WEBVTT

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Thanks for tuning in. Hamtalk Live will be on

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the air shortly. Please stand by. Thanks for

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tuning in. Hamtalk Live will be on the air shortly.

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Please stand by. This episode of HamTalk Live

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is brought to you by Tower Electronics. For cables,

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connectors, and more, call 920 -435 -2973 or

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visit pl -259 .com and by the HamStation. Get

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your new radio or antenna by calling 800 -729

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-4373 or go to hamstation .com. everyone! This

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is Neil Rapp, WB9VPG, and welcome to HamTalk

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Live episode number 48, Sunspot Cycles with Karl

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Lutzelschwaub. K9LA, recorded live on Thursday,

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January 19th, 2017. I'm your host, Neil Rapp,

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WB9VPG. Thanks for tuning into this episode of

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HamTalk Live. Tonight, We're joined by Carl Lutzelschwaab,

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K9LA, who will take your questions about sunspot

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cycles and how they affect radio propagation.

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We will take your calls live in just a few minutes.

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Last week, John Davis, WB4QDX, was here to talk

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about setting up a D -Star rig. We'll have some

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more D -Star, DMR, and System Fusion shows in

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the future. So if you missed the show about D

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-Star, you can listen anytime at HamTalkLive

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.com, or on iTunes, Stitcher, Google Play, TuneIn,

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SoundCloud, or YouTube, or several other podcasting

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sites. Hey, congratulations to Hope Lee, KM4IPF.

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She had over 30 ,000 views on a Facebook video.

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of her working the ham radio station on the set

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of the tv sitcom last man standing um so hope

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just keeps getting all over the screen and uh

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if you haven't seen it yet go over to facebook

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check out the ka0xtt web page there on facebook

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and you can watch that One other note, we want

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to send our condolences to the family of Charlie

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Emerson in 4OKL. Charlie was chairman of the

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Huntsville HamFest and he became a silent key

00:03:37.180 --> 00:03:40.419
this week. He was on episode number 27 of HamTalk

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Live back in August. And if you tune into Amateur

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Radio Newsline tomorrow, there'll be a special

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tribute to the friendly ham who made Huntsville

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the world's friendliest ham fest. Well, we'll

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be back. We'll have the interview with Carl Lutzelschwaab

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and you can call us with your sunspot cycle questions

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on Skype. The username there is ham talk live,

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or you can call us on. the old telephone. The

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number is 812 -NET -HAM -1. That's 812 -638 -4261.

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You can also tweet us a question or Twitter handle

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is at HamTalk Live. So we'll check those as well.

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And I'll be back with Carl Lutzelschwaab, K9LA,

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right after this word from the HamStation right

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here on HamTalk Live. This episode of HamTalk

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Live is brought to you by the HamStation. For

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We're not sure what's up with the fifth dentist,

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but four out of five dentists recommend listening

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to HamTalk Live. Hey, be sure to check out thehamstation

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.com or give Dan or Jeff a call. 800 -729 -4373.

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They've got you covered for just about anything

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you need. Tell them you heard it here on HamTalk

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Live. We're on the air every Thursday night at

00:06:06.240 --> 00:06:09.269
9 p .m. Eastern Time. Right here at HamTalkLive

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.com and if you missed the show you can listen

00:06:11.569 --> 00:06:14.629
to the archive on the website or download it

00:06:14.629 --> 00:06:19.740
for most popular podcasting websites. Carl Lutzelschwaab,

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K9LA, was first licensed in October of 1961 with

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the callsign WN9AVT. His interest in amateur

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radio came from being a shortwave listener in

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the fifth and sixth grades using a National NC

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60 with a long wire out the basement window.

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His amateur radio interests ultimately led to

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a career in electronics. His interest in propagation

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goes back to his college days at Purdue University

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where he earned a bachelor of science in electrical

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engineering in 1969 and a master's in 1972. Carl

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retired in October 2013 after 41 years as an

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RF design engineer with Motorola and Raytheon,

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which is formerly Magnavox. He's authored many

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articles and given many presentations on solar

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effects on the radio propagation. He and his

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wife Vicki Lutzer -Schwab, AE9... YL have been

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on several DXpeditions. He's at the top of the

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DXCC honor roll, having worked all current DXCC

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entities. He's also completed DXCC on 160, and

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is nearing five -band worked -all zones. His

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website contains many of his articles and tutorials.

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That's over at K9LA. And he's also the vice director

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of the ARRL Central Division. So Carl, welcome

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to HamTalk Live. Well, hello, Neil. I'm glad

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to be here and hope I can provide some good information

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to all the listeners. Yeah, sure. We appreciate

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you coming on the show and appreciate your help

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with things at my school as well. And we want

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to start off just talking about the sunspot cycle.

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We know from studying from the license that there's

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this 11 year cycle. And so tell us a little more

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about that cycle and where we are in that cycle

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right now. Okay Neil, very good. Well we measure

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solar cycles from solar minimum through solar

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maximum and then back down to solar minimum.

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Sometimes it's not real easy to tell when a solar

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minimum is. because there are many things going

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on. Now the average length of a solar cycle as

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you stated is about 11 years and I can't stress

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the fact that it's about 11 years. Of the 24

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cycles that we have in recorded history the length

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varies from a couple years shorter than 11 to

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several years longer than 11. Average rise time

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of a solar cycle is about four years. So after

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hitting solar minimum, we should usually expect

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to see the maximum about four years later. And

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some simple math says the average descent is

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therefore seven years. So what that tells us

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is the descent is much slower than the rise.

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And that's been going on for... or at least all

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the 24 cycles that we have recorded. Now, posted

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in various places, I was just looking at it on

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QRZ .com, is figure one, which I thought might

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help, and I'll talk about figure one. If you

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can view it, that's great. If not, hopefully

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I can explain it. What it is is just shows the...

