Technical FAQs 4

Does a 6-15 GHz solar radio observation system have an observation ability?

The observation of multiple eruptions indicates that the 6– 15 GHz solar radio observation system initially possessed an observation ability. In the next step, we need to continuously improve the system according to the observation situation to obtain higher-quality data. 3.4.

Where does RSTN measure solar radio bursts?

RSTN uses four widely spaced antennae to observe the Sun between 18 MHz and 15 GHz to measure solar radio bursts: Palehua (Ka'ena Point), Learmoth, San Vito and Sagamore Hill. The data presented here are provided, ‘as is,’ and in most cases the linked documentation is the entirety of available information.

What are solar radio bursts?

The radio bursts you are searching for follow this cycle. Known as ‘Type III solar radio bursts’, they are closely linked to solar flares, which are tremendous explosions of radiation from the Sun’s surface. Solar flares fling electrons out into space.

What is a solar radio spectrograph?

The Learmonth Solar Radio Spectrograph observes the radio emmission of the Sun from 25MHz to 180 Mhz. Solar radio spectrograph display radio bursts or "sweep" events. These are classified into particular types.

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