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Op 11 okt. 2021 om 16:43 heeft Job Geheniau <jobge...@gmail.com> het volgende geschreven:
Hi all,
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But a 409 MHz is possible to build a quad array of long Yagi without too much difficulty
http://www.bambi.net/sara/AntDesg.pdf
http://www.mtmscientific.com/yagi.pdf
Lester B Veenstra K1YCM MØYCM W8YCM 6Y6Y
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Op 13 okt. 2021 om 20:57 heeft 'Lester Veenstra' via Society of Amateur Radio Astronomers <sara...@googlegroups.com> het volgende geschreven:
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Op 13 okt. 2021 om 20:59 heeft eddiem...@gmail.com het volgende geschreven:
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Op 13 okt. 2021 om 21:17 heeft Mario I0NAA <mario...@gmail.com> het volgende geschreven:
The program Murmur, available from my web site http://i0naa.altervista.org/ , is designed to help in understanding if a receiving system is potentially able to detect Pulsar.
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This may be a dumb question, but why can't amateur radio astronomers, just do what the professionals do, link up those with radio astronomy antennas & receiver systems to form a large VLA?
Is it the math, lack of experience, the needed coordination and time among SARA members?
My question isn't just targeted at you, Job, this is to all in SARA, who are reading this email thread and are very experienced in RAS.
Looking for a reason as to why not?
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Ah, Marcus!
I knew you would answer, thank you!:-D
So, why don't we all think about it, no need to say yes or no right now, and perhaps maybe meet to plan out a solution (innovative), not requiring so much technical debt and economic resources maybe?
But, of course, over some time to gather RA business, technical and security requirements, because we are all very busy.
We could attempt this as a SARA member project. Wouldn't such an attempt catch RAS media attention, possibly intrigue some professionals to help, or be amused at such an attempt? Not to mention, it could motivate not just SARA members but others (donors or investors and new SARA members) who have a real fascination with Amateur Radio Astronomy. Especially since this hobby for the inexperienced as myself, is challenging (technical skills-wise) and for the citizen scientist, monetary-wise.
Remember when we were children or younger, we would try things without even giving much thought to the challenges, and not even paying much mind to those who would say, "Hey, you can't do that or no it can't be done".But as time goes on, the word NO has become ingrained in so many of us, our thoughts, subconscious, everyday thinking, and it's very easy for us to talk ourselves out of what could be!
That's my experience in life! I remember a quote, I saw, "When someone tells me no, it doesn't mean I can't do it, it simply means I can't do it with them"Karen E. Quinones Miller
Give it some thoughts, what Job Geheniau is doing, I find very intriguing and will do so, very soon, despite any math or technical challenges!
I've said too much as usual.:-D
On 2021-10-13 7:56 p.m., Anthony wrote:
I read read about your proposal, partially on your Canadian Centre for Experimental Radio Astronomy, website last week. My very reasons for inquiring about your surplus 5.5 M dish antenna. Because of reading about the Deuterium survey project and your "Unfortunate confluence of both corporate and municipal politics at Smith Falls".
Did a little research on several Deuterium experiements and it looked like the issues were with the location of the antennas & receivers, they needed to be in locations with very, very low RFI. operating at 327 MHz to obtain 92 cm D1 detection.
The common issue seemed to be around RFI at 327 MHz and tediously identifying all of the interference noise sources. Some of the articles I read, touched on search locations at the Galactic center, along with the Galactic anti-center, but the background temps of ~500K dominated the receiver temperature.
This meant, multiple beams (some experiments using eight antennas) and maybe longer integration time is required in order to obtain a significant detection of D1 at 92 cm, deuterium spin-flip transition. No wonder you stated 24x7, for two years! Some of these articles are dated 2004, 2005, and 2008. Not sure if there are any other experiments that were conducted and it didn't look like these experiments back then were100% sure of the detection D1, I may be wrong?
Guess any members interested, would require a location with very little RFI, bandpass filters in the range of 327 -600 MHz, centered on 327 MHz, a good amount of antennas (between at least 6 - 10 SARA members), and lots of our antenna time dedicated to conduct the IDEA experiment.
I wish other members were interested, this looks like a significant project that could yeild rewards!
But we all have our own interest in this hobby, and the social problem as you and Wolfgang brought out, I guess.
There ARE projects that are less technically demanding and require only "loose" coordination. I wrote about one I proposed a couple of years ago:
http://www.ccera.ca/files/memos/ccera-memo-0009.pdf
Got very little traction.
It distinguishes itself in a few important ways:
(1) The end result could produce results that are scientifically interesting and potentially novel
(2) Because everyone is pointing at the NCP, large numbers of stations could be looking at the same piece of sky 24/7 -- no tracking
required.
(3) No real-time data-sharing requirement.
(4) Antenna requirements are modest, and not everyone needs exactly the same antenna
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On Wed, Oct 13, 2021 at 9:34 PM Marcus D. Leech <patchv...@gmail.com> wrote:
On 2021-10-13 7:56 p.m., Anthony wrote:
I read read about your proposal, partially on your Canadian Centre for Experimental Radio Astronomy, website last week. My very reasons for inquiring about your surplus 5.5 M dish antenna. Because of reading about the Deuterium survey project and your "Unfortunate confluence of both corporate and municipal politics at Smith Falls".Did a little research on several Deuterium experiements and it looked like the issues were with the location of the antennas & receivers, they needed to be in locations with very, very low RFI. operating at 327 MHz to obtain 92 cm D1 detection.
The common issue seemed to be around RFI at 327 MHz and tediously identifying all of the interference noise sources. Some of the articles I read, touched on search locations at the Galactic center, along with the Galactic anti-center, but the background temps of ~500K dominated the receiver temperature.
This meant, multiple beams (some experiments using eight antennas) and maybe longer integration time is required in order to obtain a significant detection of D1 at 92 cm, deuterium spin-flip transition. No wonder you stated 24x7, for two years! Some of these articles are dated 2004, 2005, and 2008. Not sure if there are any other experiments that were conducted and it didn't look like these experiments back then were100% sure of the detection D1, I may be wrong?
Guess any members interested, would require a location with very little RFI, bandpass filters in the range of 327 -600 MHz, centered on 327 MHz, a good amount of antennas (between at least 6 - 10 SARA members), and lots of our antenna time dedicated to conduct the IDEA experiment.
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