DDRC InkDarling Downs Radio Club Incorporated September 2018

The Official Journal of the Darling Downs Radio Club Incorporated

Office BearersPresident:David Erdmann VK4DAV

Vice-President:Klaus Merretz VK4HCC

Secretary:Sheryl Erdmann SWL

Treasurer:Kevin Crandell VK4VKX

Contact the clubAll contact should be made to the Secretary of the DDRCi via email:secretary@ddrci.org.auOr by phoning the Secretary on 07 46961045.

Next months meetings:

Held at Toowoomba City Library Meeting Rooms

Management Committee8th October, 2018

Technical/Social meeting22nd October, 2018:

NOTICES From the Editor’s Desk

Another month has passed and it appears that these months are moving very fast. So here I am once again bringing you another newsletter, I hope that you will enjoy it and I am keen for your comments. Another thing that I am thinking about is to have a column for letters to the editor, so if you have any issues for discussion or just point of view please send me some letters.Due to popular demand, I have started a new column for the foodies out there. So if you have any favourite recipes that you would like to share please forward them to the secretary and I will publish one recipe each month.This month we are preparing the JOTA event at Oakey and Bunya Park Toowoomba with the Scout/Guide Groups. As you already know, this is an annual event where the Scouts, and Guides can communicate with their counterparts all over the world. It is a fun week end for them and a good exercise for us amateur radio operators in setting up portable stations. This year we have made contact with an American group thanks to our newest member Warren (W4RRN) in Alabama, US, we will be working on echolink for these contacts, also contact has been arranged with the Bundaberg Scouts thanks to Klaus for organising this exercise. I wish to thank all that are participat-ing in making this event successful. I would like to thank Da-vid Cavanagh for his support in providing IRLP on the Bunya Mountains repeater for the week end. The node number for this repeater is 6401.Scouts and Guides will be participating in phonetic alphabet and Morse code decoding via games.

2 Metre NetEvery Sunday

80 Metre NetEvery Saturday

Scrub Turkey Net 2 metres

Thursdays

Remember to join us on Sunday mornings at 10 am for the Darling Downs Radio Club 2 metre net, Join our net control-ler Kevin VK4VKX for a chat and to have a good rag chew.

Or if you prefer HF, then join the conversation of 80 meters hosted by Theo VK4ESK, I am sure that you will be able to ask questions and get several responses by a group af very knowledgeable amateurs, after all, this is what amateur ra-dio is all about.

Another well attended net is on Thursday nights commenc-ing at 7:30 pm on the Mt Kynoch repeater 147.050 +ve offset and 91.5Hz tone, this is the Scrub Turkey Net hosted by Merv VK4EM, you might hear a lot talk regarding SSTV and satellite issues.

Happy Birthday to all those members that are celebrating another birthday this month of September. Hope you have a wonderful day in the company of your family and friends. If you have difficulty in blowing out the candles, please do not hesitate to call for assistance. All the best for the day and many wishes from all of us at the club.

To all those members that are not feeling very well, (Merv VK4EM hope that you are getting better from your ordeal, Craig VK4AC you will have to look after your ribs, Kevin VK4VKX I hope that you caught the spider that gave you that nasty sting, David VK4MU better to wear boots and keep away from those snakes) hope that you will overcome those ailments and that you recover quickly, we at the DDRCi wish all of you the best and a quick recovery. Look forward to seeing you at the meeting in the near future.

For the FoodiesApple Teacake in a Mug

This is fun and different to make! This recipe makes twolarge mug cakes.Ingredients:

• 6 tablespoons Self Raising Flour• 4 tablespoons brown sugar• 1 egg, lightly beaten• 1 apple, peeled, cored and grated• 2 tablespoons milk• 2 tablespoons canola oil• 1/2 teaspoon ground cinnamon

Oceania DX ContestThe OCDX contest is Oceania's only international style con-test where contacts with stations all over the globe are able to participate.

