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<v Speaker 1>Welcome once again to the Doctor Sky experience heard exclusively

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<v Speaker 1>here on Talk Radio seventy seven WABC, as we like

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<v Speaker 1>to mention and call it the crown Jewel of radio,

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<v Speaker 1>the iconic seventy seven Talk Radio WABC, beaming out of

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<v Speaker 1>New York City, the nation, the world, and I'm sure

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<v Speaker 1>out to the cosmos. Yes you're listening to me, Steve Kates,

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<v Speaker 1>Doctor Sky, and proudly here on this great radio station

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<v Speaker 1>we bring you interesting information on solar cycle twenty five

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<v Speaker 1>and the great solar storms that have been happening this

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<v Speaker 1>particular week. Listening to this particular update, it's current as

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<v Speaker 1>of May the eleventh, twenty twenty four, the current solar

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<v Speaker 1>wind speed is now five hundred and sixty miles per second.

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<v Speaker 1>That is the stream of particles that move out and

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<v Speaker 1>permeate the solar system. There's a seventy five percent chance

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<v Speaker 1>of more X flares on the Sun, and the massive

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<v Speaker 1>Sunspot group Active Region thirty six sixty four, which now

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<v Speaker 1>contains forty three very active and magnetically charged sunspots, will

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<v Speaker 1>indeed give us some great information in the form of

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<v Speaker 1>energy from the Sun as it now transitions to the

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<v Speaker 1>right side of the Sun and soon to disappear to

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<v Speaker 1>the backside of the Sun. The sunspot number as of

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<v Speaker 1>this particular date is one hundred and fifty six on

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<v Speaker 1>the Sun. But let's talk a little bit more about

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<v Speaker 1>solar flares and what's been happening this week. We continue

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<v Speaker 1>to update you on what happens on our star, the Sun,

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<v Speaker 1>ninety three million miles away. Solar flares of sunspot cycle

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<v Speaker 1>twenty five are interesting. Indeed, solar cycle twenty five began

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<v Speaker 1>on December of twenty nineteen, and it should peak some

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<v Speaker 1>astrophysicists and astronomers believe by late twenty twenty four or

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<v Speaker 1>even early into twenty twenty five. These are geomagnetic stores.

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<v Speaker 1>But let me qualify what we talk about here on

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<v Speaker 1>the ductor Sky experience and Solar cycle twenty five. Sunspots

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<v Speaker 1>appear in the photosphere of the Sun. That's the light area,

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<v Speaker 1>the bright area that you see in need those protective

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<v Speaker 1>solar glasses to view the Sun safely. The temperature of

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<v Speaker 1>that photosphere is about twelve thousand degrees fahrenheit, and these

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<v Speaker 1>sunspots are actually cooler regions on the Sun. Remember, the

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<v Speaker 1>Sun is not solid. It's more described as gaseous, but

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<v Speaker 1>it's more like a plasma. But more on that in

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<v Speaker 1>future reports. Those sunspots, these cores that are darker, are

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<v Speaker 1>about six thousand degrees fahrenheit, and they are surrounded by

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<v Speaker 1>a pnumberal region which is a little bit fainter. What's

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<v Speaker 1>interesting about these sunspots is they are magnetically charged, and

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<v Speaker 1>they are full of magnetic energy. So when some of

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<v Speaker 1>these sunspots butt up against another one, their opposite polarities

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<v Speaker 1>plus minus or minus plus cause what we call the

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<v Speaker 1>phenomenon of solar flares. Now, if you can imagine this,

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<v Speaker 1>and it's hard to even be able to talk about

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<v Speaker 1>because it's so out of this world, the average flare

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<v Speaker 1>intensity is as if you detonated, let's say a hundred

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<v Speaker 1>million hydrogen bombs. That energy, of course, is pushed out

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<v Speaker 1>into space, and in many cases, the Sun pushes out

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<v Speaker 1>other material called coronal mass ejections. These are highly charged

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<v Speaker 1>particles protons that move out at a slower speed than

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<v Speaker 1>the speed of light. A solar flare literally travels from

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<v Speaker 1>the Sun to the Earth in about eight and a

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<v Speaker 1>half minutes. That's the speed of light. But these coronal

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<v Speaker 1>mass ejections, these particles can take upwards of fifteen to

