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amateur for more information about ICOM radios.

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Good evening, everyone. It's time for HamTalk

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Live. It's episode number 184, the HamSci WWV

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Festival of Frequency Measurements, recorded

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live on Thursday, October 3rd, 2019. I'm your

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host, Neil Rapp, WB9VPG. Thanks for tuning in

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to this episode of HamTalk Live. Tonight we're

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joined by Dr. Nathaniel Frisell, W2NAF. and we'll

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take your calls live in just a few minutes. Last

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week, Joe Karsha, NJ1Q, and Michelle Patnode,

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W3MVP, were here to talk about the So Now What

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podcast from ARRL. And if you missed the show,

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you can listen anytime over at hamptalklive .com

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or on your favorite podcast app. or on YouTube,

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or you can catch the rebroadcast on WTWW, that's

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5085 AM Saturday mornings or Saturday evenings

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rather, at about 630 PM Eastern Time. Before

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we take a break here. Hey, don't forget about

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fallout. It's the 100 watts of the wire podcast

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fallout. That's October 11th through the 13th

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and Christian K zero STH is encouraging everyone

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to get outdoors and enjoy some radio before the

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chill arrives here in the US. And while it's

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not a contest, there are some prizes and points.

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So go over to 100watsandawire .com slash activities

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and check out all the information there on Fallout.

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Get outside next weekend and participate. So

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I'll be back with Nathaniel right after this

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word from ICOM right here on HamTalk Live. Heard

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For more information on ICOM radios, be sure

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to visit 5 out of 4 people have trouble with

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fractions. Now, here's Neil Rapp with more HamTalk

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Live. Thanks to ICOM for bringing HamTalk Live

00:05:43.470 --> 00:05:46.990
your way. Be sure to check them out at icomamerica

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.com slash amateur. Our guest tonight is Dr.

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Nathaniel Frisell, W2NAF. He is now an assistant

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professor at the University of Scranton in physics,

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where he teaches digital signal processing. fundamental

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physics and electromagnetics. He is the lead

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organizer of HamSci, a project that explores

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how amateur radio can help us understand more

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about the physics of the ionosphere. Nathaniel

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completed his PhD in electrical engineering in

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spring 2016 at the Superdarn HF Radar Laboratory

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at Virginia Tech. He was also involved in the

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Virginia Tech Amateur Radio Association, where

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he coordinated the VE team. And his interests

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include HF, CW, HF propagation, and radio scouting,

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including involvement at the W2FSR station at

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Forestburg Scout Reservation in New York, as

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well as working on the K2BSA staff at the National

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Scout Jamboree. And so, Nathaniel, welcome back.

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Thank you so much, Neil. It's a pleasure to be

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here. Well, it's always good to have you back

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here and last time I think was for your big award

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so congratulations again on on being the ham

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vincen amateur of the year and I really like

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this and before the show we were already talking

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all this science stuff uh... the science geeks

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were you know we gotta ask all these all these

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technical science questions and so we weren't

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going to bore everybody with those on the show

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here tonight but uh... we're already talking

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about this uh... this new project but and we'll

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talk about that here in just a second but but

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first how's the the move going you you were in

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g i t and now uh... you just started the new

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gig over at Scranton and you're back to teaching.

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You're back in the classroom again trying to

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balance the workload between the classroom and

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your research. So how's it all going? That's

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right, Neil. I think things are going fine. So

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I'm teaching a couple lectures and a couple of

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labs this semester and I have a few undergraduate

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research students working with me as well. One

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of them I was able to bring to the Tapper Digital

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Communications Conference last week and another

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one is working on a project that we're going

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to send some HF radio receivers down to Antarctica

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again and that's through a collaboration with

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MJIT. So I think things are coming along just

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fine. Over. All right, very good. Well, you know,

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it's it's always a challenge and I was sharing

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with you before the show, you know, some of the

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things that happened in the classroom like 311

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,000 percent error, you know that there might

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be something wrong there. There might be And

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I'm learning that too now as I'm teaching a physics

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one class You know some of the students are are

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really quite bright You just give an exam and

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we had a few students just you know walk away

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with perfect Perfect exams and other students

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they struggle a little bit more But hopefully

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they'll all get to where they need to be by the

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end if they figure out f equals ma then Life

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is good That's right And that vector math, you

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know the vector and vectors. Yes, I told them

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I like so much of this class is just knowing

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how to manipulate vectors properly Yeah, I brought

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up the the V word in class the other day we're

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talking about Polarity and molecules and I was

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like, yeah, you can, you can figure out the resultant

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dipole and they're like, Oh no, not that word

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again. Well, let's talk about this WWV. I love

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the name. It's the, the festival of frequency

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measurements. It just, it just has a ring to

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it. So tell us about what it is and who's participating

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and what you hope to learn out of this. Sure.

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Neil. So the WWV centennial festival of frequency

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measurements is a science activity that goes

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along with WWV's 100th anniversary celebrations.