Oceania stations may contact any station for QSO points whilst non-Oceania stations are required to contact any sta-tion in Oceania for QSO points.

The contest runs over the first two full weekends in Octo-ber and has SSB, CW and SWL categories. Go to the contest web site for more information.

Aim Of The ContestOceania Stations

The aim of the contest is for stations within the Oceania Region is to contact as many other amateur radio stations as possible within the 24 hours of the contest on any of the 160M, 80M, 40M, 20M, 15M and 10M amateur bands. Each prefix worked on each band is counted as a multiplier.

DX Stations outside Oceania

Contests

Method

Distribute the dry ingredients evenly between two large mugs and stir well. In a jug, combine the egg, milk, oil and apple. Stir well and add half in each cup. Using a dessert spoon, mix the two mugs well making sure you get all the dry flour in the bottom. Cover the mug loosely with cling wrap and microwave on high for 2 minutes (based on an 800 watt oven). Allow to stand for a minute to cool slightly, then carefully run a knife around the inside to loosen. Tip the cake out onto a plate and serve with butter and a sprinkle of cinnamon and white sugar or nutmeg, or you can add custard, whipped cream or ice cream!Recipe Tips and hintsYou may need to adjust the cooking times depending on your microwave to avoid overcook-ing the cake. Try cooking for 1 minute, and if it needs longer, additional bursts of 15 sec-onds until it is cooked to your liking.

Ghost radio station http://www.bbc.com/future/story/20170801-the-ghostly-radio-station-that-no-one-claims-to-runOz licences under review!http://www.southgatearc.org/news/2018/july/australian-ham-radio-exam-system-under-review.htm#.W6cY42gzbIUMeteor scatter infohttps://www.electronics-notes.com/articles/ham_radio/amateur-propagation/meteor-scatter-burst-communications.php

Some interesting links to try

HOT NEWS

Buy, Swap Sell,

If you have anything to sell or swap or if you are looking for something to buy, that elusive bit of equipment that you have been looking for, this is the place to advertise it, just send the details to the secretary and she will pass this on to be published in the following month newsletter. Just make sure that you include your details, perhaps just your callsign.

Club Luncheon

Remember the next club luncheon will be on the 13th of October at the Blue Mountain Hotel in Ruthven st. Harlaxton. To book your place please call Theo on 46910371. Good meals and good company is to be enjoyed by all, come and join us for a wonderful get together.

JOTAPreparations for the Jamboree on the Air for the Oakey and Bunya Park Scouts/Guides in Toowoomba are well under-way. Equipment has been sourced as well as antennas, they are all ready to be in place for a good week end.

Social/Technical Meeting

Another social/tech meeting has been and gone. We had an informative meeting with most of the discussions revolving around JOTA. Many thanks goes out to Alec Brown from the Bunya Park Scout group for his attendance. Alec had a few questions for us as well as answering a few question that we had. Alec has been very enthusiastic with our involve-ment in JOTA and also very keen in assisting us with other projects that we can attempt at the scout den. Another issue that was briefly discussed was the possibility of live streaming the social/technical meetings in the future, this will be mainly for those members that for whatever rea-son cannot attend in person, they will not miss out.

Traveling to the Sun: Why Won’t Parker Solar Probe Melt?

This summer, NASA’s Parker Solar Probe will launch to travel closer to the Sun, deeper into the solar atmosphere, than any mission before it. If Earth was at one end of a yard-stick and the Sun on the other, Parker Solar Probe will make it to within four inches of the solar sur-face.Inside that part of the solar atmosphere, a region known as the corona, Parker Solar Probe will provide unprecedented observations of what drives the wide range of particles, energy and heat that course through the region — flinging particles outward into the solar system and far past Neptune.Inside the corona, it’s also, of course, unimaginably hot. The spacecraft will travel through material with temperatures greater than a million degrees Fahrenheit while being bombarded with intense sun light.So, why won’t it melt?Parker Solar Probe has been designed to withstand the extreme conditions and temperature fluctuations for the mission. The key lies in its custom heat shield and an autonomous sys-tem that helps protect the mission from the Sun’s intense light emission, but does allow the coronal material to “touch” the spacecraft.

