Skip to main content

Our Friend the Sun

I had the opportunity to listen to a leading Space Weather Expert the other day, a chat with Professor Gordon P Turnbull. While the questions he was asked may seem a little basic I thought it worth reprinting the transcript here:

Can you explain sunspots?

Sunspots are dark spots on the surface of the sun that are cooler and less active than the surrounding areas. They are caused by intense magnetic activity and are associated with solar flares and coronal mass ejections. Sunspots can last for a few days to a few months and their number and size varies over time in a pattern known as the sunspot cycle. The sunspot cycle is roughly 11 years long and during the maximum phase of the cycle, there are more sunspots and more solar activity. Sunspots have been observed and studied for centuries and have been found to have a significant impact on Earth's climate and weather.

What effect do sunspots have on the earth’s ionosphere?

Sunspots can have a significant impact on the Earth's ionosphere, which is the layer of the Earth's atmosphere that is ionized by solar radiation. The ionosphere plays an important role in long-distance radio communication and navigation.

During times of high solar activity, such as during the maximum phase of the sunspot cycle, the ionosphere can become more active and dynamic. This can result in increased ionization and a thicker ionosphere, which can lead to improved radio propagation and increased absorption of radio waves. This can cause changes in the frequency of the radio waves, which can cause distortion and fading of long-distance radio signals. This can be particularly problematic for high-frequency (HF) radio communications.

On the other hand, during times of low solar activity, such as during the minimum phase of the sunspot cycle, the ionosphere can become less active and stable. This can result in decreased ionization and a thinner ionosphere, which can lead to poor radio propagation and increased scattering of radio waves. This can cause increased noise and fading of long-distance radio signals. This can also be particularly problematic for high-frequency (HF) radio communications.

Overall, sunspots can have a significant impact on the Earth's ionosphere and can affect long-distance radio communication and navigation.

Thanks. Can you explain the K and A indexes?

The K and A indices are measures of geomagnetic activity. They are used to quantify the level of disturbance in the Earth's magnetic field caused by solar activity.

The K index is a measure of the short-term variation in the Earth's magnetic field and is based on data from a single magnetic observatory. It is a 3-hourly measurement and ranges from 0 to 9, with higher values indicating greater geomagnetic activity. The K index is based on the deviation

of the Earth's magnetic field from a quiet-day curve and is calculated using the largest deviation in each of the three magnetic field components (H, D and Z) over a 3-hour period.

The A index is a measure of the longer-term variation in the Earth's magnetic field and is based on data from multiple magnetic observatories. It is a daily measurement and ranges from 0 to 400, with higher values indicating greater geomagnetic activity. The A index is based on the average of the K index values over a 3-hour period and is calculated for each of the magnetic field components (H, D and Z) and then combined to give a single value.

Both the K and A indices are used to indicate the level of geomagnetic activity and are used in forecasting and in the study of space weather. They are also used to help operators of power systems, pipelines, and communication systems to protect their equipment and networks from the effects of space weather.

K and A indices are both published by various space weather agencies and can be accessed online, including the National Oceanic and Atmospheric Administration (NOAA) in the United States and the European Space Weather Portal (ESWP) in Europe.

Brilliant. What are solar storms then?

Solar storms, also known as space weather events, are disturbances in the solar wind that can affect the Earth's magnetic field, atmosphere, and climate. They are caused by the sun's activity, such as solar flares and coronal mass ejections (CMEs), which send large amounts of charged particles and electromagnetic radiation towards the Earth.

Solar flares are sudden, intense bursts of electromagnetic radiation that are emitted from the sun's surface. They are caused by the sudden release of magnetic energy stored in the sun's atmosphere.

Coronal mass ejections (CMEs) are large eruptions of plasma and magnetic field from the sun's corona, which is the outermost layer of the sun's atmosphere. They are caused by the sudden and explosive release of magnetic energy stored in the sun's corona.

Both solar flares and CMEs can cause disturbances in the solar wind, which is a stream of charged particles that flow out from the sun in all directions. When these disturbances reach the Earth, they can cause geomagnetic storms, which are disturbances in the Earth's magnetic field.

These solar storms can have a range of effects on the Earth, including:

• Interference with satellite and communication systems

• Power grid disruptions

• auroras (northern and southern lights)

• Increased radiation levels for astronauts and high-altitude aircraft

• Disruption of GPS signals

• Damage to orbiting satellites

Overall, solar storms are disturbances in the solar wind caused by the sun's activity and can have a range of effects on the Earth's magnetic field, atmosphere, and climate.

Quite enlightening I’m sure you’ll agree. If you’ve stuck with reading this article to the end you might be wondering if Professor Turnbull really speaks like that? Well, he doesn’t. In fact, he doesn’t exist at all. The questions are my own and the answers are produced by ChatGPT, Gordon P Turnbull, get it? CHatGPT is an AI chatbot that uses an internet-scraped dataset to answer real-world questions conversationally. There has been no editing of the answers at all.

