Category Archives: Space Weather

Did the Miyako earthquake affect Medium Wave reception at a Japanese DXpedition?

by Satoshi Miyauchi, JP1SCQ, with Nick Hall-Patch, VE7DXR

Introduction

In early November 2025, several members of our Totsuka DXers Circle in Japan (TDXC  https://www.tdxc.net/abouttdxc/ ) traveled from the Tokyo area to Tanohata village in Iwate prefecture on northern Honshu island in order to take part in a medium wave (MW) DXpedition that took place on the 8th and 9th of the month.  The site was about 500m (1/3 mile) from the Pacific Ocean, overlooking Kitayamazaki cliffs, a very scenic area (Figure 1), but also one from which a great deal of long-haul DX had been heard in the past, including trans-polar WBZ-1030kHz, as well as the farthest possible Antipodes DX such as R. Nacional in Argentina on 870kHz and Radio Monte Carlo in Uruguay on 930kHz.

Figure 1

Our listening post was a meeting room in the Tanohata Nature Training Center, where we set up our receivers, such as Perseus and Airspy HF+discovery, plus our recording gear and accessories (Figure 2).

Figure 2

My recording software was SDR Console, but playback and analysis also used WavViewDX.  We set up a TDDF (Twisted Double Delta Flag) antenna with a northeast directional pattern in order to receive medium-wave broadcasts from North America. (Figure 3)

Figure 3 – TDDF antenna; note that low-noise pre-amplifier with bias-T is a must.

Directional patterns from Kazu GOSUI

On the second evening, November 9th, while enjoying the reception, an emergency earthquake alert was issued, and shaking struck. Inside our building, nearly 200 meters above sea level on the solid bedrock of Kitayamazaki, the shaking felt less intense than the reported magnitude of 6.9, even with an epicenter only 140km away. (Figure 4)

Figure 4

However, since earthquakes had been occurring even before that day and numerous aftershocks were felt afterward, it left us with a vague sense of unease. Later, a tsunami advisory was announced on the radio, plus the Tohoku Shinkansen train back to Tokyo had also stopped, and I myself couldn’t help worrying about whether it might affect my return home the following day. At that moment, I had a conversation with the members there, thinking, “If there’s something related to the earthquake recorded, that would be amazing.” However, during the real-time reception, we were targeting signals from North America in 10kHz steps, and there was no effect noticed upon those receptions.

Unusual Signal Dropouts Observed

I played back the SDR files using WavViewDX (https://rweiss.de/dxer/tools.html), a software with many capabilities, including a choice of displaying all signals across the MW band at 9 or 10kHz channel spacing, but, because I was looking for North American DX, I only realized a week after returning home that the reception conditions for the 9kHz spaced domestic Japanese stations had significantly changed around 0715 to 0745UT (16:15 to 16:45 Japan time) on 9 November, based on our recordings. The dropouts on various channels over 0715 to 0745UT are quite obvious in Figure 5; I had never seen such sudden attenuation before.  For those not familiar with WavViewDX, the green vertical lines on the display represent stronger signals being received on broadcast channels, while gray or black areas represent weak or no signal. (For a more detailed description of WavViewDX and its capabilities, see https://swling.com/blog/2025/10/an-introduction-to-wavviewdx-sdr-playback-software-a-totsuka-dxers-circle-article-by-kazu-gosui

Figure 5 – WavViewDX display of signal dropouts. X-axis is frequency of received signal, Y-axis is time UTC

A first look at the data led to a couple of other observations:

  1. Signals originating north of the receiving site, primarily from the island of Hokkaido, were largely unaffected by the attenuation. (It is true that our antenna’s directionality was northeast, but it also received the stronger domestic stations from southwest of the antenna.)
  2. Regarding signals from North America, even during the same time period, the intense attenuation observed in domestic stations was generally not seen. It is unclear, however, whether some dips in North American signals around that time were due to normal fading or to the same cause that brought about the attenuation in domestic stations.

What Could Have Caused These Dropouts?

Local sunset?

These sudden drops in signal strength corresponded quite closely with local sunset at 0722UT, normally a time of disturbed propagation (see Figure 6), so the most straightforward possibility is simply the well-known change in ionospheric propagation conditions that occurs at sunset.   Was that all that there was to it?  However, we had been listening and recording the previous day as well, and analyzing those recordings with WavViewDX yielded no sign of dropouts in domestic signal strength at sunset on that day.   Examining recordings that had been made at the same site, using similar equipment, on 24 October 2024, also showed no dropouts taking place at local sunset.

