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Hmmm, give or take a few millimeters? A millimeter is 0.0394 inches or thereabouts. A “few” might make a difference? I was always reminded of trying to get the very best precision when fabricating and locating the important parts.
Larry
Pahrump, nv
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Dr. Wilson, I wasn’t trying to be disparaging.
I have been and am still in this situation myself, lol. I was just trying to sort out things that might be causing you issues in your signal acquisition and processing. 2 mm is a pretty large discrepancy (I think and that may be in error) at nearly 0.08 inches. If you had the aluminum sheet metal in small gauge thickness, I bet you could lay it out in the sheet and then have an air conditioning shop or even a high school shop class cut the pieces out for you. Then use aluminum angle at the corners and with a hand drill , drill and then install pop rivets to make the corners. Hack saw and a small vise would be almost all you need. I make a lot of stuff similarly.
Keep plugging away at it and I am sure you will resolve it all to your satisfaction!
Larry
Pahrump, NV
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Have you checked the swr of the feed to ensure that it's well matched to the 50ohm LNA impedance? If you don't have one yet, I very highly recommend purchase of these reduced function vna units. Well worth the price since it enables easy optimisation of antenna performance. Don't forget to also purchase a calibration set of short, open and 50 ohm terminations.
Alternatively the nano vna can do the same and much more but is more complicated to use.
Cheers,Hamish
On Wed, Jun 2, 2021, 00:26 Jon Wallace <wall...@comcast.net> wrote:
Kevin,I have written up my first attempts at detecting the H line with a SDR and it might be helpful for you to read through that (https://www.radio-astronomy.org/pdf/JonWallace-Article-SARAJournal-Feb-2019.pdf). There was also a good article in the journal last month.
I am not an engineer so will not be able to troubleshoot, but your peaks don't look like hydrogen line peaks and they should vary somewhat (the galaxy appears to move towards and away from us so the Doppler shift should show). Perhaps you could do a 24 hour scan at 1 Declination and see how the signal varies as I did for a test.
For such a small horn, you will need longer integration - I used 5 minutes. When I did 30 seconds on SDR# I got nothing. I have some trouble shooting ideas in my article that might be worth checking - like pointing at a cement floor to get a baseline...
Best of luck and hang in there! Someone here will help you find the problem.
Jon
On 06/01/2021 1:53 AM Kevin Wilson <kevinaw...@gmail.com> wrote:I spent the better part of Memorial Day doing a survey of Quadrant 3 of the Milky Way. The attached image shows the area of the six scans I made. These were 30-second integrations. I have also attached an image showing the combined spectra of the scans. All have the same general profile with a bump around 1420.3 MHz (presumably the hydrogen line) and another around 1419.5 MHz (source unknown), plus some noise at the left end of the scans. A scan of an area away from the galactic plane removes both bumps but leaves the noise at the left side.
I have two questions:
First, does anyone have any idea what the bump at 1419.5 could be? I thought it was just interference, but because it disappeared when pointed away from the galactic plane that explanation doesn't seem to fit.
Second, should the scans of hydrogen across that area show bumps with identical red shifts? I would have expected the speed of the hydrogen to be different at various points, so I'm surprised they all spanned 1420.23–1420.37 MHz. The only difference is in the signal strength. Is that normal? I want to make sure that what I am detecting is actually the hydrogen line and not something else.
I made scans that included integrations of up to 10 minutes, but those didn't seem to change the basic profile of the spectrum. All the scans combine in the attached spectrum were 30-second integrations.
Any help on this would be appreciated. I'm new to radio astronomy, but I've been doing visual astronomy as a hobby for 40 years. This horn antenna for hydrogen is my second radio astronomy build.
System:
- horn antenna
- Nooelec LDA with hydrogen line filter
- Nooelec SDR dongle
- Raspberry Pi 4 using GNU Radio with a spectrometer created by the Digital Signal Processing in Radio Astronomy (DSPIRA) group at the University of West Virginia
- SMU9250 to read altitude and azimuth
Kevin A. Wilson
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On Aug 23, 2021, at 10:59 AM, Kevin Wilson <kevinaw...@gmail.com> wrote:
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Hi Kevin,
Question, running the LNA off of the waveguide to the SDR, directly to your Raspberry PI, are the LNA & SDR protected from the weather or do you disconnect? In my setup, I'm looking to do something similar but need to determine if the LNA & SDR can be protected from rain or can they handle the outside elements?
Thanks.
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Hi Kevin,
Question, running the LNA off of the waveguide to the SDR, directly to your Raspberry PI, are the LNA & SDR protected from the weather or do you disconnect? In my setup, I'm looking to do something similar but need to determine if the LNA & SDR can be protected from rain or can they handle the outside elements?
Thanks.
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Hi Anthony: If I put holes as you suggest, my pipes will fill up with mud-dauber wasps nests. Very fine screen works. For larger enclosures, I throw in bug-killer vapor strips. Have to vacuum the bugs out in the spring, but at least no nests...
Don
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Marcus
The water condenses from the change from hot moist air to cold dry air. So an additional way to avoid this would be to keep the experiment in hot dry air. Desert anyone?
Paul
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Marcus
The seepage is one of the reasons I chose to use perforated aluminum stock for my conical design. The holes are small enough that they will not disrupt the RF integrity. They also reduce the weight of the antenna for one person handling. Additionally, they will allow easier bending the cone into its shape.
The design includes a 3 foot ring on the open end to stabilize the shape. It also has a ring midway down the cone for the same purpose and for mounting near the center of gravity considering the waveguide piece and cone weight.
Paul
That sounds like a "serious piece of iron". Good luck with it.
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Or better still, keep the active area a bit warmer than surroundings, either by normal electronics , or with an additional warming resistor.
The enclosure becomes the condensing surface, not the active circuit.
The final, necessary touch, is a weep hole at the lowest point to let the condensed water out.
Trying to seal boxes is doomed to failure, unless you go to hermetic extremes that will pass a hydrogen leak test. Be better way is breathing holes that let the water vapor out, naturally, before it condenses, and finally, the hot/cool division of surfaces for what remains to condense on.
Lester B Veenstra K1YCM MØYCM W8YCM 6Y6Y
452 Stable Ln (HC84 RFD USPS Mail)
Keyser WV 26726
GPS: 39.336826 N 78.982287 W (Google)
GPS: 39.33682 N 78.9823741 W (GPSDO)
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Home: +1-304-289-6057
US cell +1-304-790-9192
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From: sara...@googlegroups.com [mailto:sara...@googlegroups.com] On Behalf Of Paul Oxley
Sent: Wednesday, August 25, 2021 8:12 PM
To: sara...@googlegroups.com
Subject: Re: [SARA] Hydrogen Line Survey
Marcus
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Or in extremes, keep the chamber pressurized with dry nitrogen.
Lester B Veenstra K1YCM MØYCM W8YCM 6Y6Y
452 Stable Ln (HC84 RFD USPS Mail)
Keyser WV 26726
GPS: 39.336826 N 78.982287 W (Google)
GPS: 39.33682 N 78.9823741 W (GPSDO)
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Home: +1-304-289-6057
US cell +1-304-790-9192
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From: sara...@googlegroups.com [mailto:sara...@googlegroups.com] On Behalf Of Paul Oxley
Sent: Wednesday, August 25, 2021 8:12 PM
To: sara...@googlegroups.com
Subject: Re: [SARA] Hydrogen Line Survey
Marcus
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metal copper screen or galvanized mesh (Chicken wire square ½ inch grid foe example)
for example
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All you need is small plastic tie wraps to hold new grid to old grid
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