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Natural Radio Lab

Natural Radio is the VLF radio emissions that originate terrestrially from lightning and within the earth's magnetosphere through interaction with the Sun. Most of these radio signals, sferics, tweeks, whistlers, chorus and others, occur within the range of human hearing, and can be heard with simple receivers as described on this site.

Natural Radio Lab also looks at Space Weather and Geomagnetic Storms. These are affected by solar activity such as the solar wind, sunspots, solar flares and coronal mass ejections or CMEs. In the popular media, these events are often loosely referred to as "solar storms" or "sun storms".

Please explore this site. I hope you go beyond reading what's here and actually go out and take the opportunity to hear whistlers or the enchanting sounds of the dawn chorus.

Mark Karney, N9JWF
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What is the “Kp”?

naturalradiolab.com Posted on January 19, 2012 by Mark KarneyOctober 21, 2012

The K-index is a code that is related to the maximum fluctuations of the horizontal components of the magnetic field measured on a given magnetometer, and relative to a geomagnetically quiet day. Each geomagnetic observing station generates its own K index and the weighted average of all stations is Kp or the Planetary K-index. Because of its method of calculation, the Kp-index is not real time.

At SEC (Space Environment Center, NOAA), the final real-time K-index which is referred to as the “Estimated Kp“, (as opposed to the official Kp) appears on the website http://www.sec.noaa.gov/today.html, and is determined after the end of the prescribed three hour intervals (0000-0300,0300-0600, …, 2100-2400). The maximum negative and positive
deviations in the horizontal components during a given 3 hour period are added together to get the total maximum fluctuation.

The Kp-index ranges from 1-9, with 1 being very quiet and 9 indicating major geomagnetic activity. When the Kp approaches 6, Natural Radio activity is usually high. If the Kp is 6 or greater I am almost always able to hear chorus and VLF emissions for an hour or two after sunrise.

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