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Smooth sunspot number for the last one two three

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four five six solar cycles that'd be cycle 19

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20 21 22 23 and 24 and that extends from about

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1954 up to the present date and let me jump in

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here too if if you aren't looking at the pictures.

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We also have those on our Twitter. So if you

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go to HamTalk Live on Twitter or on our Facebook

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page, they're there as well, as well as in that

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news post on QRZ .com. So you can try to see

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those if you want to follow along. Yeah, well,

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thanks, Neil, for further additional information

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there. What we can see there is cycle 19 as maybe

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most of you are aware has been the biggest one

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in our recorded history Now that doesn't say

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that the Sun has done bigger cycles before Before

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we started even viewing sunspots, but at least

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19 is the biggest cycle 20 was kind of small

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About half the size of 19 and then cycles 21

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and 2 came 22 came along and they were pretty

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good not as big as 19, but they provided lots

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of good 10 meter openings worldwide. Cycle 23,

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which peaked around 2000 for the first peak,

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was not too far behind cycle 2, so it gave lots

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of good worldwide opportunities. And then cycle

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24, if you can see the picture, it stands out.

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It's the lowest cycle in our lifetimes. So things

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have been kind of going down. since cycle 19

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and maybe a little bit later we'll talk about

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that. If you get the picture you'll see some

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of those solar cycles have dual peaks. In other

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words they peak the first time then they take

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a little dip and then go up again. What that

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is is just that the solar hemispheres aren't

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in sync. Sunspots in the northern hemisphere

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sometimes are greater and that causes a peak

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and then sunspots in the southern hemisphere

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are just come roaring back and that causes another

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peak. Interesting phenomena, and there's a lot

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of good stuff that we won't talk about, but hopefully

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I'll cover some of the general stuff. With cycle

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24, we're in the decline. We're more than halfway

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down to solar minimum, which is expected to be

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in about 2020. And then of course that kind of

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suggests that in 2024 cycle 25 will peak So that's

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it that's a little bit background on that question

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Okay, well since we're we're kind of you know

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approaching the bottom of the cycle here We noticed

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that the bands have been pretty bad for a while

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Seems like every time I get on Twitter. It's

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the bands are dead Jim and you know the Forecast

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just says you know band closed band closed band

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closed so Why is this one so much worse than

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the normal? That's a real good question As I

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mentioned just a couple of minutes ago cycle

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24 is the lowest one in our lifetime And it also

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suggests that maybe cycle 25 is going to be low

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also. Now why is the cycle so much worse? Well,

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it's because for the past several solar cycles,

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the sun's magnetic field has been weakening.

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And of course, sunspots are tied to the sun's

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magnetic field and the plasma flow within the

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sun. So that's why it's weakening. Now we don't

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fully understand or at least solar scientists

00:14:03.039 --> 00:14:07.059
don't fully understand why the sun's magnetic

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field is weakening, but it is. And there sure

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is a lot of research trying to understand, you

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know, how solar cycles are generated. You know,

00:14:18.559 --> 00:14:21.779
we want to do that to be able to predict future

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cycles because of, you know, space operations

00:14:28.240 --> 00:14:31.450
out there. An active sun creates more hazard

00:14:31.450 --> 00:14:34.710
to the astronauts. Of course, Ham Radio was interested

00:14:34.710 --> 00:14:38.690
in what solar cycles are doing. Now, I've got

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a figure two on there posted to the qrz .com

00:14:43.710 --> 00:14:47.529
and all the places that Neil said. And what it

00:14:47.529 --> 00:14:51.190
shows is all 23 recorded solar cycles, or 24

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recorded solar cycles. And what the figure shows

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is that the first four cycles were rather high.

00:14:59.539 --> 00:15:04.120
The next three cycles were rather low. The next

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six or so cycles were kind of high. Then we went

00:15:09.559 --> 00:15:12.000
into a period of about four solar cycles that

00:15:12.000 --> 00:15:14.600
were kind of low. And then we hit the modern

00:15:14.600 --> 00:15:17.700
times where cycle 19 was, and that was very high.

00:15:18.240 --> 00:15:25.820
So what we've had is we've had a period of very

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high solar cycles followed by a period of low

00:15:28.840 --> 00:15:32.980
solar cycles followed by another period of high

00:15:32.980 --> 00:15:37.299
solar cycles followed by another period of low

00:15:37.299 --> 00:15:40.399
and then this recent period of very high solar

00:15:40.399 --> 00:15:45.080
cycles. What that suggests is we're now headed

00:15:45.080 --> 00:15:48.679
for some low solar cycles, 24, 25, maybe even

00:15:48.679 --> 00:15:52.269
26. We like I said, we can't really predict that

00:15:52.269 --> 00:15:55.110
very well, so we're just gonna have to wait and

00:15:55.110 --> 00:16:05.649
see what happens The solar cycles of course get

00:16:05.649 --> 00:16:10.830
into how good the bands are Yeah, and that's

00:16:10.830 --> 00:16:16.490
the the next thing here is okay, so the bands

00:16:16.490 --> 00:16:21.690
are dead you know the bands are not what they

00:16:21.690 --> 00:16:26.149
have been for several years so what do we do

00:16:26.149 --> 00:16:29.690
about it what what implications does the cycle

00:16:29.690 --> 00:16:33.649
have on trying to choose a band and operating

00:16:33.649 --> 00:16:37.669
times and and and get through this low part of

00:16:37.669 --> 00:16:45.980
the cycle yeah that's a good question As we've

00:16:45.980 --> 00:16:49.860
since we've been proceeding on the descent of

00:16:49.860 --> 00:16:56.100
cycle 24 The bands have been pretty bad and the

00:16:56.100 --> 00:16:59.000
reason for that is when there are lots of sunspots

00:16:59.000 --> 00:17:04.480
There's lots of ionization mostly in the especially

00:17:04.480 --> 00:17:07.920
in the f2 region, which is Generally what is

00:17:07.920 --> 00:17:11.039
used for for long -distance communications worldwide?