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And the idea of doing the festival frequency

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measurements, both the name and the idea for

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doing this particular experiment, really came

00:10:39.019 --> 00:10:43.460
from David Kasdan, Alpha Delta 8 Yankee, at the

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Case Western Reserve University Case Amateur

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Radio Club, W8EDU. So both he and his students

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have really been leading the charge in making

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sure this happens. asks participants to do is

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to measure the Doppler shift at their station

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of the 5 MHz frequency. And when you do that,

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you'll find out that even though WWV has a very,

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very stable and accurate 5 MHz carrier, what

00:11:21.440 --> 00:11:25.159
you actually receive in your own backyard is

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not stable and not right at 5 MHz. There's a

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substantial amount of frequency shift to be seen.

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And that frequency shift can very often be attributed

00:11:35.679 --> 00:11:40.649
to variations occurring in the ionosphere. Very

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good. So how do you go about taking all these

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measurements and crowdsourcing them? So there

00:11:47.809 --> 00:11:51.370
is a frequency measurement experiment page on

00:11:51.370 --> 00:11:54.309
HamSci .org. If you go to HamSci .org there's

00:11:54.309 --> 00:11:56.909
a news or blog post up right now about this and

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then there's a link to a procedure page and on

00:12:00.230 --> 00:12:04.080
the procedure page it explains how you're going

00:12:04.080 --> 00:12:05.779
to set up your equipment and what you're going

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to measure. Some of the important things here

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is you can use almost any receiver, but you do

00:12:13.899 --> 00:12:19.059
have to have some sort of very stable oscillator

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to measure against. And one popular choice these

00:12:24.100 --> 00:12:26.960
days are GPS -disciplined oscillators, which

00:12:26.960 --> 00:12:32.120
actually synchronize with the GPS network of

00:12:32.120 --> 00:12:36.360
satellites and they can use that to steer or

00:12:36.360 --> 00:12:38.720
discipline a local oscillator and you can get

00:12:38.720 --> 00:12:42.940
a very stable local oscillator almost to the

00:12:42.940 --> 00:12:46.000
caliber of being a piece of test equipment and

00:12:46.000 --> 00:12:49.440
then you can feed that into your radio and you

00:12:49.440 --> 00:12:53.600
can use that to compare that signal with the

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one coming in from WWV and that can allow you

00:12:57.460 --> 00:13:01.360
to record the Doppler shift measurements. You

00:13:01.360 --> 00:13:03.980
often use a program, there's a program called

00:13:03.980 --> 00:13:07.019
Spectrum Lab. You can either use that or even

00:13:07.019 --> 00:13:11.019
the frequency measurement utility within FL Digi.

00:13:11.259 --> 00:13:14.120
Those are both ways that you can record the data

00:13:14.120 --> 00:13:16.559
to the computer and then you're going to want

00:13:16.559 --> 00:13:20.980
to upload those observations to a data repository

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site called Zenodo where we have a HamSci community

00:13:24.600 --> 00:13:29.659
page. So you're gonna gather all this data on

00:13:29.659 --> 00:13:32.700
the Doppler shift and what are you what are you

00:13:32.700 --> 00:13:35.580
hoping to find from this? Well, we're really

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hoping to learn about new ionospheric dynamics

00:13:39.500 --> 00:13:43.440
that maybe we don't know about or maybe we know

00:13:43.440 --> 00:13:47.240
about but don't understand and There's a whole

00:13:47.240 --> 00:13:51.519
zoo of different things out there different phenomena

00:13:51.519 --> 00:13:55.620
Things such as traveling on a spirit disturbances

00:13:56.360 --> 00:14:01.960
You can see changes due to the sunrise and sunset,

00:14:02.659 --> 00:14:05.100
other things as well. Some of these things I

00:14:05.100 --> 00:14:07.659
mentioned, like traveling atmospheric disturbances,

00:14:07.940 --> 00:14:10.320
that's a very generic term. There's a lot of

00:14:10.320 --> 00:14:14.059
things that can cause them. So not all the traveling

00:14:14.059 --> 00:14:17.480
atmospheric disturbances are the same. So by

00:14:17.480 --> 00:14:20.559
looking at these measurements, we might be able

00:14:20.559 --> 00:14:27.200
to learn something new. Okay, so have you I mean

00:14:27.200 --> 00:14:31.259
it's just happened in what two days now right

00:14:31.259 --> 00:14:35.240
since yeah, it's the anniversary of WWV which

00:14:35.240 --> 00:14:38.659
we were fortunate enough to have a couple of

00:14:38.659 --> 00:14:43.059
those guys from the special event station on

00:14:43.059 --> 00:14:47.080
here a couple of weeks ago, but Have you been

00:14:47.080 --> 00:14:49.779
able to gather anything out of the dated already?