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<v Speaker 1>twenty hours or more. But here's a little history of

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<v Speaker 1>Solar cycle twenty five as far as X flares and

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<v Speaker 1>geomagnetic storms. Remember, geomagnetic storms go from a G one

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<v Speaker 1>up to a G five, which we just had this

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<v Speaker 1>past weekend. Let's do a little history. The first geostorm

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<v Speaker 1>of this particular cycle happened on May twelfth of twenty

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<v Speaker 1>twenty one. That was a G three storm, not seen

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<v Speaker 1>widely around the world, but it did interfere with lie

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<v Speaker 1>little bit with high frequency radio and communications. On July third,

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<v Speaker 1>twenty twenty one, the first of the X flares of

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<v Speaker 1>this solar cycle. On Halloween of twenty twenty one, another

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<v Speaker 1>X flare from the Sun November fourth, twenty twenty one,

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<v Speaker 1>our first G four solar storm. Unfortunately, at that time,

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<v Speaker 1>auroras were not widely visible as they were over this

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<v Speaker 1>past weekend. Moving through our time capsule, January twenty ninth

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<v Speaker 1>of twenty twenty two, a solar storm actually wiped out

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<v Speaker 1>thirty eight of forty nine small little satellites like the

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<v Speaker 1>Little SpaceX satellites because of the intense radiation. Moving on

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<v Speaker 1>to January twenty twenty three, another solar storm. But it

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<v Speaker 1>gets more interesting. On March thirteenth, twenty twenty three, one

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<v Speaker 1>of the fastest coronal mass ejections of this cycle were recorded.

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<v Speaker 1>We talk about a speed of twelve hundred miles per

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<v Speaker 1>second as opposed to the current wind speed of five

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<v Speaker 1>hundred and sixty miles per second that hit the Earth

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<v Speaker 1>within its energy in a little bit less than twenty hours.

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<v Speaker 1>Moving on to March the twenty third of this particular year,

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<v Speaker 1>as we continue to talk about these events in astronomy,

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<v Speaker 1>that was a G four solar storm knocked out some

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<v Speaker 1>power stations in the US, albeit on a minor scale.

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<v Speaker 1>And then moving on to April twenty first of twenty

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<v Speaker 1>twenty three, another G four solar storm. Now, what's going

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<v Speaker 1>on with the latest on the Sun? A brand new

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<v Speaker 1>CME just launched off the Sun today as we're doing

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<v Speaker 1>this recording on May the eleventh. On the X scale,

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<v Speaker 1>it was a five point eight, and that particular energy

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<v Speaker 1>may energize the entire G numbers, meaning those geo storm

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<v Speaker 1>levels all the way up to a number five like

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<v Speaker 1>we had this past weekend. So in simple English, keep

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<v Speaker 1>your eyes peeled to the northern sky in dark conditions,

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<v Speaker 1>because you may get, indeed to see something, as many

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<v Speaker 1>people did over this previous weekend and this weekend entirely

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<v Speaker 1>when they saw the un auroras as far south of

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<v Speaker 1>Puerto Rico into Mexico and areas to the south like Florida,

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<v Speaker 1>and here in Arizona where I am a fascinating story

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<v Speaker 1>again solar and sunspot active region as we talk about

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<v Speaker 1>it here, This particular active region known as number three

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<v Speaker 1>six sixty four thirty six sixty four with forty three

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<v Speaker 1>very energetic sunspots, is now moving to the lower right

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<v Speaker 1>side of the Sun. So if you still have those

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<v Speaker 1>solar glasses from last month's eclipse, make sure they don't

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<v Speaker 1>have any holes in them, and you can actually see

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<v Speaker 1>this sunspot on the right edge of the Sun, one

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<v Speaker 1>of the most massive sunspots of all time. But in conclusion,

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<v Speaker 1>let's talk about the Great Carrington event. That's an event

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<v Speaker 1>that was widely observed by Richard Carrington and another astronomer

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<v Speaker 1>back in September of eighteen fifty nine when they observed

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<v Speaker 1>a sunspot about as large as this group right now,

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<v Speaker 1>and it produced one of the most massive X flares.