00:17:12.539 --> 00:17:16.029
and what that means is when there's more ionization,

00:17:16.670 --> 00:17:19.269
the higher frequencies can be refracted back

00:17:19.269 --> 00:17:22.450
to Earth. They don't go through the ionosphere

00:17:22.450 --> 00:17:26.529
into space to never return unless the universe

00:17:26.529 --> 00:17:29.009
is, you know, closed and folds back on itself.

00:17:29.250 --> 00:17:32.710
But we won't get into that. Yeah. We hope that's

00:17:32.710 --> 00:17:34.710
not happening. Yeah. If you want to know more

00:17:34.710 --> 00:17:38.650
about that Star Trek episode number. Yeah, exactly.

00:17:39.869 --> 00:17:44.710
OK. So, you know, there are two things that really

00:17:44.710 --> 00:17:48.170
determine if you can have a QSO between you and

00:17:48.170 --> 00:17:50.410
a target location. One is there's got to be enough

00:17:50.410 --> 00:17:54.269
ionization in the ionosphere to be able to refract

00:17:54.269 --> 00:17:57.410
the frequency you're on, to send it back to Earth

00:17:57.410 --> 00:18:01.450
so it can maybe go for another hop or do something

00:18:01.450 --> 00:18:04.470
even more exotic like ducting up in the ionosphere.

00:18:06.049 --> 00:18:09.819
The other issue is ionospheric absorption. In

00:18:09.819 --> 00:18:12.000
other words, I'm sure everyone's heard of the

00:18:12.000 --> 00:18:15.680
D region, and that's responsible solely for loss,

00:18:16.420 --> 00:18:21.339
signal strength loss during propagation. So it

00:18:21.339 --> 00:18:23.700
determines if you can hear that other station

00:18:23.700 --> 00:18:27.740
or not, and if he can hear you. Actually, there's

00:18:27.740 --> 00:18:29.960
really a third issue. It's called polarization,

00:18:31.359 --> 00:18:35.579
vertical, circular, horizontal, et cetera, elliptical.

00:18:36.269 --> 00:18:39.670
But that's less of a problem and it's usually

00:18:39.670 --> 00:18:42.750
not a big issue So most of the time we kind of

00:18:42.750 --> 00:18:46.170
ignored on HF at least when we get down to 160

00:18:46.170 --> 00:18:50.069
meters it starts getting important for some good

00:18:50.069 --> 00:18:54.490
physical reasons but Like I said the polarization

00:18:54.490 --> 00:18:56.369
is not a big issue, so I'm not going to worry

00:18:56.369 --> 00:19:02.849
about it too much Now as as cycle 24 approaches

00:19:02.849 --> 00:19:05.589
minimum we're gonna have We're going to have

00:19:05.589 --> 00:19:08.509
less and less openings on 10, 12, and 15 meters.

00:19:09.230 --> 00:19:10.990
Now you may wonder, how can we have any less

00:19:10.990 --> 00:19:14.849
than we're having right now, right? But generally

00:19:14.849 --> 00:19:18.690
North -South propagation is, it kind of happens

00:19:18.690 --> 00:19:21.289
on 10 meters. In fact, yesterday there are a

00:19:21.289 --> 00:19:24.269
lot of South Americans on up here. I could hear

00:19:24.269 --> 00:19:26.609
them up here in Fort Wayne, Indiana, which is

00:19:26.609 --> 00:19:30.990
up in the Northeast corner of the state. So 10

00:19:30.990 --> 00:19:34.230
meters is not. There's going to be a lot of nothing

00:19:34.230 --> 00:19:36.950
there, but at times there could be some good

00:19:36.950 --> 00:19:38.789
propagation. And of course, during the summer,

00:19:39.170 --> 00:19:42.549
you should always check 10 meters for sporadic

00:19:42.549 --> 00:19:46.490
E. That happens regardless of a solar cycle,

00:19:46.569 --> 00:19:50.970
where we are in a solar cycle. So don't give

00:19:50.970 --> 00:19:54.089
up completely. Every once in a while, exercise

00:19:54.089 --> 00:19:58.170
those band switches. In general, of course, the

00:19:58.170 --> 00:20:01.839
low bands seem to approve as we approach solar

00:20:01.839 --> 00:20:07.319
minimum. But recently there have been some interesting

00:20:07.319 --> 00:20:13.180
questions about this conventional wisdom. Many

00:20:13.180 --> 00:20:15.480
people have expected the low bands to be a lot

00:20:15.480 --> 00:20:19.200
better than they appear to be. Trying to figure

00:20:19.200 --> 00:20:23.059
out why they're not as good is kind of interesting.

00:20:23.700 --> 00:20:26.539
So who knows, maybe we'll learn something as

00:20:26.539 --> 00:20:29.500
we go through this solar min period. but I think

00:20:29.500 --> 00:20:33.319
the general takeaway is just for the next several

00:20:33.319 --> 00:20:38.000
years until cycle 25 gets going there's going

00:20:38.000 --> 00:20:40.319
to be few openings in the high bands and most

00:20:40.319 --> 00:20:45.019
of us are going to be well beyond the low bands

00:20:45.019 --> 00:20:50.940
you know 17, 20, 30, 40, 80 and 160. 20 and 17

00:20:50.940 --> 00:20:53.640
will probably be still be pretty good throughout

00:20:53.640 --> 00:20:56.490
the solar min period. Of course, they won't be

00:20:56.490 --> 00:20:58.750
as good as at solar max, but they'll still be

00:20:58.750 --> 00:21:02.250
worldwide DX opportunities. 40 and 30 ought to

00:21:02.250 --> 00:21:05.210
be really, really good. And hopefully 80 and

00:21:05.210 --> 00:21:09.569
160 will pick up. So for the next couple of years,

00:21:09.730 --> 00:21:13.869
move down in frequency is the advice. All right.

