First Drift Scan from my 2.4m Dish with Airspy Mini and VIRGO

[Ayushman Tripathi]

Hi!

Here's the H-line data I captured from my 2.4m dish station in a 21-hour drift scan. I've attached an interactive 3D HTML plot you can rotate, zoom, and hover to see RA, Dec, frequency, and Doppler velocity for each point, along with plot images.

You can see the RA progression in the plot corresponding to each hydrogen peak as the Milky Way drifted through the beam.

There's little to no RFI in the raw data now. I'll do longer observations soon and share the results.

I'll optimize the data processing and plotting in the coming days.

System details:

• Hardware: Airspy Mini

• Software: VIRGO-based script

• Feed: Cantenna with SAWbird H1 LNA

• System: Raspberry Pi 500, fully remote operation

•   Dish: Fixed pointing for now

3D HTML URL:   https://www.icloud.com/iclouddrive/078xlIb4HBU2AQ_MYqDiosd3Q#hline%5F3d%5Finteractive



Thanks

[Alex P]

Hello Ayushman,

Good Work !

Can you acquire a 24 hr slice at either Dec +20 dg or Dec +40 dg ?

These are some of the brightest regions of the MW.

Thanks,

Alex

[Ayushman Tripathi]

Hi Alex,

Thank you! Yes, I'll do 24/7 drift scans since the dish is fixed pointing and I'm obtaining the data remotely. I can visit once every ~2 months to adjust the pointing. The good thing is there's not even a single RFI spike visible in the raw data as I turned off even any light bulbs. 

I'll also create a Zenodo page so the data is properly archived and verifiable if I find anything unusual.

Thanks.

[b alex pettit jr]

Ayushman,

Why are you taking 24/7 scans of the same region ?

What changes from day to day ?

Do you have a better plot of this.

There seems to be an unusual pattern in the background .

Alex

[Ayushman Tripathi]

Hi Alex,

Stacking multiple days should improve SNR, and it also helps with transient detection since any unusual signals would stand out. Real astronomical signals should repeat, while RFI won’t.

I visit the site every 2 months, so I’ll change the pointing to a different declination on my next visit. My long-term goal is to set up 3-4 dishes of 2m or larger for SETI observations. A motorized remote control mount would be nice, but for a dish this size I’d need to build one myself. By the way I think for smaller dishes like DD and WiFi dish Discovery Drive motorized mount should be available soon as per the discovery dish web page,

Regarding the better plot, yes, I captured the data but haven’t processed it yet. I’ll process yesterday’s data soon and share. Did you get a chance to look at the 3D HTML plot?

Thanks.

On 11 Feb 2026, at 06:27, 'b alex pettit jr' via Society of Amateur Radio Astronomers <sara...@googlegroups.com> wrote:



Ayushman,

Why are you taking 24/7 scans of the same region ?

What changes from day to day ?

Do you have a better plot of this.

There seems to be an unusual pattern in the background .

<1770771252570blob.jpg>

Alex

On Tuesday, February 10, 2026 at 07:16:52 PM EST, Ayushman Tripathi <ayushmantr...@gmail.com> wrote:

Hi Alex,

Thank you! Yes, I'll do 24/7 drift scans since the dish is fixed pointing and I'm obtaining the data remotely. I can visit once every ~2 months to adjust the pointing. The good thing is there's not even a single RFI spike visible in the raw data as I turned off even any light bulbs. 

I'll also create a Zenodo page so the data is properly archived and verifiable if I find anything unusual.

Thanks.

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[Ayushman Tripathi]

Also, could you please point out which part you’re referring to ? 

And It might be a data processing artifact, I’ll be improving the processing soon.

Here’s the link of discovery drive: https://www.rtl-sdr.com/discovery-drive-an-affordable-antenna-rotator-crowd-funding-pre-launch-page-now-active/comment-page-1/

[Stephen Arbogast]

Congratulations  Ayushman, I  can tell  you are  are  excited. The  journey is just  beginning.

I  too  am waiting  for the Kraken RF   motor drive  for  my  discovery dish.

I am just  wondering   if  multiple  measurements  separated by days  would  be helpful since our  earth moves around the sun or  maybe  the differences would  be  insignificant...     any thoughts?

Stephen

[b alex pettit jr]

Hi Ayushman,

I looked at the 3D plot, but at that angle, it is difficult to eval the actual data ..

That is why I prefer the Z axis orientation.

