 150, Solar Flux 200)). Results so far in respect of subhorizon access to satellite RS13, have been good enough to suggest that we are going to have an interesting northern hemispheres winter DX. But if you are to get good results, you have to be lucky, and you have to be able to appreciate how the gradual daily shift west of RS13s orbit plane , affects when and where ,you hear the satellite and, who you may be able to contact through it. As regards operating technique, CW is king. Meaningful SSB qsos are all but impossible presently, and this will not improve unless there is a marked increase in solar flux. There are 3 reasons for this CW only, statement at the moment. Firstly signals coming from subhorizon locations are rarely if ever tone 9. T1 or T2 signals are much more the daily fare at this time. Secondly signal propagation is highly variable. For example recent reception from RS13 when it was south of Adelaide in Australia , was doppler shifting 150 Hz in just over 1 minute, then jumping back 150 Hz and staring the downward doppler drift all over again. Experience in previous solar cycles suggests this is a feature caused by the marginal solar flux. In previous cycles the signals have been much less disturbed. However if the solar flux does improve, the third problem will get worse. Mornings on 29.46 to 29.5 searching for signals are already being shattered by Russian FMers. Whilst afternoons are being blasted by FMing Gs , EAs, DLs, 9H1s , Ws and VEs. None of whom have ever heard of band plans. But all is not lost provided you can second guess where the signals will be propagating from, get on a narrow band filter and screen out much of the QRM. Then given RS13s westward shift this has meant, signals in early October afternoons utc coming to GM from the Easter North Pacific. By end October these afternoon contacts were fom the North West Pacific , and now in mid November, they are coming from the Indian Ocean, unfortunately hopelessly disturbed as they pass west of Perth Australia going north. Here in Scotland the winter days are getting shorter and shorter. Dawn is around 0800 and sunset is around 1600, but in spite of this the DX comes in even when RS is flying over the the night side of earth beyond the terminator. RS can get at least 3000 kms into the night side and still see the underside of a sunlit ionosphhere. So no one should be surprised by predawn or post sunset contacts . Indeed whilst discussing the solar terminator it is worth pointing out that for reasons which are not at all clear , RS13 sometimes tracks across antarctica in silence until it crosses the terminator into the night side heading east. It then quite often begins to put good signals into GM with very little distortion for several minutes. A trick which can occur on up to 3 successive orbits. Unfortunately these good signals have a disasterous habit of disappearing completely just before the satellite reaches VK or ZL. Please note however that doppler shift on these signals usually suggests that they are coming by non great circle paths.