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<v Speaker 1>We don't know the exact X number. And again that

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<v Speaker 1>particular solar storm and sunspot group was literally placed at

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<v Speaker 1>the front and center of the Sun. So we call

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<v Speaker 1>it the kill shot when that giant sunspot group erupts

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<v Speaker 1>and it sends out a CMA chronal mass ejection. Most

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<v Speaker 1>damage on a very high leveled numbered X flare caused

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<v Speaker 1>what happened in eighteen fifty nine, what did it cause

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<v Speaker 1>during the Internet era, then the Victorian Internet, we use

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<v Speaker 1>telegram and many telegraphers were actually shocked when they were

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<v Speaker 1>keying out messages and many of the transmission telephone like lines,

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<v Speaker 1>telegraph lines literally went a fire and a blaze. Now

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<v Speaker 1>that's incredible. We live in a digital world. I need

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<v Speaker 1>not remind you. And the problematic thing now is if

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<v Speaker 1>we have a similar type X flare on the Sun.

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<v Speaker 1>Not to be alarmist, but are we speaking truth and science,

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<v Speaker 1>This could very well knock down not only power grids,

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<v Speaker 1>but also could destroy satellites. And right now, this is

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<v Speaker 1>very interesting story. Back in March of nineteen eighty nine,

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<v Speaker 1>another massive X flare fifteen on the X flare scale,

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<v Speaker 1>It actually hit and it hid an area in Canada

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<v Speaker 1>and at Quebec, and it knocked out power by disrupting

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<v Speaker 1>those generators to about thirty million people. And people may

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<v Speaker 1>wonder why, Well, the real truth of the matter is

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<v Speaker 1>the reason that that particular solar storm was so effective

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<v Speaker 1>there is that the rock, or the surface rock of

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<v Speaker 1>that part of the nation and part of the world

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<v Speaker 1>is very hard, igneous rock. And when those solar protons

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<v Speaker 1>and storms hit the earth in other areas that are softer,

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<v Speaker 1>they get absorbed for a good portion of their energy

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<v Speaker 1>into the ground. But in this particular case, the energy

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<v Speaker 1>bounced off the hard rock and shot itself back up

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<v Speaker 1>to transformers and power lines, causing that great damage. To

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<v Speaker 1>listen to me, Doctor Sky and the Doctor Sky Experience,

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<v Speaker 1>you can hear our updates with Frank Morono on the

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<v Speaker 1>other side of Midnight and every other Wednesday at one am.

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<v Speaker 1>He's kind enough to transform the name of the show

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<v Speaker 1>to Cosmic Conversations with me, Doctor Sky, as we talk

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<v Speaker 1>about the great realms of astronomy, space, aviation, and weather

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<v Speaker 1>and privilege and honored to be with owner and operator

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<v Speaker 1>John Katzimatides every Sunday morning as we take our minds

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<v Speaker 1>off the political world and talk about the great vast

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<v Speaker 1>unknown on the Cat's Roundtable, and then more and more

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<v Speaker 1>as these events happen. Look for me Doctor Sky with

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<v Speaker 1>the Doctor Sky Experience, updates on Kats and Cosby on

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<v Speaker 1>the Great five PM Show. If you'd like to email me,

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<v Speaker 1>that's simple. It's doctor Sky's show. Just Drsky Show at

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<v Speaker 1>gmail dot com. And what do we say, folks, Always

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<v Speaker 1>remember to keep your eyes to the skies as I

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<v Speaker 1>try to earn that opportunity. It's a privilege and honor

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<v Speaker 1>to be here on talk radio seventy seven WABC with

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<v Speaker 1>all the listeners. As we call it the crown Jewel

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<v Speaker 1>of radio mentioned before, the iconic seven Talk Radio w

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<v Speaker 1>A b C beaming ourselves out from New York City,

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<v Speaker 1>the nation, the world, and I'm sure the cosmos. I'm

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<v Speaker 1>Doctor Sky with the Doctor Sky Experience. I'm your navigator

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<v Speaker 1>on the highway to the heavens, a highway that has

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<v Speaker 1>yet no tolls, so we can expand our minds and

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<v Speaker 1>look deep into the cosmos on things that go bump

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<v Speaker 1>in the day and bump in the night. I'm your navigator.

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<v Speaker 1>Thanks for joining me.
