Engineering topics
Publications and source records attributed to Tsurutani, B. T..
Using empirical results on the interplanetary magnetic field strengths of magnetic clouds versus velocities, we show that the 1 September 1859 Carrington solar flare most likely had an associated intense magnetic cloud ejection which led to a storm on Earth of DST ~ -1760 nT.
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In this paper we describe our plans to better understand this phenomenon using TEC measurements from ground and space-borne GPS receivers.
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Polar cap boundary layer waves are ELF/VLF electric and magnetic waves detected on field lines just adjacent to the polar cap. Intense waves are present at this location essentially all (96%) of the time.
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The purpose of this paper will be to examine a specific but important subset of magnetic storms, those that are caused by large southward, smoothly rotating magnetic fields: interplanetary magnetic clouds.
Interplanetary shocks can trigger intense dayside auroral brightenings and very fast anti-sunward auroral expansions. these auroral phenomena are called shock-auroras.
Slow magnetic clouds have been analyzed to determine their characteristics and geoeffectiveness.
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