solar corona and wind Langmuir wave structure

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notFritzArgelander
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solar corona and wind Langmuir wave structure

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Post by notFritzArgelander »


This is more of a solar radio than optical thing. Let me know if its beside the point.

https://phys.org/news/2021-09-langmuir- ... urces.html
Scopes: Refs: Orion ST80, SV 80EDA f7, TS 102ED f11 Newts: AWB 130mm, f5, Z12 f5; Cats: VMC110L, Intes MK66,VMC200L f9.75 EPs: KK Fujiyama Orthoscopics, 2x Vixen NPLs (40-6mm) and BCOs, Baader Mark IV zooms, TV Panoptics, Delos, Plossl 32-8mm. Mixed brand Masuyama/Astroplans Binoculars: Nikon Aculon 10x50, Celestron 15x70, Baader Maxbright. Mounts: Star Seeker IV, Vixen Porta II, Celestron CG5
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FRAZ Scotland
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Re: solar corona and wind Langmuir wave structure

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Post by FRAZ »


A couple of thoughts:

This has been examined since the 1970's! That is a surprise, I would have thought the technology was much more limited the further back we go.
It seems a huge expense to use the more current Parker Solar Probe and Solar Orbiter to collect this data but then I suppose if it is already collected it is just a matter of interpreting the data.
Mentored by Keith, Mike, John and Bill. (The old guard) and forever grateful.

Spending obscene amounts of money building a big fracking solar telescope.
(Trying my best not to curse or swear :) )
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Re: solar corona and wind Langmuir wave structure

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LOFAR - The low frequency array is used here so I looked at a 6 minute explanation of what it is here.

Mentored by Keith, Mike, John and Bill. (The old guard) and forever grateful.

Spending obscene amounts of money building a big fracking solar telescope.
(Trying my best not to curse or swear :) )
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notFritzArgelander
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Re: solar corona and wind Langmuir wave structure

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Post by notFritzArgelander »


FRAZ wrote: Wed Sep 15, 2021 10:40 am A couple of thoughts:

This has been examined since the 1970's! That is a surprise, I would have thought the technology was much more limited the further back we go.
It seems a huge expense to use the more current Parker Solar Probe and Solar Orbiter to collect this data but then I suppose if it is already collected it is just a matter of interpreting the data.
The probes have additional capabilities that provide information unavailable from an Earth observatory. Optical imaging, particle counts and local EM field measurements help ground radio observation .
Scopes: Refs: Orion ST80, SV 80EDA f7, TS 102ED f11 Newts: AWB 130mm, f5, Z12 f5; Cats: VMC110L, Intes MK66,VMC200L f9.75 EPs: KK Fujiyama Orthoscopics, 2x Vixen NPLs (40-6mm) and BCOs, Baader Mark IV zooms, TV Panoptics, Delos, Plossl 32-8mm. Mixed brand Masuyama/Astroplans Binoculars: Nikon Aculon 10x50, Celestron 15x70, Baader Maxbright. Mounts: Star Seeker IV, Vixen Porta II, Celestron CG5
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