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Thursday, March 1, 2018

Monitoring Analysis - 1730 to 1930

 
Solar Activity continues to remain  very low – no sunspots visible!
 
Despite this,  there is enough residual ionisation to support long-haul propagation into Melbourne during our pre-sunrise window on frequencies below about 12 MHz, dominated by short–path (darkness) from Asia, Europe, Africa and the Middle East.
 
This summary shows notable frequency usage as monitored on February 28, 2018, officially the last day of summer!
 
1730-1800
 
7240 CHINA Xizang PBS Lhasa Chinese
7300 CHINA CRI-Kashi Arabic
7360 VATICAN VR-SMG Ukrainian from *1740
7385 CHINA Xizang PBS Lhasa Tibetan
7395 SINGAPORE BBC Korean
7400 CHINA CRI-Xian Swahili
7410 CHINA CRI-Baoji Russian
7425 IRAN Arabic
7450 CHINA Xizang Lhasa Chinese
7460 TAIWAN SOH Chinese
7465 SINGAPORE BBC Dari
11750 SRI LANKA SLBC Sinhala
11760 GERMANY VOA-Lampertheim Kurdish
11790 GERMANY BVB-Nauen English
11945 FRANCE NHK-Issoudin Japanese
11985 GERMANY AWR-Nauen *1730 Kabyle
12040 THAILAND VOA-Udon Oromo
 
1900-1930
 
5900 BULGARIA BVB-Kostinbrod Arabic
5905 FRANCE RTA-Issoudin Arabic
5925 IRAN Arabic
5950 ETHIOPIA V. of Tigray Revolution, Tigrinya
5970 ALBANIA CRI-Cerrick French
5985 CHINA CRI-Beijing Portuguese
5990  ROMANIA RRI Romanian
5995 S. KOREA VOH Korean
6030 ETHIOPIA R. Oromiya Afar
6055 ALBANIA CRI-Cerrick French
6090 ETHIOPIA R. Amhara Amharic
6110 CHINA CRI-Xian Russian
6110 ETHIOPIA R. Fana Oromo (co-channel China)
6120 TURKEY Turkish
6130 SWAZILAND TWR-Manzini dialects
6160 CHINA CRI-Beijing German
6180 ROMANIA RRI German
 
 
 

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