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bob-c

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Posts posted by bob-c

  1. 3 minutes ago, geoflewis said:

    There is a strong body of opinion that high resolution planetary imaging isn't possible with a fast jetstream parked overhead. Whilst experience indicates that is a reasonable general rule, there have been several occasions when that has not been proved true. Take last night as an example......

    My wife and I had been binge watching the David Tenent 4 part series "Inside Man" and were heading for bed around midnight, but as usual I popped my head outside first and to my surprise there was a clear sky. I checked a couple of weather sites, including the jetstream forecast and thought, NO, I'll be wasting my time, then thought again, well why not give it a go. FYI here are 2 jetstream forecast for midnight 14 October and 1am 15 October - different sites, but essentially the same with a fast jetstream parked over the UK.

    Jetstream_15Oct22_0000.JPG.fbce11972d5149465fed396be907ad71.JPG

    Jetstream_15Oct22_0100.thumb.JPG.2cd7bc5e1b617122a3aa871a4c717031.JPG

    So how did I capture this?

    2022-10-14-2347_9-GDL_RGB_PIPP(F6000)-DeRot_lapl4_ap26_P100_sharp_R6_AFP_R6(v2-DN)_AFP.jpg.2c0120111535d7db7a8b8252cfc43c61.jpg

    Ok, so maybe not fully hi res, but far better than I saw a few nights ago with the jetsream out of the way. I managed 5 x 6 min SERs over about 45 mins, the above image comprising best 6000 frames from 3 of the de-rotated and quality graded SERs, so 18000 frames in total.

    After Jupiter, I thought I'd try Mars for the first time this year, however, by the time I got Mars on the sensor and defined capture settings in FireCapture, fog had rolled in so quickly that Mars was no longer visible naked eye, and the nearby waning moon had dimmed considerably, so I called it a wrap. It seems that if the jetstream doesn't always get you, then fog definitely will.

    So back to imaging through a fast jetstream; it's something that I've discussed a few times with my mentor, Dave Tyler, who suggests that it's not just the jetstream, but whether it comprises a steady laminar flow, or there is turbulant mixing going on. My location in south Norfolk was right in the middle of the flow last night and I suspect that whilst the atmosphere was fast moving, it was doing so at a stable rate, not mixing as much as it might do at the edges of the stream. It's just a contention, but nevertheless, not for the first time I was able to image fairly successfully through the jetstream.

    I'm interest to learn what others think about this.

     

    Don't know much about the Jet stream Jeff, but it looks a fine image to me. 

     

    Bob.

    • Thanks 1
  2. 3 hours ago, robin_astro said:

    I love the blue colour, confirmed by the spectrum which is brighter at the blue end

    Here is the raw  spectrum image. (Using an ALPY 600 spectrograph)

    SN2022hrs_ALPY600_raw_4x600s_20220422.png.3b631ddbb5c077b42650b91bbc1bf053.png

    The deep absorption line marked is from singly ionised Silicon formed by nuclear fusion in the thermonuclear explosion of  the white dwarf (this is a type 1a). 

    (The other lines in the background are from natural airglow and light pollution)

    and here is the calibrated spectrum 

    image.png.aff27d6d9d5969a1506f2cbb4756546e.png

    We can measure the velocity of the  material thrown out by the explosion by how far the absorption line has been blue shifted due to the doppler effect (~15000 km/s.) The silicon is actually from the partially "nuclear burned" material near the surface of the white dwarf. Heavier elements up to Iron are produced  by further fusion deeper within the explosion. It is near maximum at about mag 12.5 currently which, taking into account the distance to the galaxy makes it several billion time more luminous than the sun

    Cheers

    Robin

    Thanks Robin for this information,  it is a bit above my old head though to take in but i am fascinated by all of it, thank you very much .

     

    Bob.

  3. Hi , thought i would have a try for the new (SN2022HRS) supernova that was discovered on the 16th of this month in NGC4647 in Virgo. It outshines the host galaxy easily. It consists of 10x600s stacked and processed in APP and Photoshop.

    Equipment used, OOUK ODK12 ,  A A 294c ProTec Hypercam,  Ioptron 120ec mount. Zwo 290 mini guide cam.

    Capture Software  APT.  and guided with Phd2.

     

    Bob

    10FRS_600S-SUPERNOVA copy.jpg

    10FRS_600S-SUPERNOVA  2022HRS.copy.jpg

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