|
Frequency Allocation Chart
U.S. and International RF spectrum allocations extending from 9 kHz to 300 GHz
The
Electromagnetic Spectrum
including a frequency-wavelength conversion utility.
Frequency-to-wavelength Conversion
Very Low and Low Frequency Radio Stations
|
Site
|
ID
|
Frequency (kHz)
|
Wavelength (meters)
|
Radiated Power (kW)
|
Royal Navy,
Gippsland, Woodside, Australia
|
VL3DEF
|
13.0000
|
|
|
Batumi, Russia
|
UVA
|
14.6000
|
|
100*
|
Vladivostok, Russia
|
UIK
|
15.0000
|
20,000.0000
|
100*
|
Rosnay, France
|
HWU
|
15.1000
|
|
400
|
Bombay, India
|
|
15.1000
|
|
|
Rugby, United Kingdom
|
GBR
|
16.0000
|
|
45
|
Noviken, Norway
|
JXN
|
16.4000
|
|
45
|
St. Assie, France
|
FTA
|
16.8000
|
|
23
|
Varberg Sweden (Grimeton Radio)
|
SAQ
|
17.2000
|
|
|
Cutler, Maine
|
|
17.8000
|
|
|
USN TACAMO mobile
worldwide
|
unidentified
|
17.9000
|
|
|
Matotchkinchar, Russia
|
UFQE
|
18.1000
|
|
100*
|
Katabomman, S.
Vijayanarayanam village, India
|
VTX3
|
18.2000
|
|
|
Rhauderfehn, Germany
|
|
18.5000
|
|
500
|
Anthorn, United Kingdom
|
GQD
|
19.0000
|
|
42
|
Arkhanghelsk, Russia
|
UGE
|
19.4000
|
|
150*
|
Criggons, United Kingdom
|
GBZ
|
19.6000
|
|
44
|
Harold E. Holt, Australia
|
NSW
|
19.8000
|
|
1000
|
Amundsen/Scott
South Pole base, Antarctic
|
unidentified
|
20.0000
|
15,000.0000
|
|
Isola di Tavolara, Italy
|
ICV
|
20.2700
|
|
43
|
Lualualei, Hawaii
|
NPM
|
21.4000
|
|
480/566
|
Ebino Huyshu, Japan
|
|
23.4000
|
|
|
Cutler, Maine
|
NAA
|
24.0000
|
|
1800
|
Jim Creek, Washington
|
NLK
|
24.8000
|
|
192/250
|
Various locations
|
RAB99, etc.
|
25.0000
|
12,000.0000
|
|
Omega Station,
LaMoure, North Dakota
|
|
25.4000
|
|
silent
|
VLF upper
limit, LF lower limit
|
|
30.0000
|
10,000.0000
|
|
Kaliningrad, Russia
|
UGKZ
|
30.3000
|
|
100*
|
|
|
35.0000
|
8571.4286
|
|
Keflavik, Iceland
|
NRK
|
37.5000
|
|
100
|
Niscemi, Italy
|
|
39.9000
|
|
25
|
Japan
|
JJY
|
40.0000
|
7,500.0000
|
50 kW
|
Aquada, Puerto Rico
|
NAU
|
40.7500
|
|
100
|
Irkutsk, Russia
(time standard)
|
RTZ
|
50.0000
|
6,000.0000
|
50 kW |
Ft. Collins
(time standard) |
WWVB
|
60.0000
|
5,000.0000
|
50 kW ERP
|
Rugby (time
standard)
|
MSF
|
60.0000
|
5,000.0000
|
|
Moscow |
RBU |
66.6700 |
|
|
|
|
70.0000 |
4285.7143 |
|
Aarjaeng,
Hamburgsund & Vallda, Sweden |
|
71.5830 |
|
30.8** |
Jomfruland, Norway |
|
71.5833 |
|
30.8** |
73 kHz Amateur
Radio Band - lower limit |
|
71.6000 |
4189.9441 |
|
Baku, Azerbaijan |
|
72.0000 |
|
43.0** |
St. Assise, France |
FTA72 |
72.1000 |
|
46.5** |
Kostinbrod,
Bulgaria |
LCI5 |
72.2000 |
|
41.1** |
Baku, Azerbaijan |
|
72.3000 |
|
43.0** |
Shmidta MYS, Russia |
|
72.3000 |
|
44.8** |
Chittagong,
Bangladesh |
|
72.5000 |
|
43.0** |