Figure 6

In fact, over many years in Japan, not only at this location but across various areas, records have been accumulated during the same time window, because good trans-Pacific DX occurs around local sunset.  Nowhere in these records has a situation such as observed this time—a significant attenuation of domestic stations at local sunset—been found. Therefore, it seemed unlikely that sunset was the cause of the dropouts, but what else could it have been? Continue reading

Auroras, HF Predictions, and More: A Look at Australia’s Space Weather Site

Many thanks to SWLing Post contributor Jerome van der Linden, who writes:

For some time, I have subscribed to a service that alerts me via email when our weather bureau wants to inform people about the likelihood of aurora activity that might lead to the ability to observe the southern hemisphere auroras, such this example:

SUBJ: ASWFC AURORA OUTLOOK

ISSUED AT 0627 UT ON 31 May 2025

FROM THE AUSTRALIAN SPACE WEATHER FORECASTING CENTRE

A halo CME is expected to impact Earth on 01-Jun at 2100UT +/- 8 hours. This impact is expected to produce auroral activity on 01-02 Jun, with a chance of continued activity on 03-Jun. Warnings and/or alerts will follow if significant geomagnetic activity occurs.

Quite recently, I discovered that the Bureau of Meteorology (“the BOM”) in Australia has, as part of its www.bom.gov.au website, an Australian Space Weather Forecasting Centre: https://www.sws.bom.gov.au/. It has a number of interesting headings (with links) that may be of interest to others in the SW hobby, such as “Solar”;”HF Systems”, and “Products and Services”. With the respect to the last, it would appear that a number of organisations subscribe to services provided by the BOM, including Australian airlines. In addition it seems even Stockholm Radio subscribes to some of the services, and an example of hour by hour HF frequency area prediction is shown in these graphs:

There’s far too much for me to review on this website, so I suggest interested SWLers may care to have a look for themselves, as there’s a lot of information there, which is updated regularly.

A New Eye on the Sun: CCOR-1 and the Future of Solar Weather Monitoring

Many thanks to SWLing Post contributor, Jake Brodsky (AB3A), who writes:

One of the key instruments for predicting when solar weather events will
arrive here at Earth is the Chronograph. And one of the most widely used
Coronagraphs is the LASCO instrument onboard the SOHO spacecraft at
Lagrange Point 1 (L1). This is a place where the spacecraft orbits L1 in
a halo fashion, just like the James Webb Space Telescope at L2. The
advantage of L1 is that it gets a mostly uninterrupted view of the sun.

SOHO was designed for a two year mission. And here we are nearly 30
years later and the spacecraft is still working. However, the solar
panels have degraded over that time, the gyros are no longer working,
and though the spacecraft has lots of fuel, it is running on borrowed time.

The older LASCO C2 and C3 coronagraph images are amazing, considering
that they’re 30 year old technology. Still, after 30 years we can do
better.

Enter CCOR, or the Compact Coronagraph. The scientists at Naval Research
Lab decided to see what they could do to improve on LASCO. The result
was CCOR-1. CCOR-1 was launched on GOES-U which, upon arriving on
station in Geostationary Orbit, became GOES 19.

Since it arrived on station last July, I’ve been waiting patiently for
the images from the new coronagraph to become available. It’s taken some
time and it won’t be officially available until April. However, you can
see what it looks like under the “experimental” instruments on NOAA’s
web page.

See https://www.swpc.noaa.gov/products/ccor-1-coronagraph-experimental

Unlike the LASCO instrument onboard SOHO at L1, Geostationary orbit
doesn’t offer an uninterrupted view of the sun. Often you’ll see the
moon photobombing its way through the image. And there are times when
the Earth may block the view of the sun. However, CCOR-1 reports
reliably every 15 minutes, whereas LASCO images can be delayed for many
hours until the SOHO spacecraft antenna points back at Earth.

When the CCOR-1 data is ready for scientific use, it will become an
important backup for the aging SOHO spacecraft. Also note that NOAA is
planning to launch a new replacement for SOHO at L1 called the Space
Weather Follow On to L1 or SWFO.

Solar weather is critical for many uses, besides just shortwave radio.
These include predicting degraded GPS accuracy, Satellite Operations,
Power Grid Operations, and in extreme cases, even alerting pilots of
excessive radiation risks when flying in the vicinity of the North and
South poles.