00:21:13.869 --> 00:21:24.500
Very good. That's what I'm hearing is 160. I

00:21:24.500 --> 00:21:27.079
can kind of cheat with my antenna and get 160,

00:21:27.460 --> 00:21:33.000
but that takes some wire. So you may want to

00:21:33.000 --> 00:21:36.960
think about that 160 antenna. Well, we're going

00:21:36.960 --> 00:21:39.599
to take a break. And when we come back, we're

00:21:39.599 --> 00:21:42.900
going to take your phone calls. So get ready

00:21:42.900 --> 00:21:47.579
to call in. The number is 812 -NET -HAM -1 and

00:21:47.579 --> 00:21:50.960
I'll be back to take your calls with Carl Lutzelschwaab

00:21:50.960 --> 00:21:53.819
right after this message from Tower Electronics

00:21:53.819 --> 00:21:57.839
right here on HamTalk Live. This episode of HamTalk

00:21:57.839 --> 00:22:00.880
Live is brought to you in part by Tower Electronics.

00:22:01.119 --> 00:22:03.539
Tower Electronics has been the Ham's Dime Store

00:22:03.539 --> 00:22:06.940
since 1978. When you need connectors, mobile

00:22:06.940 --> 00:22:10.200
and handheld antennas, cables, or adapters, visit

00:22:10.200 --> 00:22:13.779
Scott or Jill at a HamFest near you. Or you can

00:22:13.779 --> 00:22:19.980
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00:22:19.980 --> 00:22:25.000
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00:22:25.000 --> 00:22:28.259
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00:22:40.849 --> 00:22:44.089
Workman, and HamPro products. And don't miss

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00:22:48.150 --> 00:22:52.430
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00:22:52.430 --> 00:23:01.900
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00:23:01.900 --> 00:23:06.940
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00:23:06.940 --> 00:23:10.099
voice with Skype at HamTalk Live or give us a

00:23:10.099 --> 00:23:16.660
call at 812 -NET -HAM -1. That's 812 -638 -4261.

00:23:16.920 --> 00:23:21.019
Now here's more HamTalk Live. Thanks to Scott

00:23:21.019 --> 00:23:23.119
and Jill at Tower Electronics for sponsoring

00:23:23.119 --> 00:23:25.799
the show yet again tonight to help bring you

00:23:25.799 --> 00:23:28.910
HamTalk Live. They're back on the road. They'll

00:23:28.910 --> 00:23:31.710
be at the Fort Myers, Florida and St. Charles,

00:23:31.710 --> 00:23:35.690
Illinois ham fest this weekend. and Collinsville,

00:23:35.690 --> 00:23:39.390
Illinois and Arcadia, Florida next Saturday.

00:23:39.849 --> 00:23:46.509
Or you can call them at 920 -435 -2973 or visit

00:23:46.509 --> 00:23:51.089
them online at pl -259 .com. Tell them you heard

00:23:51.089 --> 00:23:54.170
it on HamTalk Live and be sure to listen to HamTalk

00:23:54.170 --> 00:23:57.230
Live Thursday nights at 9 p .m. Eastern time

00:23:57.230 --> 00:24:00.869
right here on HamTalkLive .com. Also check out

00:24:00.869 --> 00:24:03.029
our Facebook page and Twitter feed to search.

00:24:03.900 --> 00:24:09.019
For ham talk live. So now it's time for your

00:24:09.019 --> 00:24:12.460
questions. So if you have a question For Carl

00:24:12.460 --> 00:24:18.000
Lucil Schwab, K9LA, call 812 -NET -HAM -1. That's

00:24:18.000 --> 00:24:23.400
812 -638 -4261. Go ahead and call that right

00:24:23.400 --> 00:24:28.079
now. 812 -NET -HAM -1. Now is the time to call

00:24:28.079 --> 00:24:32.539
in. You can also Skype us. You can Skype us at

00:24:32.539 --> 00:24:37.980
HamTalk Live. So give us a call on Skype. and

00:24:37.980 --> 00:24:40.920
join the conversation, or if you'd rather type,

00:24:41.299 --> 00:24:45.859
you can tweet us. Over on Twitter, at HamTalkLive

00:24:45.859 --> 00:24:49.940
is our handle there. So if you have a question

00:24:49.940 --> 00:24:54.480
about propagation and sunspots, give us a call.

00:24:55.279 --> 00:24:58.240
And by the way, Carl, I've noticed you've been

00:24:58.240 --> 00:25:03.259
on the AWRL audio news lately, and my friend

00:25:03.259 --> 00:25:07.589
Sean Kutsko It seems to say your last name a

00:25:07.589 --> 00:25:10.589
lot. I think he just likes saying Lutzl Schwab.

00:25:11.549 --> 00:25:16.089
So a friend of mine mentioned that. For what

00:25:16.089 --> 00:25:18.170
it's worth, we've kind of Americanized it, I

00:25:18.170 --> 00:25:22.670
guess. We pronounce it Litzl Schwab. But they

00:25:22.670 --> 00:25:24.289
even pronounce it a different order in Switzerland.