00:14:50.379 --> 00:14:54.320
Yes, so we have so far and that's really thanks

00:14:54.320 --> 00:14:58.639
to some very good volunteers that we have participating

00:14:59.759 --> 00:15:03.639
So on the Zenodo website, and again, you can

00:15:03.639 --> 00:15:07.100
get to a link to that from hamsci .org, on the

00:15:07.100 --> 00:15:10.100
Zenodo repository, we have about 40 submissions

00:15:10.100 --> 00:15:13.639
from many different places, many different operators

00:15:13.639 --> 00:15:17.679
providing data. And some of them have even presented

00:15:17.679 --> 00:15:22.220
their data in a presentation form. So one very

00:15:22.220 --> 00:15:26.120
nice presentation comes from an amateur Steve

00:15:26.120 --> 00:15:30.019
Sirwin, whiskey off a five, foxtrot, Romeo foxtrot,

00:15:30.360 --> 00:15:33.559
and he lives in San Antonio, Texas, so he's measuring

00:15:33.559 --> 00:15:36.379
the path between Fort Collins, Colorado, where

00:15:36.379 --> 00:15:39.399
WWV is, to his station in San Antonio, Texas,

00:15:39.740 --> 00:15:42.240
and he has absolutely beautiful figures which

00:15:42.240 --> 00:15:46.519
show the Doppler shift changes at dusk and dawn,

00:15:46.820 --> 00:15:51.480
and it shows that you see very few changes. in

00:15:51.480 --> 00:15:54.019
the five megahertz signal during the day. But

00:15:54.019 --> 00:15:58.720
if you look at night, you do have quite prominent,

00:16:00.139 --> 00:16:03.039
quite a bit of ionospheric variability there,

00:16:03.299 --> 00:16:06.100
which looks like traveling ionospheric disturbances.

00:16:07.379 --> 00:16:10.080
I'm looking at the figure now. It looks like

00:16:10.080 --> 00:16:13.639
there's about a, it's about one hertz peak to

00:16:13.639 --> 00:16:20.649
peak Doppler shift on the signal. Yeah, I took

00:16:20.649 --> 00:16:23.490
a real quick glance at it right before the show

00:16:23.490 --> 00:16:27.549
and and it was it was pretty pronounced So yeah,

00:16:28.129 --> 00:16:30.289
I mean this is hot you're on to something here.

00:16:30.289 --> 00:16:33.230
Yeah, this is hot off the press really I mean

00:16:33.230 --> 00:16:35.429
Steve just sent this this morning just posted

00:16:35.429 --> 00:16:40.450
it on Zenodo today and yeah, anyone who goes

00:16:40.450 --> 00:16:45.110
to the Hamside Oregon is a nodo and searches

00:16:45.110 --> 00:16:48.860
for Whiskey Alpha -5, Foxtrot, Romeo, Foxtrot,

00:16:48.980 --> 00:16:53.220
WA -5, FRF, and there's a Noto repository. They'll

00:16:53.220 --> 00:16:57.460
be able to see his PowerPoint, or the PDF of

00:16:57.460 --> 00:16:59.879
his PowerPoint there, and it's very clear the

00:16:59.879 --> 00:17:02.820
difference between day and night. It's as clear

00:17:02.820 --> 00:17:06.819
as day and night, really. Yeah, it's very pronounced.

00:17:08.259 --> 00:17:12.119
You're getting some good stuff. Yeah, so a couple

00:17:12.119 --> 00:17:14.700
things I want to point out about this is, first

00:17:14.700 --> 00:17:19.990
of all, As much as we do know about the ionosphere

00:17:19.990 --> 00:17:23.569
and space, there's so much that we still do not

00:17:23.569 --> 00:17:26.990
know and we haven't been able to really observe

00:17:26.990 --> 00:17:31.269
well. This is a great case of this because I

00:17:31.269 --> 00:17:35.369
showed these slides to my friend Dr. Phil Erickson,

00:17:35.450 --> 00:17:38.849
WNPJE, who's up at the MIT Haystack Observatory.

00:17:39.009 --> 00:17:42.029
I'm like, Phil, have you seen these types of

00:17:42.029 --> 00:17:45.119
oscillations or variability? at nighttime, do

00:17:45.119 --> 00:17:47.019
you know what this is from? And he said, you

00:17:47.019 --> 00:17:51.180
know, Nathaniel, no, I really don't. And if you

00:17:51.180 --> 00:17:54.119
do a Google Scholar search for nighttime MSTIDs,

00:17:54.119 --> 00:17:57.220
you'll see a lot of optical observations, airglow

00:17:57.220 --> 00:18:03.039
observations. But these five megahertz HF observations,

00:18:03.400 --> 00:18:05.900
you know, they're really kind of unique. I don't

00:18:05.900 --> 00:18:09.079
think they have been studied very much professionally.

00:18:09.779 --> 00:18:13.480
So this is something you know, that's a real

00:18:13.480 --> 00:18:16.940
contribution we can have to professional science.

00:18:18.980 --> 00:18:23.380
And that's, you know, being a science teacher

00:18:23.380 --> 00:18:28.039
and having a degree, you know, in chemistry,

00:18:28.400 --> 00:18:33.880
that's always been a connection for me is, you

00:18:33.880 --> 00:18:38.480
know, the ham radio aspects of science. And this

00:18:38.480 --> 00:18:42.339
brings them together and it's just It's just

00:18:42.339 --> 00:18:47.240
really exciting to hear that this is happening

00:18:47.240 --> 00:18:54.140
in mass quantities. Yeah, it's really very exciting.