" Also, could you please point out which part you’re referring to ? "

THIS

'Stacking' multiple days/weeks of signals will require LSR correction. Is that enabled in your software ?

Alex

======================================

On Tuesday, February 10, 2026 at 09:59:04 PM EST, Ayushman Tripathi <ayushmantr...@gmail.com> wrote:

Hi Alex,

Stacking multiple days should improve SNR, and it also helps with transient detection since any unusual signals would stand out. Real astronomical signals should repeat, while RFI won’t.

[fasleitung3]

As the earth moves around the sun and as a smaller contribution the earth rotates, there is a doppler shift which varies over time. The variation over just a few days may be not too significant but if you are talking about longer time frames this becomes important.

The solution to this is to correct all measurements for this and relate velocities to the local standard of rest. I highly recommend to do this in any case.

I wrote an article about this in the July/August 2021 issue of the SARA journal. For your convenience, I have attached this article here.

Best regards,

Wolfgang

[b alex pettit jr]

Thanks Wolfgang.

 this is a link to a VLSR Calculator 

http://f4klo.ampr.org/vlsrKLO.php

Alex

=============================

[b alex pettit jr]

This gives an idea of the VLSR error / day 

The VLSR curve shifts with respect to the MW as the Earth rotates about the Sun 

                Alex  P

[Ayushman Tripathi]

Hi Stephen,

Thanks! Yes, it'll help a lot for DD and WiFi dishes, as we can remotely control them then.

[Ayushman Tripathi]

Hi Alex,

Yes, that background jump in that RA slice, was not in yesterday's data, but it was in the 9th Feb data.  It might be something specific to that observation.
I'll try to find the reason why it appeared in that plot but not in yesterday's. I'll also reprocess the 9th Feb data to make sure something didn't get messed up in the script.

Yes, VIRGO supports VLSR, there's a vlsr=True parameter in the plot function that displays the graph in the VLSR frame of reference. I tried it last month and will try it again soon.
I've attached yesterday's plots and also the 3D HTML that you can rotate and check.


3D LIVE HTML: https://www.icloud.com/iclouddrive/0f4xYAqp0Xkwf6xu4eDn7l2MQ#hline%5F3d%5Finteractive_2

[b alex pettit jr]

Hi Ayushman,

What causes this  pattern in the plots ?

If you want to find low level signals, these could be a problem

[Ayushman Tripathi]

Hi Alex,

Those appear to be 3D rendering artifacts from matplotlib's 3D rendering. I'm working on fixing that.

Interestingly, when I plot the same data using Plotly (WebGL-based), those tiny squares don't appear.

Thanks.

You can find the whole 3D Plot attached here:  https://www.icloud.com/iclouddrive/0f4xYAqp0Xkwf6xu4eDn7l2MQ#hline%5F3d%5Finteractive_2

[b alex pettit jr]

Hi Ayushman,

This Looks Good !!!

Make sure any AGC option on the SDR is Disabled ( automatic gain control )

The dark region ( shown in box ) looks like a decreased gain due to the H signal  .. maybe ?

[Peet Denny]

Awesome stuff, Ayushman. Very beautiful.

What explains the sinusoidal distribution of *frequency* in this plot?

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[Alex P]

On Thursday, February 12, 2026 at 10:15:10 AM UTC-5 Peet Denny wrote:Awesome stuff, Ayushman. Very beautiful.

[Ayushman Tripathi]

Hi Alex,

Yes, looks like it. I'll make sure the AGC stays off, it should be off already, but I'll double-check.

Thanks.

[Ayushman Tripathi]

Hi Peet,

Thank You. Yes, as Alex mentioned, the plot is still in the topocentric frame. I’ll apply the VLSR correction and compare the result.

On Thursday, February 12, 2026 at 10:15:10 AM UTC-5 Peet Denny wrote:

[Stephen Arbogast]

Wolfgang,

Thank you for  your  article.  

[Ayushman Tripathi]

Hi Alex,

The artifact that appeared similar to automatic gain control (AGC) effect from the SDR was actually caused by the baseline correction. I’ve corrected it and will share a few days of VLSR-corrected averaged data soon.

I’ll also upload the data to GitHub weekly.

Also next month I’ll move my DD feed to the same remote location where the 2.4 m dish is installed, and use a 1.5 m solid dish instead of the WiFi dish as that place doesn't have RFI problem.

Thanks

[b alex pettit jr]

Hi Ayushman,

My correction technique is not always Perfect either  :)

Regards,

Alex