Millisecond solar radio bursts in the metric wavelength range

Details Millisecond solar radio bursts in the metric wavelength range Millisecond solar radio bursts in the metric wavelength range

2010-09-22

arxiv.org/abs/1009.4477v1

2006AIPC..848..224M

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

Recent Advances in Astronomy and Astrophysics: 7th International Conference of the Hellenic Astronomical Society. AIP Conferen

Scientific paper

10.1063/1.2347982

A study and classification of super-short structures (SSSs) recorded during metric type IV bursts is presented. The most important property of SSSs is their duration, at half power ranging from 4-50 ms, what is up to 10 times shorter than spikes at corresponding frequencies. The solar origin of the SSSs is confirmed by one-to-one correspondence between spectral recordings of Artemis-IV1 and high time resolution single frequency measurements of the TSRS2. We have divided the SSSs in the following categories: 1. Broad-Band SSSs: They were partitioned in two subcategories, the SSS-Pulses and Drifting SSSs; 2. Narrow-band: They appear either as Spike-Like SSSs or as Patch-Like SSSs; 3. Complex SSS: They consist of the absorption-emission segments and were morphologically subdivided into Rain-drop Bursts (narrow-band emission head and a broad-band absorption tail) and Blinkers.

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