00:18:55.599 --> 00:18:58.200
Well, you've done an excellent job of putting

00:18:58.200 --> 00:19:02.079
this stuff together and just look forward to

00:19:02.079 --> 00:19:05.059
hearing more about this and some of the plans

00:19:05.059 --> 00:19:08.099
that you have for the future. And now I understand

00:19:08.099 --> 00:19:14.049
you've got a a grant for a lot of this. Yeah,

00:19:14.269 --> 00:19:17.190
so it hasn't quite started yet actually, even

00:19:17.190 --> 00:19:21.710
though we've done so much. So these types of

00:19:21.710 --> 00:19:25.089
observations that people are making with the

00:19:25.089 --> 00:19:27.490
receivers and the GPS discipline oscillators

00:19:27.490 --> 00:19:30.569
that they already have, we're trying to develop

00:19:30.569 --> 00:19:35.490
a personal space weather station device that

00:19:35.490 --> 00:19:39.220
can basically standardize these types of measurements.

00:19:40.119 --> 00:19:45.319
We'd like to create a device that is built, designed

00:19:45.319 --> 00:19:48.640
from the ground up to address some of the scientific

00:19:48.640 --> 00:19:51.339
needs that a typical radio setup wouldn't have.

00:19:51.640 --> 00:19:54.819
Like it's going to have a high quality oscillator

00:19:54.819 --> 00:19:58.500
in it that's going to, GPS disciplined oscillator

00:19:58.500 --> 00:20:00.920
in it. It's going to have the ability to do time

00:20:00.920 --> 00:20:05.940
stamping. It's going to have the ability to measure

00:20:05.940 --> 00:20:09.900
multiple things at the same time and We would

00:20:09.900 --> 00:20:13.000
like to build this and be able to distribute

00:20:13.000 --> 00:20:15.640
it either distribute it or make it available

00:20:15.640 --> 00:20:19.039
to amateur radio operators really all over the

00:20:19.039 --> 00:20:21.720
world eventually and create a network that can

00:20:21.720 --> 00:20:25.940
very consistently make Measurements like the

00:20:25.940 --> 00:20:29.000
ones you're seeing from this WWE festival frequency

00:20:29.000 --> 00:20:33.319
measurement But we want to you know have them

00:20:33.279 --> 00:20:37.359
be more standardized and more carefully measured.

00:20:38.259 --> 00:20:42.039
So we just won a large NSF grant, $1 .3 million.

00:20:43.279 --> 00:20:46.420
It's a collaborative grant shared among a few

00:20:46.420 --> 00:20:49.099
different institutions. That's going to provide

00:20:49.099 --> 00:20:52.019
some funding to help develop a prototype for

00:20:52.019 --> 00:20:55.180
this particular personal space weather station.

00:20:57.119 --> 00:20:59.420
And one of the things that you learn in science

00:20:59.420 --> 00:21:03.210
is Sometimes, it all comes down to the funding.

00:21:04.829 --> 00:21:06.009
Congratulations on that. Well, you know, it certainly

00:21:06.009 --> 00:21:09.529
helps. Thank you. I mean, it helps on so many

00:21:09.529 --> 00:21:14.309
different levels because, really, we've been

00:21:14.309 --> 00:21:16.910
doing a lot of these projects on a volunteer

00:21:16.910 --> 00:21:19.289
basis. We have many volunteers who've been helping.

00:21:19.630 --> 00:21:22.269
But now that we have funding, it can accelerate

00:21:22.269 --> 00:21:26.450
the process. Even here at the university, the

00:21:26.450 --> 00:21:29.130
fact that I have funding actually gives me more

00:21:29.130 --> 00:21:32.740
time. And more justification to spend my time

00:21:32.740 --> 00:21:35.559
working on this project rather than some of the

00:21:35.559 --> 00:21:38.660
other responsibilities I might have so it really

00:21:38.660 --> 00:21:41.500
allows people to redirect their time to work

00:21:41.500 --> 00:21:44.900
on these things and and make it come together

00:21:44.900 --> 00:21:51.900
I Think something Yeah, and one thing I'm very

00:21:51.900 --> 00:21:55.240
excited about is the Collaborative nature of

00:21:55.240 --> 00:21:59.740
this so I've been working with the Tapper group.

00:22:00.039 --> 00:22:03.059
They're doing a lot of the engineering work on

00:22:03.059 --> 00:22:06.259
this project and that's where I was able to connect

00:22:06.259 --> 00:22:09.079
with a lot of the people who are working on this

00:22:09.079 --> 00:22:12.299
project. And so the TAPR portion of the project,

00:22:12.460 --> 00:22:15.420
they're calling it the Tangerine SDR, Software

00:22:15.420 --> 00:22:18.619
Defined Radio, and it's actually, the Tangerine

00:22:18.619 --> 00:22:21.559
SDR is going to be, you know, certainly to support

00:22:21.559 --> 00:22:23.339
the personal space weather station, but it's

00:22:23.339 --> 00:22:25.900
going to be modular so it can support other applications

00:22:25.900 --> 00:22:30.500
as well. We meet every Monday night at 9 p .m.