The data is a couple of years old so don’t ask about the war in Ukraine for example as it will probably describe the siege of Sevastopol in 1855, which we won.

ChatGPT is free to try with a trial account here https://chat.openai.com/

Microsoft is investing heavily in the firm behind this tech and there is a more capable and modern version in development now.

Unsurprisingly, many firms including HMG have banned the use of ChatGPT. It is after all that chatty equivalent of Wikipedia on steroids and everything on the internet is true, isn’t it?

73 Mike, G0KAD (or is it???)

Comments

g3ysx said…
If you have access to it, it is worth reading
https://www.economist.com/business/2023/01/30/the-race-of-the-ai-labs-heats-up

This is clearly going to be a major technology.

Independent of Mike’s work I tried some other amateur radio questions which I will post.

My impression is that this is curate’s egg in terms of the quality of the output. However, I can see a major utility. I personally always find it very hard to write a first draft of anything, but I can see that as a tool to start a paper which would then be subject to rigorous expert redrafting it has potential.

Distressingly I see a similarity between the output of unedited ChatGTP and the statements made by certain major public figures often on the news.

Popular posts from this blog

CARC WSPR Challenge Detailed Results for March 2023

There is a lot of detail in the following, but I provide it so entrants can see who worked whom, and of course so anyone with the time can see if I have have made any errors in the software. There are three categories: Tx, Rx and QSO where QSO is a bidirectional exchange of WSPR information between a pair of stations at some time in the month. Comments are welcome Stewart/G3YSX Tx Category Posn Call Stns SQ Score 1 2E0XDZ 790 368 290720 2 G4PEO 665 331 220115 3 M0WID 518 271 140378 4 M0HQM 414 237 98118 5 G3YSX 342 212 72504 6 M6DPW 215 140 30100 7 M0IJP 24 21 504 8 G0UPL 1 1 1 Detailed report  M0WID heard by the following  518  stations: ['2E0BWX', '2E0FWE', '2E0HQR', '2E0ILY/KIWI', '2E0PYB', '2E0XDZ', '2M0JAT', '4X6FB', '56IGJF', '5B4CY', '7L4IOU', '9H1US', '9K2RA', 'AA0ZT', 'AA1A...

CARC WSPR Report 23 April 2024

Processing time: real 17m20.081s user 15m14.753s File size 11.4GB Spots file =  wsprspots-2024-04.csv Tx Catagory Spots file =  scrubbed-spots.csv Posn Call Stns SQ Score 1 M0WID 1110 448 497280 2 M0LMG 1091 450 490950 3 G3YSX 976 439 428464 4 G4PEO 934 436 407224 5 M7GIM 845 415 350675 6 2E0XDZ 745 359 267455 7 G4ANN 592 305 180560 8 GX3WSC 597 293 174921 9 M0JGH 585 292 170820 10 M1YAP 506 287 145222 11 M0HQM 511 270 137970 12 M0EPX 255 165 42075 13 M6JGW 212 119 25228 14 M0IJP 152 85 12920 15 M5SB 142 80 11360 16 G0UPL 1 1 1  Total Callsigns worked = 1607  Rx Catagory Posn Call Stns SQ Score 1 M0WID 1307 900 1176300 2 G3YSX 1035 733 758655 3 M0LMG 773 532 411236 4 G4ANN 633 453 286749 5 M1YAP 447 314 140358 6 M7GIM 433 311 134663 ...

CARC WSPR Report 15 April 2024

  Tx  Category Posn Call Stns SQ Score 1 M0WID 985 419 412715 2 M0LMG 939 402 377478 3 G3YSX 770 350 269500 4 2E0XDZ 745 359 267455 5 G4PEO 546 297 162162 6 M7GIM 540 296 159840 7 GX3WSC 507 264 133848 8 M0JGH 505 264 133320 9 G4ANN 469 264 123816 10 M0HQM 429 245 105105 11 M1YAP 402 244 98088 12 M0EPX 204 135 27540 13 M6JGW 212 119 25228 14 M5SB 142 80 11360 15 M0IJP 122 71 8662 16 G0UPL 1 1 1 Total Callsigns worked = 1367  Rx Category Posn Call Stns SQ Score 1 M0WID 1124 732 822768 2 G3YSX 794 574 455756 3 M0LMG 662 453 299886 4 G4ANN 500 361 180500 5 M1YAP 377 260 98020 6 M7GIM 243 176 42768 7 G4PEO 230 162 37260 8 GX3WSC 208 144 29952 9 M0HQM 100 75 7500 10 M0EPX 95 75 7125 11 M5SB 96 73 7008 12 2E0XDZ ...