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Wednesday, March 2, 2016

MONITORING RESEARCH

 
MONITORING RESEARCH
 
Solar Activity continues to remain at a very low level, which means that long-haul, multi-hop propagation over darkness or semi-darkness paths will be unreliable on frequencies above about 14 MHz.
 
The 9, 11 and 13 MHz spectrum is now heavily congested, and this summary of notable observed frequency occupancies in Melbourne in the pre-sunrise window on March 1, 2016 reflects high channel usage in the 1930 to 2000 period.
 
9360 TAIWAN SOH Chinese
9380 INDIA nat network
9390 THAILAND R. Thailand Udon English
9400 FRANCE R. Denge Kurdistane, Issoudun, Kurdish
9420 GREECE VOG Greek
9425 N. KOREA German
9440 CHINA CRI-Kunming English
9470 BOTSWANA VOA Kirundi
9515 GERMANY VOA-Lampertheim Kurdish
9525 INDONESIA English
9555 S. ARABIA Arabic
9590 SAO TOME VOA French
9660 VATICAN VR-SMG Latin Liturgy
9675 S. ARABIA Turkish
9690 SPAIN Spanish
9700 THAILAND VOA-Udorn Korean
9745 CHINA CRI-Urumqi Esperanto
9755 VATICAN VR-SMG Latin Liturgy
9895 UAE RTI-Dhabbaya French
 
11530 SPAIN Spanish
11660 ASCENSION Hausa
11670 INDIA English
11710 INDIA English/French
11775 FRANCE RTA-Issoudun Arabic
11810 ASCENSION BBC English
11820 S. ARABIA Arabic
11860 S. ARABIA R. Sanna, Arabic
11915 S. ARABIA Arabic
11930 S. ARABIA Arabic
11985 FRANCE RTA-Issoudun Arabic
11995 FRANCE RFI-Issoudun French
 
13640 INDIA Arabic/French
13695 INDIA English to 1945*

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