00:25:25.799 --> 00:25:30.259
Yeah, so so what I thought I would do is See

00:25:30.259 --> 00:25:34.539
if I can outscore Sean and by saying Lutzl Schwab

00:25:34.539 --> 00:25:38.579
more times in the show Than he does so and maybe

00:25:38.579 --> 00:25:43.279
we'll maybe we'll have a contest And guess the

00:25:43.279 --> 00:25:46.779
number of times that I said Lutzl Schwab tonight,

00:25:46.779 --> 00:25:54.200
so We We used to see Sean quite a bit when he,

00:25:54.200 --> 00:25:57.400
of course, he lived in Nineland. But now that

00:25:57.400 --> 00:25:59.519
he's out at headquarters, we see him at Dayton

00:25:59.519 --> 00:26:02.559
and maybe some other ham fest, but that's about

00:26:02.559 --> 00:26:09.380
it. Yeah, he's got his hands full of all kinds

00:26:09.380 --> 00:26:13.779
of work out there in Connecticut, so he's abandoned

00:26:13.779 --> 00:26:17.619
us of Nineland. Yeah, he's done a lot of violence

00:26:17.619 --> 00:26:20.849
on the air, right? Yeah, islands on the air.

00:26:21.089 --> 00:26:23.630
Yeah, there we go. Yeah, he's having a lot of

00:26:23.630 --> 00:26:25.809
fun. Yeah, Parker, yeah. He's having lots of

00:26:25.809 --> 00:26:32.849
fun. All right, 812 -NATAM -1. 812 -638 -4261

00:26:32.849 --> 00:26:36.430
is the phone number for Carl Lutzelschwaab. I

00:26:36.430 --> 00:26:41.259
got it in there again. What are some... While

00:26:41.259 --> 00:26:44.000
we're waiting on the calls here to come in and

00:26:44.000 --> 00:26:46.960
questions, again, you can tweet us over at HamTalk

00:26:46.960 --> 00:26:51.619
Live on Twitter. What are some websites that

00:26:51.619 --> 00:26:56.099
people could go to to get the solar weather and

00:26:56.099 --> 00:27:00.380
propagation reports and that kind of thing? What

00:27:00.380 --> 00:27:03.160
are just some website addresses that you would

00:27:03.160 --> 00:27:07.640
suggest for people to check out? OK, well, as

00:27:07.640 --> 00:27:10.240
one might expect, there are quite a few out there.

00:27:10.750 --> 00:27:16.829
You know, the ARRL puts out a propagation bulletin

00:27:16.829 --> 00:27:21.589
every Friday and it's authored, it's edited by

00:27:21.589 --> 00:27:27.470
Tad K7RA. So he talks a lot about the numbers,

00:27:27.990 --> 00:27:34.490
sunspots, the geomagnetic field indices and also

00:27:34.490 --> 00:27:40.349
most of the time a lot of reader input. It's

00:27:40.349 --> 00:27:43.609
good practical information that you can read

00:27:43.609 --> 00:27:46.750
there. Of course, if you're a member of the ARRL,

00:27:46.869 --> 00:27:49.390
you can subscribe to that propagation bulletin

00:27:49.390 --> 00:27:51.410
for free, and it shows up in your email every

00:27:51.410 --> 00:27:56.289
week. Of course, CQ Magazine has a propagation

00:27:56.289 --> 00:28:01.230
column by Thomas NW7US. Lots of good info there.

00:28:01.829 --> 00:28:03.789
Now, if you're just looking on the web for some

00:28:03.789 --> 00:28:08.170
websites, spaceweather .com. Space weather is

00:28:08.170 --> 00:28:13.730
all one word. There are lots of measurements

00:28:13.730 --> 00:28:17.990
on the left side of their homepage, and in the

00:28:17.990 --> 00:28:20.369
center is usually lots of good discussion on

00:28:20.369 --> 00:28:26.609
various issues. One of the ones that has just

00:28:26.609 --> 00:28:31.670
mucho information is the Space Weather Prediction

00:28:31.670 --> 00:28:35.269
Center in Boulder, Colorado. Their website is

00:28:35.269 --> 00:28:47.579
www .swpc .com. So swpc .noaa .com. And they

00:28:47.579 --> 00:28:50.380
have lots of measurements, they have models,

00:28:50.599 --> 00:28:53.480
they have lots of tutorials to help you understand

00:28:53.480 --> 00:28:57.640
what all these measurements mean. I believe that's

00:28:57.640 --> 00:29:00.549
.gov. If I remember right. Yeah, you're right.

00:29:01.869 --> 00:29:08.190
And apparently we've got some sunspots on the

00:29:08.190 --> 00:29:11.910
line here. Your audio is breaking up a little

00:29:11.910 --> 00:29:17.230
bit. Well, okay, maybe it's not sunspots. So

00:29:17.230 --> 00:29:21.250
we apologize for that, but keep on going. We're

00:29:21.250 --> 00:29:25.990
in good shape here. Okay. Also www .qrz .com

00:29:25.990 --> 00:29:31.109
has a little panel. shows solar terrestrial data.

00:29:34.150 --> 00:29:38.750
Another good site is www .solarham .net. It has

00:29:38.750 --> 00:29:41.910
lots of data. And there are many more out there,

00:29:42.289 --> 00:29:44.609
and I'm sorry if I didn't include maybe some

00:29:44.609 --> 00:29:48.710
of your favorites, but they're all over the place.

00:29:50.269 --> 00:29:53.210
It's kind of like propagation prediction programs.

00:29:53.470 --> 00:29:56.970
They're all The same, it's the bells and whistles

00:29:56.970 --> 00:29:59.390
and how they present the data that's different.