Karachi, Pakistan |
|
72.5000 |
|
43.0** |
Jeloey, Norway |
LCE |
72.8500 |
|
46.5** |
Ruiselede, Belgium |
ORL28 |
72.9000 |
|
40.0** |
Dutch Harbor,
Alaska |
|
73.2500 |
|
47.0** |
Kodiak, Alaska |
|
73.2500 |
|
46.0** |
Crimond, Scotland |
|
73.2500 |
|
46.0** |
Rugby, England |
MTO21 |
73.2500 |
|
46.0** |
Arkhangelsk, Russia |
UGE |
73.4000 |
|
41.8** |
Halifax, Nova Scotia |
CFH |
73.6000 |
|
54.0** |
Bombay, India |
|
73.6000 |
|
50.0** |
Deutsch Altnbg,
Austria |
|
73.8500 |
|
44.8** |
Crimond, Scotland |
|
74.2000 |
|
46.0** |
London, England |
GYD |
74.2000 |
|
40.0** |
Akkul, Kazakhstan |
|
74.2000 |
|
30.0** |
Petrozavodsk,
Russia |
|
74.4000 |
|
33.0** |
73 kHz Amateur
Radio Band - upper limit |
|
74.4000 |
4032.2581 |
|
Koenigswusterh,
Germany |
DKQ2 |
74.5000 |
|
43.0** |
Kalsborg, Sweden |
SAY |
74.5500 |
|
40.0** |
Varberg, Sweden |
SAY |
74.5500 |
|
47.0** |
Nyon or Prangins, Switzerland
(time standard)
|
HBG
|
75.0000
|
4,000.0000
|
|
Mainflingen, Germany
(time standard)
|
DCF77
|
77.5000
|
|
|
Loran-C navigation
system
|
|
100.0000
|
3,000.0000
|
|
|
|
108.0000
|
2777.7777
|
|
|
|
120.9000
|
|
|
Telekom Mainflingen
|
DCF42
|
123.7000
|
|
|
EFR Mainflingen
|
DCF49
|
129.1000
|
|
|
136 kHz Amateur
Radio Band - lower limit |
|
135.7000 |
2,210.7590 |
|
WA2XTF
|
|
136.7500
|
|
Inactive |
136 kHz Amateur
Radio Band - upper limit |
|
137.8000 |
2,177.0682 |
|
EFR Burg |
DCF39 |
139.0000 |
|
|
Hamburg Meteo |
DDH47 |
147.3000 |
|
|
|
|
157.1875 |
1908.5487 |
|
License
Free Expt. Band - lower limit |
|
160.0000 |
1,875.0000 |
|
Radio France
International,
Allouis
|
|
162..0000
|
|
|
|
|
171.4062
|
1750.2284
|
1* |
"Watering
Hole"
|
|
185.3000
|
|
1* |
License
Free Expt. Band - upper limit |
|
190.0000 |
1,578.9474 |
|
|
|
|
|
*Input
power
**dBW |
Sources: |
http://www.boulder.nist.gov/timefreq/stations/wwvb.htm
|
http://moondog.astro.louisville.edu/flares/stations.html
|
http://www.scnt01426.pwp.blueyonder.co.uk/Articles/MSF/MSF.htm
|
http://www-star.stanford.edu/~hail/stations/stations.html
|
http://www.geocities.com/CapeCanaveral/Hall/8701/73khz/services.htm
|
http://www.qsl.net/g4cnn/lf/lf.htm
|
http://www.vlf.it/trond2/below10.html |
http://www.vlf.it/trond2/10-15khz.html |
http://www.vlf.it/trond2/15-20khz.html |
http://www.vlf.it/trond2/20-25khz.html |
http://www.vlf.it/trond2/25-30khz.html |
FCC Declines to
Grant [the Requested 135.7-137.8 kHz] Amateur LF Allocation
Report
and Order
In evaluating whether amateur privileges should be added to the
135.7-137.8 kHz band the FCC considered the potential for interference
conflicts with Power Line Carrier (PLC) operations associated with the
national power grid.