Have a look at the CCOR-1 images. It is much better at illuminating the
corona of the Sun, though it does have limitations based upon where it
is located.

73,

Jake Brodsky,
Amateur Radio Station AB3A

The Sun is Flaring (X and M Class )

Many thanks to SWLing Post contributor Troy Riedel, who shares the following news courtesy of the excellent SpaceWeather.com site:

THE SUN IS FLARING AGAIN: Sunspot AR3947 is sizzling with activity. Since yesterday it has produced three X-class solar flares and multiple strong M-flares. NOAA’s GOES-16 satellite recorded the extreme ultraviolet and X-ray flashes:

Each flare has produced a shortwave radio blackout on Earth. Almost all longitudes of our planet have experienced intermittent loss of signal below 20 MHz during local daylight hours. Long-distance propagation has been very unreliable.

Remarkably, no significant CMEs have emerged. For some reason, these explosions have not lifted much material out of the sun’s atmosphere. Future blasts may behave differently, however, and the activity shows no sign of abating as the sunspot turns toward Earth.

Parker Solar Spacecraft

Flying Into the Sun

On Christmas Eve the Parker Solar Probe is going to enter the Sun’s atmosphere for the first time to study Solar Wind. For radio hobbists of all ilks, this will hopefully help us understand more about the origins of Solar Wind, and thereby help us understand more fully the effects this has on radio signals (and other space weather issues).

The following is an exerpt from an article on ARS Technica by Eric Berger

Almost no one ever writes about the Parker Solar Probe anymore.

Sure, the spacecraft got some attention when it launched.  It is, after all, the fastest moving object that humans have ever built. At its maximum speed, goosed by the gravitational pull of the Sun, the probe reaches a velocity of 430,000 miles per hour, or more than one-sixth of 1 percent the speed of light. That kind of speed would get you from New York City to Tokyo in less than a minute.

And the Parker Solar Probe also has the distinction of being the first NASA spacecraft named after a living person. At the time of its launch, in August 2018, physicist Eugene Parker was 91 years old.

But in the six years since the probe has been zipping through outer space and flying by the Sun? Not so much. Let’s face it, the astrophysical properties of the Sun and its complicated structure are not something that most people think about on a daily basis.

However, the smallish probe—it masses less than a metric ton, and its scientific payload is only about 110 pounds (50 kg)—is about to make its star turn. Quite literally. On Christmas Eve, the Parker Solar Probe will make its closest approach yet to the Sun. It will come within just 3.8 million miles (6.1 million km) of the solar surface, flying into the solar atmosphere for the first time.

Read the whole article here

Posted by Robert Gulley K4PKM

Spaceweather.com: Sunspot “visually rivals Carrington’s famous sunspot”

Many thanks to SWLing Post contributor, Troy Riedel, who shares the following news via Spaceweather.com:

Above: Carrington’s sunspot (to scale) compared to today’s giant sunspot AR3664.

HUGE SUNSPOT HURLS CME TOWARD EARTH: A sunspot so large it visually rivals Carrington’s famous sunspot of 1859 hurled a CME toward Earth today. Don’t worry! A new Carrington Event is not in the offing. The incoming CME isn’t potent enough. However, this huge sunspot merits watching while Earth is in its strike zone. Full story @ Spaceweather.com.

CME impact alerts: Sign up for Space Weather Alerts to receive an instant text message when the CME arrives.

Rich’s propagation observations during the total solar eclipse

Many thanks to SWLing Post contributor, Rich Stahl, who writes:

In Ocean View NJ, our eclipse started at 2:08, 3:23 totality, and ended 4:35. We have a daytimer here on 1020, WWAC, at 1900 watts, and I was curious if KDKA, at 50kw, also on 1020, would have any presence during the event. I used my Tecsun PL330, on the internal ferrite antenna, and did a band scan 530-1710 every fifteen minutes to see what it would capture. From 2:15 up to the 3:45 scan, the radio captured between eight and ten signals per scan. Up to this point, the sun still had the D layer fully ionized. But after the mid point, the 4:00 scan had 19 captures, the 4:15 scan had 38, and the 4:30 scan had 36. The D layer had obviously de-ionized considerably. The very next scan, at 4:45, captures back down to 9. The sun was back in business. And never did I hear a peep out of KDKA.

Rich Stahl
WR3V
Ocean View, NJ

Thank you for sharing your findings, Rich! Perhaps others can comment with their observations as well.