00:22:31.279 --> 00:22:34.359
Eastern on the internet on a team speak session

00:22:34.359 --> 00:22:36.900
and we have a list serve and that's where we're

00:22:36.900 --> 00:22:39.160
able to do a lot of our collaborative development.

00:22:39.359 --> 00:22:42.819
And then we meet twice a year once at the Tapper

00:22:42.819 --> 00:22:45.160
Digital Communications Conference which just

00:22:45.160 --> 00:22:49.400
happened in Detroit last weekend. And then again

00:22:49.400 --> 00:22:51.859
at the HamSci workshop which is going to happen

00:22:51.859 --> 00:22:56.380
in Scranton this March 20th and 21st. to continue

00:22:56.380 --> 00:23:00.500
the development of this project. Oh, that sounds

00:23:00.500 --> 00:23:05.220
like a fabulous project and glad to hear that

00:23:05.220 --> 00:23:09.339
the funding is there and the volunteers are there

00:23:09.339 --> 00:23:13.740
and it's all coming together. So congratulations

00:23:13.740 --> 00:23:17.660
once again. Thank you. Thank you so much. We're

00:23:17.660 --> 00:23:20.720
going to come back. We're going to talk to Nathaniel

00:23:20.720 --> 00:23:23.740
some more. And we're going to give you a chance

00:23:23.740 --> 00:23:28.559
to ask your questions. So be sure to give us

00:23:28.559 --> 00:23:31.960
a call. That telephone number to call again is

00:23:31.960 --> 00:23:41.640
812 -638 -4261. It's 812 -NET -HAM -1. And we'll

00:23:41.640 --> 00:23:44.339
take your calls when we come back after this

00:23:44.339 --> 00:23:48.400
word. from Tower Electronics right here on HamTalk

00:23:48.400 --> 00:24:15.099
Live. I'm not so sure why I ever used any other

00:24:15.099 --> 00:24:19.259
PL259s. Mine are better. Besides, you deserve

00:24:19.259 --> 00:25:05.869
the best. You know I love you. If a man says

00:25:05.869 --> 00:25:08.130
something in the woods and there are no women

00:25:08.130 --> 00:25:10.980
there, is he still wrong? You're listening to

00:25:10.980 --> 00:25:39.869
HamTalk Live with Neil Rapp. Thanks as always

00:25:39.869 --> 00:25:43.430
to Tower Electronics for bringing HamTalk live

00:25:43.430 --> 00:25:48.529
your way each and every week. Their HamFest schedule

00:25:48.529 --> 00:25:52.349
this weekend, it's actually tomorrow and Saturday

00:25:52.349 --> 00:25:57.269
in Belton, Texas. And then Chickasaw, Alabama,

00:25:57.710 --> 00:26:02.049
October 12th. And October 19th, Greenville, Tennessee.

00:26:02.650 --> 00:26:06.309
But you can visit them anytime, anywhere at PL

00:26:06.309 --> 00:26:11.589
-259 .com. At HamTalk Live, you can visit us

00:26:11.589 --> 00:26:15.190
anytime, anywhere at HamTalkLive .com or live

00:26:15.190 --> 00:26:18.869
every Thursday night at 9 p .m. at HamTalkLive

00:26:18.869 --> 00:26:22.130
.com. And be sure to check us out on Facebook,

00:26:22.289 --> 00:26:25.230
Twitter, and Instagram. And it's time now for

00:26:25.230 --> 00:26:29.549
your calls. So if you have a question for Nathaniel,

00:26:29.609 --> 00:26:36.269
please give us a call at 812 -638 -4261. It's

00:26:36.269 --> 00:26:42.049
812 -NET -HAM -1. Or you can tweet us. It's at

00:26:42.049 --> 00:26:45.450
HamTalk Live. And if you're listening to us on

00:26:45.450 --> 00:26:50.329
WTWW or on the podcast version, we're not here.

00:26:50.490 --> 00:26:54.670
It's Thursday night, so we're not here. Sorry

00:26:54.670 --> 00:26:57.589
that we won't be able to take your questions

00:26:57.589 --> 00:27:02.250
live on the show, but we can always fit those

00:27:02.250 --> 00:27:06.930
questions in offline here as well. So we're going

00:27:06.930 --> 00:27:09.549
to talk a little bit about the next big project,

00:27:09.910 --> 00:27:16.059
but first let me run over here to Twitter. Brett

00:27:16.059 --> 00:27:20.099
caught my my near mistake and and he knows that

00:27:20.099 --> 00:27:23.859
I've caught on to this That at the beginning

00:27:23.859 --> 00:27:28.160
I almost said a hundred wires and a watt instead

00:27:28.160 --> 00:27:31.440
of a hundred watts and a wire so Brett caught

00:27:31.440 --> 00:27:36.599
that so I know somebody's listening so Very good

00:27:36.599 --> 00:27:39.279
eight one two six three eight four two six one

00:27:39.279 --> 00:27:43.450
is the number so let's talk a little bit about

00:27:43.450 --> 00:27:47.029
some future plans and and i guess first would

00:27:47.029 --> 00:27:50.009
be this hamsai conference that you've got coming

00:27:50.009 --> 00:27:54.069
up and and amazingly it's at the university of

00:27:54.069 --> 00:27:58.349
scranton that's right we're planning the 2020

00:27:58.349 --> 00:28:01.650
hamsai workshop at the university of scranton

00:28:01.650 --> 00:28:04.869
and the plan is to have it march 20th and march

00:28:04.869 --> 00:28:09.269
21st and this is an opportunity to come uh meet

00:28:09.269 --> 00:28:13.720
fellow ham radio science enthusiasts and professional

