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Magnetic Storms
in the News!!!

 

 

BGS's Eskdalemuir Observatory is situated in the Southern Uplands of Scotland. It opened in 1908.

On Tuesday, October 28, 2003 an extreme blast of plasma (ionized gas) was ejected from the sun and hurled toward earth at a speed of 5 million miles per hour. Measuring X17 on the Richter scale of solar flares, the flare is the fourth most powerful seen and the most powerful to affect the earth since the 1989 event that knocked out the power grid in Quebec, Canada.

The storm impacted the earth on Wednesday October 29 and immediately began to interfere with high-frequency voice-radio communications for planes flying near the North Pole. Lesser effects were also felt in some power grids and satellite operators re-positioned satellites in sensitive areas to reduce the likelihood of loss due to overloading of sensitive electronics.

Magnetic effects were detected by magnetometer installations around the world to lesser or higher degrees depending on their proximity to the northern hemisphere. GEM Advanced Magnetometer detected the storm via its Potassium magnetometer (GSMP-40) installation throughout Wednesday. Data were sampled at 10 times per second.

Data below show the magnitude of the storm and its magnetic effects. As Dr. Ivan Hrvoic, President, noted, “This is the most intense storm that I have seen in my career ... and I have been involved with magnetics and magnetic instrumentation for many years.”

Figure 1: Magnetic storm activity, Wednesday October 29, 2003 – 11:00 am to 4:00 pm EST. Maximum amplitude is 56043 nT and minimum amplitude is 54894 nT. Data acquired with GEM’s Potassium (GSMP-40) ultra-sensitive magnetometer.

As indicated in the plot above, the storm was characterized by a period of noise followed by a positive anomaly on the order of 500 nT and a subsequent negative anomaly on the order of 900 nT. These latter results are remarkable as the change from maximum to minimum occurred over the period of approximately one hour.

While severe, the amplitude of the shift to negative values did not approach a significant percentage of the earth’s approximate amplitude of 56,000 nT at this location (Richmond Hill, Ontario, Canada). Maximal danger occurs when the polarity of the incoming plasma is reversed from the direction of the earth’s field – leading to “holes” in the magnetic layer that protects the earth from severe damage. News outlets noted this effect in their regular reports, available, for example, at www.cbsnews.com/stories/2003/10/23/tech/main579650.shtml

Sunspot activity has been at a high for several weeks as shown by a plot of magnetic activity for Friday October 24. Here, we see a clear difference in amplitude between the October 28 and October 24 events as indicated by a maximum anomaly of approximately 55770 nT and a minimum anomaly of approximately 55500 nT (i.e. 270 nT peak-to-peak value).

Figure 2: Magnetic storm activity, Friday October 24, 2003 – 17:07 am to 22:39 pm EST. Maximum amplitude is 56043 nT and minimum amplitude is 54894 nT. Data acquired with GEM’s proprietary Overhauser (GSM-19) magnetometer.

These types of results are valuable in terms of characterizing activity and in helping to understand magnetic storms – a science that is still in its infancy. Magnetic  can research and monitoring holds the promise of helping to alert us to the significant effects of magnetic storms to communication systems, satellites, power grids and pipeline infrastructure. For more information on current work and the significance of magnetic measurements, please see www.gemsys.ca/Quantum/Scientific/Protecting%20Us%20from%20the%20Sun's%20Fury.htm.

GEM Advanced Magnetometers is the world-leader in production of magnetic instrumentation for monitoring geomagnetic events on a long-term and short-term basis. Instruments are installed in major observatories in the United States, United Kingdom, Germany, Canada and many other countries. Other instruments are also available for monitoring volcanic and earthquake activity. For details, visit http://www.gemsys.ca/apps_observatory.htm


GEM User Links

Below is a partial list of Magnetic Observatories that have standardized on or implemented GEM Systems. If you require additional information on a particular observatory listed (or not listed) here, please contact GEM.

Canada. Canadian National Geomagnetic Program. Standardized on GEM.

Denmark. Brorfelde Observatory. 2002 report, in part, describing Overhauser use for total field measurement. Unlike other magnetometers the GSM-19 does not require corrections (page 13). 

Finland.
Numivarji Observatory,

Germany. Niemegk and Munich Observatories.

Hungary.
Tihany Observatory.

Japan. Kakioka Observatory and others.

South Africa. Hermanus Observatory.

United Kingdom.
Multiple observatories, including Eskdalemuir Observatory, Scotland. British Geological Survey has standardized on GEM.

www.geomag.bgs.ac.uk/eskdale.html
www.geomag.bgs.ac.uk/uksurvey.html
http://www.geomag.bgs.ac.uk/observatories.html

U.S.A. Multiple observatories. USGS is standardizing on GEM.




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