high frequency
(HF)
(electromagnetic radiation, frequency 3-30 MHz)
Radio astronomy generally uses the terms high frequency
and low frequency in a general way, dividing the entire radio
spectrum (or sometimes also including medium frequency),
often intending the term high frequency to reach or include
microwave. I've seen 350 MHz used as a threshold for
low frequency (e.g., low frequency radio astronomy) but the threshold
probably varies widely based upon the topic of discussion.
In contrast to this, for regulation and communications purposes,
the ITU uses the terms high frequency and low frequency
for specific communications bands that are far different than
the typical language of radio astronomy, though astronomers clearly
must refer to these ITU bands on occasion. Some of the ITU bands:
Very low frequency | VLF | 3-30 kHz |
Low frequency | LF | 30-300 kHz |
Medium frequency | MF | 300-3000 kHz |
High frequency | HF | 3-30 MHz |
Very high frequency | VHF | 30-300 MHz |
(EMR,spectrum,band)
Further reading:
https://en.wikipedia.org/wiki/High_frequency
https://www.astron.nl/telescopes/square-kilometre-array/
https://science.nrao.edu/facilities/vla/docs/manuals/obsguide/topical-guides/hifreq
https://www.astron.nl/lofarschool2014/Documents/Monday/Heald.pdf
WaveL | Freq | Photon Energy | | |
10m | 30MHz | 124neV | begin | high frequency |
100m | 3MHz | 12neV | end | high frequency |
|
Referenced by pages:
pulsar (PSR)
radio
radio astronomy
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