00:28:13.720 --> 00:28:16.519
academic researchers. And we all come together

00:28:16.519 --> 00:28:20.180
and we present the research that we've been doing

00:28:20.180 --> 00:28:23.279
and talk about how we can further both science

00:28:23.279 --> 00:28:27.160
and amateur radio together. And it's a really,

00:28:27.160 --> 00:28:31.079
really great couple days. So we've run the workshop

00:28:31.079 --> 00:28:33.859
twice so far. We had it once at NJIT. That was

00:28:33.859 --> 00:28:36.559
the first year. And then last year Case Western

00:28:36.559 --> 00:28:38.359
Reserve hosted it. And so this year it will be

00:28:38.359 --> 00:28:41.980
at the University of Scranton. All right, and

00:28:41.980 --> 00:28:44.279
that's you know, anybody can go to that right?

00:28:44.720 --> 00:28:47.279
That's right. Yes, anyone can go. So we're still

00:28:47.279 --> 00:28:50.619
working on getting the details Set up that will

00:28:50.619 --> 00:28:54.420
be posted on Ham side at work probably in about

00:28:54.420 --> 00:28:57.140
a month or so So we still have to get some of

00:28:57.140 --> 00:29:02.000
the final details but typically it costs about

00:29:02.000 --> 00:29:04.599
a hundred seventy five dollars or so and that

00:29:04.599 --> 00:29:09.039
includes all of the food, so that's We still

00:29:09.039 --> 00:29:11.500
have to confirm all those details for this year,

00:29:11.539 --> 00:29:13.339
but that's how we've been able to run it in the

00:29:13.339 --> 00:29:18.339
past. And last year we had some very good speakers.

00:29:18.579 --> 00:29:23.299
We had Ward Silver, N0AX is the keynote speaker.

00:29:24.140 --> 00:29:28.839
And for the two invited tutorials, we had Carl

00:29:28.839 --> 00:29:33.440
Letzelswab, K9LA, who's a well -known propagation

00:29:33.440 --> 00:29:41.079
columnist. Dr. Larissa Gondrenko from the MIT

00:29:41.079 --> 00:29:47.160
Haystack Observatory Well some great People there

00:29:47.160 --> 00:29:51.039
and some great topics so if you get a chance

00:29:51.039 --> 00:29:54.380
head on over to the University of Scranton in

00:29:54.380 --> 00:29:58.980
March and and check out the third Hamseye workshop

00:29:58.980 --> 00:30:02.240
Well, what else have you got coming up here?

00:30:02.359 --> 00:30:06.880
Are you coming up with some more of these? Great

00:30:06.880 --> 00:30:10.819
ideas for studies? Oh, well, let me tell you.

00:30:11.759 --> 00:30:14.599
I mean, just working on the personal space weather

00:30:14.599 --> 00:30:20.160
station right now is taking that is a very multifaceted

00:30:20.160 --> 00:30:23.900
project in and of itself. So we have people working

00:30:23.900 --> 00:30:27.619
on the Tangerine SDR. That's going to be the

00:30:27.619 --> 00:30:30.160
higher end version of the personal space weather

00:30:30.160 --> 00:30:32.680
station. We're going to have a lower cost version.

00:30:32.720 --> 00:30:34.740
So there's design that needs to go into that.

00:30:34.880 --> 00:30:39.640
We're going to have part of the device use ground

00:30:39.640 --> 00:30:41.660
magnetometers, so there's science that needs

00:30:41.660 --> 00:30:45.380
to go into that. So just this one project is

00:30:45.380 --> 00:30:48.740
really quite diverse. And even the festival of

00:30:48.740 --> 00:30:51.319
frequencies that we're having right now, those

00:30:51.319 --> 00:30:55.220
observations are going to help give us ideas

00:30:55.220 --> 00:31:01.940
and data starting point for the designs for this

00:31:01.940 --> 00:31:05.660
personal space weather station as well. So that

00:31:05.660 --> 00:31:08.359
is part of it. But some other things, I guess

00:31:08.359 --> 00:31:10.720
some other things I have personally going on

00:31:10.720 --> 00:31:15.500
with the hamsi type activities is I'm working

00:31:15.500 --> 00:31:19.819
on a paper that looks at large -scale traveling

00:31:19.819 --> 00:31:22.019
ionospheric disturbances that you can see in

00:31:22.019 --> 00:31:26.819
both reverse speaking network and a whisper network