Accordingly, the FCC declined to make the 135.7-137.8 kHz allocation
to the amateur service. The FCC acknowledges there is potential for some
limited operation under individual experimental licenses. Low Frequency
operations under the FCC experimental license program will allow amateur use
to be coordinated with utility companies on a case-by-case basis, and allow
empirical data to be developed on the sharing possibilities in this band for
future consideration. In addition, amateurs may still make use of the
160-190 kHz band under Part 15 rules, which are much more restrictive, and
therefore more protective of PLCs, than the limits proposed in the Notice.
Notice
of Proposed Rule Making (05/15/2002)
*
ARLB095:
ARRL Petitions FCC for LF Allocations *
ARRL Petition for Rule Making for LF Allocation for the Amateur
Radio Service
136
kHz Band Would Mark First LF Allocation for [U.S.] Hams
*
Low-Frequency
Experimental License Issued *
AMRAD
Low Frequency Web Page
AMRAD
Continues LF Experiments *
AMRAD LF
Experimenters' List Archive
CEPT draft recommendation on LF allocation to Radio
Amateurs
The
Amateur Service seeks a shared LF allocation *
The Longwave Club of America
— Promoting both DXing and experimentation on the frequencies below
550 kHz.
Simple
LowFER Transmitter -- by Lyle Koehler, KØLR
Three LF
Transmitters *
QRS
Ver 2.05 Download
136kHz at G3YMC
VK2ZTO
Experimentation Pages
Altair LF Beacon
YWK
BPSK
Receiver []
How
to Design a Class-E Transmitter for Your LowFER Beacon []
SM6LKM
Beacon, etc.
Build
a simple isolated impedance bridge for LF antennas
74HC4053
Longwave upconverter PIC controlled CW/BPSK beacon transmitter
Packet
Digital Amateur Network
— free software developed
for radio amateur's use, including Argo and Jason.
ON7YD
-- [Radio] Antennas for 136kHz
2.14.
Helical antenna
In the helical antenna the loading coil (or a part of it) is incorporated in
the vertical section of the antenna. So with this antenna both capacitance and
inductance are distributed over the entire antenna. As the antenna
voltage builds up over the loading coil, the antenna voltage increases
with the height. This voltage increase results in an improved current
distribution, as in the lower part of the antenna (where the voltage is
low) less current will 'disappear'. Without capacitive top loading the
radiation resistance of a helical antenna will be 1.54 times larger as for a
'straight' vertical of the same height, this is a gain of 1.9dB. When capacitive
top loading is added the advantage of a helical antenna will be
less, for 2 reason :
-
As the antenna has more capacitive top
loading the importance (and thus the gain) of the distributed
inductance decreases.
-
As the capacitance of the vertical part of a
helical antenna is rather large compared to a 'straight' vertical (because
of the larger diameter of the vertical part) the effect (and thus the
gain) of the capacitive top-loading decreases.
An additional problem is that it is not so easy to
built a mechanical stable helical antenna. The only amateur who, to my
knowledge, used a helical antenna with success was Toni Baertschi (HB9ASB),
until the antenna was destroyed in a storm (December 1999).
3.2. Efficiency
If an antenna is fed with a certain power it will radiate a part of that
power. The remaining part is dissipated 'uselessly', in most cases converted
to heat in or around the antenna. Simplified one can say that the transmitter
feeds its power into 2 resistors, the radiation resistance (RA) and
the loss resistance (RL). The efficiency (®) of an antenna is,
[9]
On HF the efficiency of most antenna systems is very high,
90% or more. The most important sources of loss are skin effect in the
antenna wires and dissipation in the transmission line (coax cable). On VHF
and higher frequencies these last can become very important. On LF the situation is completely different, efficiencies of most antennas
used by hams are in the range of 0.01 to 1%. The source of these high losses
is dependent on the type of antenna. For electrical antennas the major
losses will be mainly in the environment and the loading coil. For
transmitting the efficiency of the antenna system will directly affect the
amount of radiated power and thus is very important. . . .
A 160 meter EH antenna Can be useful on 137 kHz (cylinder should be 6 m high x 2m
diameter).