The Science Behind Why It Won’t MeltOne key to understanding what keeps the spacecraft and its instruments safe, is understand-ing the concept of heat versus temperature. Counterintuitively, high temperatures do not always translate to actually heating another object.In space, the temperature can be thousands of degrees without providing significant heat to a given object or feeling hot. Why? Temperature measures how fast particles are mov-ing, whereas heat measures the total amount of energy that they transfer. Particles may be moving fast (high temperature), but if there are very few of them, they won’t transfer much energy (low heat). Since space is mostly empty, there are very few particles that can trans-fer energy to the spacecraft.The corona through which Parker Solar Probe flies, for example, has an extremely high tem-perature but very low density. Think of the difference between putting your hand in a hot oven versus putting it in a pot of boiling water (don’t try this at home!) — in the oven, your hand can withstand significantly hotter temperatures for longer than in the water where it has to interact with many more particles. Similarly, compared to the visible surface of the Sun, the corona is less dense, so the spacecraft interacts with fewer hot particles and doesn’t receive as much heat.That means that while Parker Solar Probe will be traveling through a space with tempera-tures of several million degrees, the surface of the heat shield that faces the Sun will only get heated to about 2,500 degrees Fahrenheit (about 1,400 degrees Celsius).

The Shield That Protects ItOf course, thousands of degrees Fahrenheit is still fantastically hot. (For comparison, lava from volcano eruptions can be anywhere between 1,300 and 2,200 F (700 and 1,200 C) And to withstand that heat, Parker Solar Probe makes use of a heat shield known as the Thermal Protection System, or TPS, which is 8 feet (2.4 meters) in diameter and 4.5 inches (about 115 mm) thick. Those few inches of protection mean that just on the other side of the shield, the spacecraft body will sit at a comfortable 85 F (30 C).The TPS was designed by the Johns Hopkins Applied Physics Laboratory, and was built at Carbon-Carbon Advanced Technologies, using a carbon composite foam sandwiched between two carbon plates. This lightweight insulation will be accompanied by a finishing touch of white ceramic paint on the sun-facing plate, to reflect as much heat as possible. Tested to withstand up to 3,000 F (1,650 C), the TPS can handle any heat the Sun can send its way, keeping almost all instrumentation safe.

The Cup that Measures the WindBut not all of the Solar Parker Probe instruments will be behind the TPS.Poking out over the heat shield, the Solar Probe Cup is one of two instruments on Parker So-lar Probe that will not be protected by the heat shield. This instrument is what’s known as a Faraday cup, a sensor designed to measure the ion and electron fluxes and flow angles from the solar wind. Due to the intensity of the solar atmosphere, unique technologies had to be engineered to make sure that not only can the instrument survive, but also the electronics aboard can send back accurate readings.

Parker Solar Probe’s heat shield is made of two panels of superheated carbon-car-bon composite sandwiching a lightweight 4.5-inch-thick carbon foam core. To reflect as much of the Sun’s energy away from the spacecraft as possible, the Sun-facing side of the heat shield is also sprayed with a specially formulated white coating.Credits: NASA/Johns Hopkins APL/Ed Whitman

The cup itself is made from sheets of Titanium-Zirconium-Molybdenum, an al-loy of molybdenum, with a melting point of about 4,260 F (2,349 C). The grids that produce an electric field for the Solar