00:31:26.819 --> 00:31:29.799
data. and i'm planning on presenting that at

00:31:29.799 --> 00:31:32.519
the american geophysical union meeting this coming

00:31:32.519 --> 00:31:35.519
december so i'll be there and a few other hamside

00:31:35.519 --> 00:31:41.119
people be there as well and um... and i'm also

00:31:41.119 --> 00:31:43.220
planning on going to the american meteorological

00:31:43.220 --> 00:31:46.779
society meeting in january so there's there's

00:31:46.779 --> 00:31:51.259
quite a bit of activity going on eight one two

00:31:51.259 --> 00:31:53.720
six three eight four two six one is the phone

00:31:53.720 --> 00:31:57.119
number if you have a question for Dr. Nathaniel

00:31:57.119 --> 00:32:03.779
Frisell, W -2 -N -A -F about HamSci and the WWV

00:32:03.779 --> 00:32:10.380
Anniversary Festival of Frequency Measurement.

00:32:10.839 --> 00:32:17.299
So, and if you're listening to this... WWV, all

00:32:17.299 --> 00:32:22.140
the time, all the time. And you measured... the

00:32:22.140 --> 00:32:26.259
Doppler shift. Make sure you send in your data

00:32:26.259 --> 00:32:30.599
and get it collected. Well, let's see. We do

00:32:30.599 --> 00:32:37.220
have a question here coming in from Brett, wy7bg.

00:32:37.640 --> 00:32:41.200
What will the ionospheric researchers be doing

00:32:41.200 --> 00:32:47.440
during the upcoming eclipse? Well, they are going

00:32:47.440 --> 00:32:51.480
to be trying to repeat some of the same sorts

00:32:51.480 --> 00:32:54.339
of experiments that happened in the last eclipse,

00:32:54.400 --> 00:32:56.160
and you might say, well, why would you do that?

00:32:56.920 --> 00:33:02.160
Well, the path of the upcoming eclipse is rather

00:33:02.160 --> 00:33:04.960
different from the path of the previous eclipse.

00:33:05.759 --> 00:33:08.079
The 2024 eclipse is going to be much more of

00:33:08.079 --> 00:33:12.539
a north -south direction, whereas the 2017 eclipse

00:33:12.539 --> 00:33:16.319
was from west to east, and so there's actually,

00:33:16.420 --> 00:33:20.349
because of Because the ionosphere is structured

00:33:20.349 --> 00:33:25.730
based on the Earth's magnetic field, you can

00:33:25.730 --> 00:33:28.710
expect to see some different behavior between

00:33:28.710 --> 00:33:31.289
those two situations. So they'll be investigating

00:33:31.289 --> 00:33:35.990
some science questions related to that, I'm sure.

00:33:37.349 --> 00:33:43.509
And if I don't move, the center of that viewing

00:33:43.509 --> 00:33:48.019
area is like three miles from my backyard. Wow,

00:33:48.019 --> 00:33:51.220
are you lucky so yeah the last time we were like,

00:33:51.480 --> 00:33:53.680
oh, we're in the wrong place And then it's like

00:33:53.680 --> 00:33:56.859
well wait wait next time is better. So just have

00:33:56.859 --> 00:33:59.480
to wait around long enough, right? Yeah. Yeah.

00:33:59.619 --> 00:34:01.640
No, I don't know if I can wait around long enough,

00:34:01.640 --> 00:34:07.140
but Maybe we'll come back and visit but Maybe

00:34:07.140 --> 00:34:10.159
we can rent out the backyard as an observatory

00:34:10.159 --> 00:34:13.519
or something. I don't know But yeah, there should

00:34:13.519 --> 00:34:16.780
be some good things and of course, you know But

00:34:16.780 --> 00:34:19.699
repeating this is always kind of necessary to

00:34:19.699 --> 00:34:22.300
make sure that, you know, there's not something

00:34:22.300 --> 00:34:25.960
wrong with the data. That's right. And, you know,

00:34:26.239 --> 00:34:28.860
we're looking to confirm things, you know, like

00:34:28.860 --> 00:34:32.239
waves that are generated by eclipses, waves in

00:34:32.239 --> 00:34:41.940
the ionosphere. with altitude, those are some

00:34:41.940 --> 00:34:45.159
of the things people will be looking at. There

00:34:45.159 --> 00:34:47.920
are people who look at VLF propagation and how

00:34:47.920 --> 00:34:52.619
that changes due to an eclipse. So there's a

00:34:52.619 --> 00:34:54.800
lot of different ways to look at the eclipse.

00:34:56.840 --> 00:34:59.980
Well, that's coming up, so we'll have to hang

00:34:59.980 --> 00:35:04.380
on for that one a little while longer, but the

00:35:04.380 --> 00:35:08.179
preparation begins now, so that's good. It does.

00:35:08.679 --> 00:35:13.280
812 -638 -4261. Let's give one last call here

00:35:13.280 --> 00:35:18.260
for some questions for Dr. Nathaniel Frisell,

00:35:18.400 --> 00:35:22.739
W2NAF from HamSci. What else is HamSci up to

00:35:22.739 --> 00:35:29.239
besides the WWV thing and the upcoming conference?