Teslavert
An 160 meter antenna based upon a classic Tesla coil *
High
Power Solid State Tesla Coil
Long
Wave Club of America-1
Long
Wave Club of America-2
Integrated LF Preamplifier Using AD712 or CA3140A Op-Amp
Source: http://frodo.bruderhof.com/ka2qpg/ad712pre.htm
Pierre Thomson, KA2QPG
Longwave Page
A
Universal LF/MF Preamplifier
by Lyle Koehler, KØLR
High-Gain LF Preamp
by Lyle Koehler, KØLR
Source: http://www.computerpro.com/~lyle/preamp/preamp.htm
E-field Whistler Receiver Design
by Scott Fusare, N2BJW
Low
Impedance Active Antenna
Long
Wave Receiver and Antenna Files
This is a very
short description of a tiny low power cw transmitter for long wave. They have
permit in Germany since January 1999. Depending on the PI-Filter components
and voltage for the final stage this transmitter would be able to reach the 100
Watts output level. Running two IRF630 in parallel they got more than 100 Watts of
output "key-down" (16.5V/9A at full load).
Source: http://www.elec-eng.leeds.ac.uk/staff/ct/LF/LF136sum.html
300 W 136kHz
Transmitter
Features:
Single Printed Circuit Board 178 x 128mm including:
Variable Crystal Oscillator
Low Pass Filter
Tx / Rx switching relays
'Optically coupled' over-current protection
VSWR Protection
The circuit is based around a high efficiency class D amplifier which uses
two STW34NB20 power MOSFETS. Rated at 200V and 34 Amps these FETs combined with
protection circuits that can respond to fault conditions in a few tens of
microseconds make for an extremely robust design.
The power output is dependent on the output matching transformer. If one 42mm
3C85 core is used, the maximum power is just over 300W. If two cores are
stacked, the power rating is increased to 400W
(Click
to enlarge)
The prototype transmitter pictured above is designed to produce
400W output from a 45V supply. The output matching transformer used is not
the toroidal type shown in the parts list. The core here is an ETD44 using a
siemens N30 core material. Although the transformer works well, it is difficult
to reproduce. Consequently, the toroidal form is recommended as it's easier to
construct.
A kit of
parts is available. http://www.g0mrf.freeserve.co.uk/300w.htm,
G0MRF HOME
Source: http://www.qsl.net/df3lp/137khz/LF-transmitter.html
Isotron
HF Antennas for small spaces
Spectrogram
Version 6 Downloads
Solar
Cycles 22-23
The
INSPIRE Project *
Radio
Jove
Very
Low Frequency Group
HAARP
AntenneX
One
of this magazine’s main goals is to provide a place for the exchange of ideas
and publication of antenna and radio-related subjects from all parts of the
globe so we could all share and learn how things are done from all viewpoints in
this ever-shrinking world. We am happy to say this goal is being met quite well
with writers from about 25 countries now represented in the thousands of pages
in this magazine.
Radio Society
of Great Britain
International
Telecommunications Union
Radio
Propagation Bibliography
*
Longwave
Technology
[Original source deleted from world wide web]
In part 15 of the FCC rules there is a
provision for unlicensed operation in a number of frequency bands. One of
these is 160 - 190 kHz. You are allowed a total feed plus antenna length
of 15 meters (about 50 feet) and an input power of 1 Watt. Since a high-Q
antenna circuit is required the bandwidth limits the mode to very narrow band
modes such as CW or narrow band digital modes. The
Longwave Club of America is for "Lowfers". In order to get
good results you need a high-Q coil. In order to learn about the subject
of high-Q coils [author] spent a couple of years finding and reading out of
print books about inductors and got a Boonton Model 160 Q-meter and did a great
many experiments.
Lyle Koehler, KØLR - This page
is dedicated to LF experimenting and home brewing
GWEN
- These sites
are going to be converted to GPS differential correction sites to serve the
land mass of the CONUS.
Secretary of the Air Force - US3984839:
Low height VLF antenna system -
Navaid Information - List Server - send mail to:
majordomo@qth.net, leave subject field blank,
in the text enter: subscribe lofer
IK1QFK Home Page: Exploring
ULF-ELF and VLF radio band -
Submarine
Communications Shore Infrastructure - also see SOSUS
& the Glomar Explorer -
Kiwa - Earth
Monitor - 10 Hz to 15 kHz.
AMRAD Low Frequency -
Modifying
the RX320 Receiver for LF/VLF Operation -
LF Engineering - active whips &
other LW hardware
New England Electric Wire Corp - Litz
wire manufacturer
MWS Wire Industries - Litz
wire -
Cooner Wire - Litz wire
Amidon - Ferrite Rods, Bars, Plates
and Tubes and Iron Power, pot cores - and application notes
Brooke Clarke's Time
& Frequency page
|
|