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What it is : Radio figure of an annularsolar occultation .

When it was taken : Oct. 14 , 2023 .

Upper row: Radio images of the 2023 Oct. 14 solar eclipse observed by the Long Wavelength Array at the Owens Valley Radio Observatory Bottom row: Schematic representation of what visible images of the eclipse looked like at the same time.

Radio images of October’s annular solar eclipse as seen by the Long Wavelength Array, with images below of what it looked like in visible light.

Where it was contain from : Owens Valley Radio Observatory Long Wavelength Array ( OVRO - LWA ) , California .

Why it ’s so special : Scientists have learn the first receiving set scope picture of an annular solar eclipse ’s famous " ring of fire " effect   — even though they were outside the eclipse ’s cardinal path .

On Saturday , Oct. 14 , 2023,an circinate solar eclipsewas seeable from inside a 125 - mile - all-embracing belt through nine U.S. state , include the northeasterly tip of California . Owens Valley Radio Observatory , in Big Pine , California , was not within that course , so it was only able to image an 80.5 % fond solar eclipse , according tothis Interactive Google Mapfrom French occultation map maker Xavier Jubier . ( Within the path of the eclipse , as much as 91 % of the Lord’s Day ’s Inner Light was blocked ) .

Looped video footage of a large shadow moving across North America

Related : The best photos of the Oct. 14 ' ring of fire ' eclipse over North America

However , radio astronomer were still able to appropriate radio prototype of the " ring of fervidness " because OVRO - LWA detect the sunlight ’s corona , or super - hot out atmosphere , which was inconspicuous to those watching the solar eclipse .

" From our lookout station site in California we were not in the belt to see the annular eclipse , yet we ’ve been able to ' see ' it all clearly unfold in radio , which reveals a much larger solar disk than its seeable counterpart thanks to its sensitivity to the extended solar corona,“Bin Chen , associate professor of physics at New Jersey Institute of Technology ’s Center for Solar - Terrestrial Research ( NJIT - CSTR ) who led the observations with colleagues , said in astatement .

The sun in a very thin crescent shape during a solar eclipse

tuner astronomy is the survey of supernal object atradio frequencies , which are invisible to human eyes . OVRO - LWA ’s nearness to the way provide a unequaled opportunity to examine the sun ’s extended corona with the raiment ’s 352 antennas , taste thousands of radio wavelengths at once .

— 15 sign the sun is pitch up for its explosive peak — the solar utmost

— See the total ' ring of fervour ' eclipse in 4 seconds in stunning satellite television

A photograph of a partial solar eclipse seen from El Salvador

— The good photos of the Oct. 14 ' ringing of flaming ' eclipse over North America

" To in the end see a ' pack of fire ' occultation this way was spectacular … we have n’t seen this quality of radiocommunication imaging of the sun before,“Dale Gary , a prof of physics at NJIT - CSTR and co - investigator on the OVRO - LWA task , articulate in the assertion . " We commonly can not see the electric glow from the ground except during a total occultation , but we can now see it all the time with OVRO - LWA . This occultation makes it that much more dramatic . "

The circinate solar eclipse on Oct. 14 also traverse parts of Mexico , Belize , Honduras , Nicaragua , Panama , Colombia and Brazil . The nextsolar eclipsevisible from North America will be a total one , crossing from the southwest to the northeast on April 8 , 2024 .

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