00:29:59.910 --> 00:30:01.630
And that's what I think you'll find with all

00:30:01.630 --> 00:30:05.750
these websites, a lot of common data, how they

00:30:05.750 --> 00:30:09.130
present it. And of course that says you'll probably

00:30:09.130 --> 00:30:12.049
feel more comfortable with maybe a certain website

00:30:12.049 --> 00:30:16.029
and kind of stick to that. Yeah. And I like to

00:30:16.029 --> 00:30:19.390
follow Dr. Tamatha Scov too, over at spaceweather

00:30:19.390 --> 00:30:23.829
.tv. She does a great job on the visuals and

00:30:24.430 --> 00:30:27.450
some good stuff there too so all kinds of stuff

00:30:27.450 --> 00:30:31.950
out there to take a look at so those are some

00:30:31.950 --> 00:30:35.009
some great resources and I will put a list of

00:30:35.009 --> 00:30:37.809
those together and send those out on on Twitter

00:30:37.809 --> 00:30:41.509
and Facebook after the show so you can get a

00:30:41.509 --> 00:30:45.029
hold of those again if you missed those so those

00:30:45.029 --> 00:30:49.069
will be up on Facebook and Twitter afterwards

00:30:49.940 --> 00:30:56.740
812 Net Ham 1 is the phone number 812 -638 -4261

00:30:56.740 --> 00:31:04.119
or you can tweet us over at Twitter at HamTalk

00:31:04.119 --> 00:31:07.980
Live or you can call us on Skype at HamTalk Live

00:31:07.980 --> 00:31:12.339
if you have a question. One other thing that

00:31:12.339 --> 00:31:17.880
I've always wondered in listening to the W1AW

00:31:17.880 --> 00:31:21.779
bulletins, we always have the sunspot numbers

00:31:21.779 --> 00:31:26.319
at the end. Today's sunspot numbers are, I kind

00:31:26.319 --> 00:31:30.200
of think sometimes it's kind of like a fortune

00:31:30.200 --> 00:31:32.700
cookie, you know, your lucky numbers for today

00:31:32.700 --> 00:31:38.160
are 2478, you know. What are those sunspot numbers

00:31:38.160 --> 00:31:42.819
that they give out on the W1AW bulletins and

00:31:42.819 --> 00:31:47.299
how can we use those to help figure this stuff

00:31:47.299 --> 00:31:49.839
out? Okay, yeah, that's a good question, Neil.

00:31:51.539 --> 00:31:54.220
Those numbers are, you know, what we observe.

00:31:55.640 --> 00:31:58.180
And you have to realize that sunspot, counting

00:31:58.180 --> 00:32:02.220
sunspots is subjective. You know, humans do it,

00:32:02.240 --> 00:32:05.210
so there can be biases in there. And of course

00:32:05.210 --> 00:32:07.869
it depends on how good your telescope is, the

00:32:07.869 --> 00:32:11.150
sky cover, etc. And that's why they use a bunch

00:32:11.150 --> 00:32:14.509
of observatories to come up with a sunspot number.

00:32:14.549 --> 00:32:16.789
Hold on here, the cat's getting twisted in the

00:32:16.789 --> 00:32:19.910
headphone. Uh -oh. Yeah, one of the cats is active,

00:32:20.009 --> 00:32:24.450
but okay. It's not the first time that's happened

00:32:24.450 --> 00:32:31.369
on the show, by the way. So we count sunspots,

00:32:31.789 --> 00:32:35.619
which are subjective. But we try and you know

00:32:35.619 --> 00:32:40.700
get them as right as we can Of course there's

00:32:40.700 --> 00:32:44.799
another solar parameter It's called the 10 .7

00:32:44.799 --> 00:32:48.539
centimeter solar flux that is measured so it's

00:32:48.539 --> 00:32:53.099
much more of a an objective measurement and Of

00:32:53.099 --> 00:32:55.119
course you have to keep your you know the receiver

00:32:55.119 --> 00:32:58.579
and the calibrated etc and all that but still

00:32:58.579 --> 00:33:01.720
it's there's no human interpretation involved

00:33:01.720 --> 00:33:06.809
now sunspots and the 10 .7 centimeter solar flux

00:33:06.809 --> 00:33:11.569
are proxies for the true ionizing radiation,

00:33:11.930 --> 00:33:14.730
which is at much, much shorter wavelengths than

00:33:14.730 --> 00:33:20.269
10 .7 centimeters. But there are relationships

00:33:20.269 --> 00:33:28.130
that relate sunspots to 10 .7 centimeter solar

00:33:28.130 --> 00:33:31.150
flux. You'll probably find those on that NOAA

00:33:31.150 --> 00:33:37.259
.gov website. So, we use those numbers to get

00:33:37.259 --> 00:33:41.839
a general picture of what propagation is like.

00:33:43.119 --> 00:33:46.680
Generally, we'd like very high sunspot numbers,

00:33:47.079 --> 00:33:50.880
very high 10 .7 centimeter solar flux. That would

00:33:50.880 --> 00:33:54.579
make the higher bands like 15, 12, and 10 very

00:33:54.579 --> 00:34:00.700
good for worldwide communications. In general,

00:34:01.079 --> 00:34:04.000
if the sunspot number is greater than about 50

00:34:04.000 --> 00:34:07.779
or so, then 10 meters has a chance of being open.

00:34:09.340 --> 00:34:13.019
If the sunspot number is only around 35, it suggests,

00:34:13.019 --> 00:34:15.480
okay, well, 15 meters at least should be open.

00:34:16.219 --> 00:34:18.960
Those are some rough numbers, and they also correspond

00:34:18.960 --> 00:34:23.780
to solar fluxes. If the solar flux is greater

00:34:23.780 --> 00:34:26.179
than about 100, then 10 meters is open. If it's

00:34:26.179 --> 00:34:29.679
greater, about 90. It's at least 15 meters will

00:34:29.679 --> 00:34:33.440
be open. So we use those. And of course, this

00:34:33.440 --> 00:34:37.099
brings us into the propagation prediction programs

00:34:37.099 --> 00:34:40.320
that are available. There are many of them out

00:34:40.320 --> 00:34:45.300
there. There's W6ELProp. It's free download.