00:35:31.900 --> 00:35:34.619
So besides that and the personal space weather

00:35:34.619 --> 00:35:41.300
station, Well, we're always looking for people

00:35:41.300 --> 00:35:45.500
who are doing science sorts of activities with

00:35:45.500 --> 00:35:47.800
ham radio. We're looking for them to contribute

00:35:47.800 --> 00:35:51.960
There's a lot of interest in the NVIS type propagation

00:35:51.960 --> 00:35:57.420
near vertical incidence skywave And this is of

00:35:57.420 --> 00:36:02.579
particular interest to people who are doing public

00:36:02.579 --> 00:36:06.440
service emergency communications and defense

00:36:06.440 --> 00:36:10.360
applications because it allows you to set up

00:36:10.360 --> 00:36:15.719
regional communications with modest antennas.

00:36:15.980 --> 00:36:20.760
And so that's a very hot topic of research. Some

00:36:20.760 --> 00:36:23.079
of the people at, some of the researchers at

00:36:23.079 --> 00:36:25.559
West Point are actually very interested in this,

00:36:25.639 --> 00:36:28.659
and they were able to come to both the HamSci

00:36:28.659 --> 00:36:32.440
workshop and the Tapper DCC and present on that

00:36:32.440 --> 00:36:34.619
sort of work. So I know that's going to be a

00:36:34.619 --> 00:36:37.699
continuing topic near Vertical Instance SkyWave

00:36:37.699 --> 00:36:43.320
and VIS. Very good. Well, all kinds of cool stuff

00:36:43.320 --> 00:36:47.960
going on, and it's HamSci .org, H -A -M -S -C

00:36:47.960 --> 00:36:53.039
-I .org. Be sure to check that out. watch what's

00:36:53.039 --> 00:36:58.099
happening because Nathaniel and his cohorts are

00:36:58.099 --> 00:37:01.719
putting together some marvelous science tied

00:37:01.719 --> 00:37:06.760
in with ham radio. So Nathaniel, again, congratulations

00:37:06.760 --> 00:37:12.940
on the new job, on the big award and another

00:37:15.550 --> 00:37:19.510
interesting measurement of the ionosphere and

00:37:19.510 --> 00:37:23.289
we look forward to hearing more as you have a

00:37:23.289 --> 00:37:27.130
chance to dig into the data and find a few more

00:37:27.130 --> 00:37:30.449
things I suspect. Yes thank you so much Neil.

00:37:32.349 --> 00:37:34.929
All right well anything else we need to we need

00:37:34.929 --> 00:37:38.650
to tell the listeners before we go here? I think

00:37:38.650 --> 00:37:43.539
that's it just keep operating and You know, be

00:37:43.539 --> 00:37:48.320
curious. I hope to see some of you come to the

00:37:48.320 --> 00:37:52.219
Hampstead workshop in 2020 at the University

00:37:52.219 --> 00:37:55.280
of Scranton. I will very much enjoy meeting you.

00:37:56.079 --> 00:38:00.079
And the more you operate, the more research you

00:38:00.079 --> 00:38:03.739
can do. That's right. If the signals aren't there,

00:38:04.280 --> 00:38:06.780
you can't measure them. So that's right. You

00:38:06.780 --> 00:38:09.199
got to have them out there. So get on the air

00:38:09.199 --> 00:38:14.639
and next weekend, Get outside if you can and

00:38:14.639 --> 00:38:17.500
participate in the Fallout activity. There's

00:38:17.500 --> 00:38:20.320
another activity for you to get on the air with,

00:38:21.039 --> 00:38:24.820
so don't forget about that. Well, that is a wrap

00:38:24.820 --> 00:38:29.320
for this week's edition of HamTalk Live. Thanks

00:38:29.320 --> 00:38:33.139
again to my guest, Dr. Nathaniel Forssell, W2NAF,

00:38:33.599 --> 00:38:37.059
and everybody in cyberspace for listening and

00:38:37.059 --> 00:38:40.969
typing in tonight. Come back next Thursday night

00:38:40.969 --> 00:38:44.869
at 9 p .m. Eastern Time and we'll have another

00:38:44.869 --> 00:38:49.010
guest. We're working on a kind of big one. So

00:38:49.010 --> 00:38:51.449
we'll see if it's next week or the week after.

00:38:51.670 --> 00:38:55.949
But we've got a big one coming on here pretty

00:38:55.949 --> 00:38:59.829
soon. So check out HamTalkLive .com for a list

00:38:59.829 --> 00:39:03.969
of all of our upcoming guests. And if you like

00:39:03.969 --> 00:39:06.610
HamTalk Live, please consider leaving us a review

00:39:06.610 --> 00:39:09.570
on iTunes or wherever you live. listen, it helps

00:39:09.570 --> 00:39:13.949
others find us faster. So for now, this is Neil

00:39:13.949 --> 00:39:18.650
Rapp, WB9VPG, saying seven three, seven five,

00:39:19.070 --> 00:39:21.969
and may the good DX be yours.