Probe Cup are made from tungsten, a metal with the highest known melting point of 6,192 F (3,422 C). Normally lasers are used to etch the gridlines in these grids — however due to the high melting point acid had to be used instead.Another challenge came in the form of the electronic wiring — most cables would melt from exposure to heat radiation at such close proximity to the Sun. To solve this problem, the team grew sapphire crystal tubes to suspend the wiring, and made the wires from niobium.To make sure the instrument was ready for the harsh environment, the researchers needed to mimic the Sun’s intense heat radiation in a lab. To create a test-worthy level of heat, the researchers used a particle accelerator and IMAX projectors — jury-rigged to increase their temperature. The projectors mimicked the heat of the Sun, while the particle accelerator exposed the cup to radiation to make sure the cup could measure the accelerated particles under the intense conditions. To be absolutely sure the Solar Probe Cup would withstand the harsh environment, the Odeillo Solar Furnace — which concentrates the heat of the Sun through 10,000 adjustable mirrors — was used to test the cup against the intense solar emission.The Solar Probe Cup passed its tests with flying colors — indeed, it continued to perform better and give clearer results the longer it was exposed to the test environments. “We think the radiation removed any potential contamination,” Justin Kasper, principal investigator for the SWEAP instruments at the University of Michigan in Ann Arbor, said. “It basically cleaned itself.”The Spacecraft That Keeps its CoolSeveral other designs on the spacecraft keep Parker Solar Probe sheltered from the heat. Without protection, the solar panels — which use energy from the very star being studied to power the spacecraft — can overheat. At each approach to the Sun, the solar arrays retract behind the heat shield’s shadow, leaving only a small segment exposed to the Sun’s intense rays.But that close to the Sun, even more protection is needed. The solar arrays have a sur-prisingly simple cooling system: a heated tank that keeps the coolant from freezing during launch, two radiators that will keep the coolant from freezing, aluminum fins to maximize the cooling surface, and pumps to circulate the coolant. The cooling system is powerful enough

to cool an average sized living room, and will keep the solar arrays and instrumentation cool and functioning while in the heat of the Sun.

In the Astrotech processing facility in Titus-ville, Florida, near NASA's Kennedy Space Center, on Tuesday, June 5, 2018, techni-cians and engineers perform light bar test-ing on NASA's Parker Solar Probe. The spacecraft will launch on a United Launch Alliance Delta IV Heavy rocket from Space Launch Complex 37 at Cape Canaveral Air Force Station in Florida. The mission will perform the closest-ever observations of a star when it travels through the Sun's at-mosphere, called the corona. The probe will rely on measurements and imaging to revo-lutionize our understanding of the corona and the Sun-Earth connection.

Credits: NASA/Glenn Benson

The coolant used for the system? About a gallon (3.7 liters) of deionized water. While plenty of chemical coolants exist, the range of temperatures the spacecraft will be exposed to varies between 50 F (10 C) and 257 F (125 C). Very few liquids can handle those ranges like water. To keep the water from boiling at the higher end of the temperatures, it will be pressurized so the boiling point is over 257 F (125 C).Another issue with protecting any spacecraft is figuring out how to communicate with it. Parker Solar Probe will largely be alone on its journey. It takes light eight minutes to reach Earth — meaning if engineers had to control the spacecraft from Earth, by the time something went wrong it would be too late to correct it.So, the spacecraft is designed to autonomously keep itself safe and on track to the Sun. Sev-eral sensors, about half the size of a cell phone, are attached to the body of the spacecraft along the edge of the shadow from the heat shield. If any of these sensors detect sunlight, they alert the central computer and the spacecraft can correct its position to keep the sen-sors, and the rest of the instruments, safely protected. This all has to happen without any human intervention, so the central computer software has been programmed and extensively tested to make sure all corrections can be made on the fly.

Launching Toward the SunAfter launch, Parker Solar Probe will detect the position of the Sun, align the thermal protec-tion shield to face it and continue its journey for the next three months, embracing the heat of the Sun and protecting itself from the cold vacuum of space.Over the course of seven years of planned mission duration, the spacecraft will make 24 orbits of our star. On each close approach to the Sun it will sample the solar wind, study the Sun’s corona, and provide unprecedentedly close up observations from around our star — and armed with its slew of innovative technologies, we know it will keep its cool the whole time.

An illustration of Parker Solar Probe approaching the Sun.Credits: NASA/Johns Hop-kins APL/Steve Gribben

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