00:34:47.360 --> 00:34:50.519
And on my website is a tutorial on how to download

00:34:50.519 --> 00:34:54.559
it and use it and interpret it. Also the Voice

00:34:54.559 --> 00:34:58.579
of America program, VOA Cap. is also a free download

00:34:58.579 --> 00:35:02.340
on the website. Just do a Google search and you'll

00:35:02.340 --> 00:35:12.159
find that program. There's a tutorial on my website

00:35:12.159 --> 00:35:17.440
at k9la .us for how to download it, set it up

00:35:17.440 --> 00:35:21.039
and use it and interpret it. We have to remember

00:35:21.039 --> 00:35:24.179
that our understanding of the ionosphere is statistical

00:35:24.179 --> 00:35:30.369
in nature. Unfortunately, a given sunspot number

00:35:30.369 --> 00:35:34.510
or solar flux number does not map to a unique

00:35:34.510 --> 00:35:38.929
level of ionization of the ionosphere. So you

00:35:38.929 --> 00:35:40.989
just have to remember that our predictions are

00:35:40.989 --> 00:35:44.449
statistical over a month's time frame. And once

00:35:44.449 --> 00:35:47.469
you understand that, they begin to make sense.

00:35:47.469 --> 00:35:50.929
And you can do some planning on what's the best

00:35:50.929 --> 00:35:55.480
band to talk to Uncle Joe over there. in maybe

00:35:55.480 --> 00:36:00.679
Arizona or something. So using the sunspot numbers

00:36:00.679 --> 00:36:04.059
is just gives an indication of where what bands

00:36:04.059 --> 00:36:08.579
might be open. The lower bands, generally the

00:36:08.579 --> 00:36:11.679
ionization is always high enough that you don't

00:36:11.679 --> 00:36:15.719
have to worry about the level of ionization.

00:36:16.019 --> 00:36:18.199
There's always enough to refract those lower

00:36:18.199 --> 00:36:21.219
frequencies back to Earth and all you're left

00:36:21.219 --> 00:36:25.750
with is how much absorption is there, and will

00:36:25.750 --> 00:36:30.010
it put the signal below your noise, which generally

00:36:30.010 --> 00:36:34.570
is limited by external noise around you, man

00:36:34.570 --> 00:36:38.909
-made noise and atmospheric noise. Also in the

00:36:38.909 --> 00:36:43.369
bulletins are the geomagnetic indices, the K

00:36:43.369 --> 00:36:48.130
index and the A index. The K index is a three

00:36:48.130 --> 00:36:51.150
hour index of how the magnetic field of the Earth

00:36:51.150 --> 00:36:56.070
is varying or being disturbed. The A index is

00:36:56.070 --> 00:37:02.510
essentially the average of the eight three -hour

00:37:02.510 --> 00:37:07.889
K indices. So it tells you if the ionosphere

00:37:07.889 --> 00:37:11.010
is disturbed or not. In general, we'd like a

00:37:11.010 --> 00:37:13.769
quiet magnetic field, which means a low A and

00:37:13.769 --> 00:37:18.750
K indices. But of course, there are always exceptions.

00:37:19.849 --> 00:37:26.670
Sometimes high A and K indices are useful, like

00:37:26.670 --> 00:37:32.309
aurora at VHF frequencies. Sometimes the ionosphere

00:37:32.309 --> 00:37:38.570
can be enhanced at low latitudes by elevated

00:37:38.570 --> 00:37:44.070
K indices. So there are some general guidelines

00:37:44.070 --> 00:37:47.489
to follow, but just understand that it's a very

00:37:47.489 --> 00:37:51.130
complicated system up there. A lot of interesting

00:37:51.130 --> 00:37:53.329
things happen and the more you know about them

00:37:53.329 --> 00:37:55.849
the more you may be prepared to work something

00:37:55.849 --> 00:38:00.070
that your friends may not work. Carl Lutzl Schwab,

00:38:00.289 --> 00:38:03.690
K9LA is our guest. You can call in and ask him

00:38:03.690 --> 00:38:08.610
a question at 812 -NET -HAM -1. That's 812 -638

00:38:08.610 --> 00:38:12.570
-4261. We have just a few minutes remaining,

00:38:12.630 --> 00:38:16.670
so give us a call on there or on Skype. Give

00:38:16.670 --> 00:38:21.349
us an audio call or you can tweet us over on

00:38:21.349 --> 00:38:26.409
Twitter at HamTalk Live. One other thing I just

00:38:26.409 --> 00:38:33.349
thought of. Carl is Most of the time I'm in a

00:38:33.349 --> 00:38:39.969
hurry, you know either in a contest or I've got

00:38:39.969 --> 00:38:45.909
a few minutes to check things before I Go upstairs

00:38:45.909 --> 00:38:49.510
to the ham shack at school and get the kids on

00:38:49.510 --> 00:38:54.190
the air and So I go over to DX Summit or QRZ

00:38:54.190 --> 00:38:58.130
and look at that little You know band conditions

00:38:58.130 --> 00:39:03.730
thing and observed and predicted and and Sometimes

00:39:03.730 --> 00:39:08.489
it seems like that's accurate and and sometimes

00:39:08.489 --> 00:39:12.670
it doesn't So I'm wondering how much of that

00:39:12.670 --> 00:39:16.889
is Is just kind of like whether it's it's predicted

00:39:16.889 --> 00:39:23.389
and how much of that is is pure measurement Well

00:39:23.389 --> 00:39:28.280
most I think most of it is pure measurement Interestingly,

00:39:28.679 --> 00:39:33.019
the ionosphere varies on a day -to -day basis

00:39:33.019 --> 00:39:39.460
quite a bit. Although solar radiation instigates

00:39:39.460 --> 00:39:45.980
the ionization process, the condition of the

00:39:45.980 --> 00:39:50.480
Earth's magnetic field also comes into play in

00:39:50.480 --> 00:39:52.960
determining how much ionization there is at a

00:39:52.960 --> 00:39:56.260
given point, at a given time. And interestingly,

00:39:56.559 --> 00:40:00.239
we're discovering and doing much more research

00:40:00.239 --> 00:40:05.739
in events that happen in the lower atmosphere

00:40:05.739 --> 00:40:08.780
that couple up to the ionosphere and they have

00:40:08.780 --> 00:40:12.380
an impact on what the ionization is. So, you

00:40:12.380 --> 00:40:14.579
know, since we don't understand that, that's

00:40:14.579 --> 00:40:17.380
why we have a statistical model of the ionosphere.

