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There is nothing on earth that impacts our lives more than our thoughts, still, the enemy has enough power to influence them. That's why every thought that crosses our mind must be taken captive and made obedient to Christ.
Behemoth sunspot AR3664 unleashes its biggest solar flare yet, sparking radio blackouts on Earth. Our turbulent sun is certainly throwing one huge solar-flaring tantrum this week. It's hard keeping up!
It's gone and done it again.
Colossal sunspot AR3664 has unleashed its most powerful solar flare yet, and Earth is once again in the firing line.
The X3.98 flare peaked in the early hours this morning (May 10) at 2:54 a.m. (0654 GMT) triggering either temporary or complete loss of high frequency (HF) radio signals across Asia, eastern Europe and eastern Africa.
4 large incoming solar bursts could supercharge the auroras this weekend
The X3.98 flare this morning is not only AR3664's largest solar flare to date, but also the 4th largest solar flare this solar cycle. Solar flares are eruptions from sunspots on our sun's surface that emit intense bursts of electromagnetic radiation. They are categorized by size into lettered groups, with X-class flares being the most powerful. Then, there are M-class flares that are 10 times less powerful than X-class flares, followed by C-class flares which are 10 times weaker than M-class flares. B-class are 10 times weaker than C-class flares and, finally, A-class flares are 10 times weaker than B-class flares and have no noticeable consequences on Earth. Within each class, numbers from 1-10 (and beyond for X-class flares) denote a flare's relative strength.
High frequency radio blackouts were observed throughout Asia, eastern Europe and eastern Africa shortly after the X-class solar flare. (Image credit: NOAA/SWPC)
The radiation travels toward Earth at the speed of light and ionizes (gives electrical charge to) the top of Earth's atmosphere, creating a higher-density environment for the radio signals to navigate through. (Note: These ionizing X-rays are not to be confused with coronal mass ejections, or CMEs, by which plasma and magnetic fields erupt from the sun. CMEs travel at slower speeds and often take several days to reach Earth.)
When attempting to travel through that ionized layer, radio waves can't help but interact with electrons that've now flooded their environment. In doing so, the radio waves lose energy due to more frequent collisions with the electrons. This can lead to radio signals becoming degraded or completely absorbed, according to the National Oceanic and Atmospheric Administration's (NOAA) Space Weather Prediction Center (SWPC). This recent X-flare eruption was also accompanied by a CME, a large expulsion of plasma and magnetic field from the sun.
Images credit: SOHO/LASCO, NOAA/SWPC, nemesis maturity channel, helioviewer.org
Music credit: YouTube Audio Library