00:40:20.110 --> 00:40:25.110
The best way to understand predictions are to

00:40:25.110 --> 00:40:29.809
realize that they're probably monthly median

00:40:29.809 --> 00:40:34.170
value, in other words, kind of almost like an

00:40:34.170 --> 00:40:37.949
average over a month's time frame. So on any

00:40:37.949 --> 00:40:41.769
given day within that month's time frame, it

00:40:41.769 --> 00:40:46.730
could be, you know, 10 to 30 % different, 10

00:40:46.730 --> 00:40:52.929
% higher to 30 % lower. So it's tough to predict

00:40:52.929 --> 00:40:58.570
propagation on a very short -term basis. In other

00:40:58.570 --> 00:41:01.429
words, what's happening today? We just don't

00:41:01.429 --> 00:41:05.030
have it yet. Of course, there's lots of work

00:41:05.030 --> 00:41:11.510
by the military, et cetera, in taking measurements

00:41:11.510 --> 00:41:15.789
from ionosans. and total electron content from

00:41:15.789 --> 00:41:21.469
GPS systems and assimilate that into a model

00:41:21.469 --> 00:41:25.590
to try and get a more up -to -date picture. I'm

00:41:25.590 --> 00:41:27.730
sure we'll see more and more to that and I know

00:41:27.730 --> 00:41:31.710
many universities are working on physical models

00:41:31.710 --> 00:41:33.929
of the ionosphere and the atmosphere, well the

00:41:33.929 --> 00:41:37.570
atmosphere really, that will hopefully give us

00:41:37.570 --> 00:41:41.780
what's the ionosphere doing right now. I find

00:41:41.780 --> 00:41:43.960
the best way to go find out how the bands are

00:41:43.960 --> 00:41:49.179
doing is, you know, I monitor a packet cluster.

00:41:49.900 --> 00:41:53.059
You know, it shows, you know, stations spot other

00:41:53.059 --> 00:41:56.260
stations. And that gives me a general, a good

00:41:56.260 --> 00:41:59.360
idea what the band is doing right now. On the

00:41:59.360 --> 00:42:04.300
higher bands, there are also the IARUNCDXF beacon

00:42:04.300 --> 00:42:09.980
system, where in a three -minute period, you

00:42:09.980 --> 00:42:13.320
could assess worldwide propagation on a given

00:42:13.320 --> 00:42:19.079
band because there are 18 beacons scattered all

00:42:19.079 --> 00:42:21.780
throughout the world. So that'll give you a good

00:42:21.780 --> 00:42:25.300
idea what's going on on 20, 17, 15, 12, and 10

00:42:25.300 --> 00:42:27.480
meters. Unfortunately, we don't have anything

00:42:27.480 --> 00:42:33.159
on the lower bands. But maybe someday we will.

00:42:33.719 --> 00:42:36.719
But there are ways to assess short -term what

00:42:36.719 --> 00:42:39.460
the bands are like. But those predictions you

00:42:39.460 --> 00:42:43.940
see on all the websites are just general. And

00:42:43.940 --> 00:42:47.460
realize that maybe one band up or down could

00:42:47.460 --> 00:42:52.139
really be what's happening. Just based on the

00:42:52.139 --> 00:42:56.079
predictions. All right. Very good. Well, thank

00:42:56.079 --> 00:42:58.440
you so much for coming on. We're just about out

00:42:58.440 --> 00:43:03.679
of time. So thank you for doing that. And I will

00:43:03.679 --> 00:43:07.739
get those websites up. online here after the

00:43:07.739 --> 00:43:12.260
show. So that is wrap for this week's edition

00:43:12.260 --> 00:43:15.000
of Ham Talk Live. I'd like to thank my guest

00:43:15.000 --> 00:43:18.619
Carl Lutzelschwaab, K9LA, and everyone out there

00:43:18.619 --> 00:43:21.460
in cyberspace for listening and calling in and

00:43:21.460 --> 00:43:24.019
invite you all back next Thursday night at 9

00:43:24.019 --> 00:43:27.239
p .m. Eastern Time when Richard Garriott de Caillou,

00:43:27.239 --> 00:43:31.619
W5KWQ, will be here to talk about operating ham

00:43:31.619 --> 00:43:35.929
radio from space and his new book called explore,

00:43:35.929 --> 00:43:39.530
create. Richard was one of the first space tourists

00:43:39.530 --> 00:43:42.949
on the International Space Station and the old

00:43:42.949 --> 00:43:46.389
timers like me may remember his father Owen W5LFL

00:43:46.389 --> 00:43:50.110
who was an astronaut on Skylab and the space

00:43:50.110 --> 00:43:52.329
shuttle and was the first to operate ham radio

00:43:52.329 --> 00:43:54.829
from space so I'm sure we'll talk a little bit

00:43:54.829 --> 00:43:58.750
about his dad as well and for a list of all of

00:43:58.750 --> 00:44:02.329
our upcoming guests visit hamtalklive .com and

00:44:02.329 --> 00:44:05.289
just click on the link there. For now, this is

00:44:05.289 --> 00:44:10.670
Neil Rapp, WB9VPG, saying 7 -3, 7 -5, and, as

00:44:10.670 --> 00:44:51.159
always, may the good DX be yours. 73, and good

00:44:51.159 --> 00:44:53.360
luck from HamTalk Live.
