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TI parts in LT Spice

Started by John Larkin October 12, 2022
On a sunny day (Thu, 13 Oct 2022 09:48:31 +0100) it happened Martin Brown
<'''newspam'''@nonad.co.uk> wrote in <ti8jcv$1pnk$2@gioia.aioe.org>:

>It is a stupid design of content management system that gives each new >entity a more or less random but unique filename from some rule. To >avoid typo collisions they populate its namespace sparsely.
This image impressed me today: https://www.space.com/solar-orbiter-5th-sun-flyby-video Of course I downloaded the animated gif, it has a similar cryptic name...
On 13/10/2022 11:24, Jan Panteltje wrote:
> On a sunny day (Thu, 13 Oct 2022 09:48:31 +0100) it happened Martin Brown > <'''newspam'''@nonad.co.uk> wrote in <ti8jcv$1pnk$2@gioia.aioe.org>: > >> It is a stupid design of content management system that gives each new >> entity a more or less random but unique filename from some rule. To >> avoid typo collisions they populate its namespace sparsely. > > This image impressed me today: > https://www.space.com/solar-orbiter-5th-sun-flyby-video > Of course I downloaded the animated gif, it has a similar cryptic name...
Of the recent JWST images these are particularly cool star https://webbtelescope.org/contents/media/images/01GEJB2906TM9VR2FSJ4TFMNQM planet Neptune & rings https://webbtelescope.org/contents/media/images/2022/046/01GCVNBC11Z11KDTJ5CFGTMX72 Again note random content management strings at work :( -- Regards, Martin Brown
On a sunny day (Thu, 13 Oct 2022 11:40:11 +0100) it happened Martin Brown
<'''newspam'''@nonad.co.uk> wrote in <ti8puc$1255$1@gioia.aioe.org>:

>On 13/10/2022 11:24, Jan Panteltje wrote: >> On a sunny day (Thu, 13 Oct 2022 09:48:31 +0100) it happened Martin Brown >> <'''newspam'''@nonad.co.uk> wrote in <ti8jcv$1pnk$2@gioia.aioe.org>: >> >>> It is a stupid design of content management system that gives each new >>> entity a more or less random but unique filename from some rule. To >>> avoid typo collisions they populate its namespace sparsely. >> >> This image impressed me today: >> https://www.space.com/solar-orbiter-5th-sun-flyby-video >> Of course I downloaded the animated gif, it has a similar cryptic name... > >Of the recent JWST images these are particularly cool > >star > >https://webbtelescope.org/contents/media/images/01GEJB2906TM9VR2FSJ4TFMNQM > >planet Neptune & rings > >https://webbtelescope.org/contents/media/images/2022/046/01GCVNBC11Z11KDTJ5CFGTMX72 > >Again note random content management strings at work :(
Lots to be discovered in the near infrared! Maybe with so many images of the same object around they _have_ to resort to some extra code in the filenames, I mean how many images of Neptune are around, thousands if not more?
On 13/10/2022 12:02, Jan Panteltje wrote:
> On a sunny day (Thu, 13 Oct 2022 11:40:11 +0100) it happened Martin Brown > <'''newspam'''@nonad.co.uk> wrote in <ti8puc$1255$1@gioia.aioe.org>: > >> On 13/10/2022 11:24, Jan Panteltje wrote: >>> On a sunny day (Thu, 13 Oct 2022 09:48:31 +0100) it happened Martin Brown >>> <'''newspam'''@nonad.co.uk> wrote in <ti8jcv$1pnk$2@gioia.aioe.org>: >>> >>>> It is a stupid design of content management system that gives each new >>>> entity a more or less random but unique filename from some rule. To >>>> avoid typo collisions they populate its namespace sparsely. >>> >>> This image impressed me today: >>> https://www.space.com/solar-orbiter-5th-sun-flyby-video >>> Of course I downloaded the animated gif, it has a similar cryptic name... >> >> Of the recent JWST images these are particularly cool >> >> star >> >> https://webbtelescope.org/contents/media/images/01GEJB2906TM9VR2FSJ4TFMNQM >> >> planet Neptune & rings >> >> https://webbtelescope.org/contents/media/images/2022/046/01GCVNBC11Z11KDTJ5CFGTMX72 >> >> Again note random content management strings at work :( > > Lots to be discovered in the near infrared!
It could be a real boon for cosmology. They can almost see back to the very first stars by using foreground Abell galaxy clusters as magnifying lenses (and accepting a lot of distortion). The sparkler galaxy is one such where the globular clusters around it are visible too. https://iopscience.iop.org/article/10.3847/2041-8213/ac90ca
> Maybe with so many images of the same object around they _have_ to resort to some extra code in the filenames, > I mean how many images of Neptune are around, thousands if not more?
I'd still prefer them named something like: <catalogue_name>_<YYYYMMDDHHMMSS>_<wavelength>_<lead observer>
>
-- Regards, Martin Brown
On 10/13/2022 14:20, Martin Brown wrote:
> On 13/10/2022 12:02, Jan Panteltje wrote: >> On a sunny day (Thu, 13 Oct 2022 11:40:11 +0100) it happened Martin Brown >> <'''newspam'''@nonad.co.uk> wrote in <ti8puc$1255$1@gioia.aioe.org>: >> >>> On 13/10/2022 11:24, Jan Panteltje wrote: >>>> On a sunny day (Thu, 13 Oct 2022 09:48:31 +0100) it happened Martin >>>> Brown >>>> <'''newspam'''@nonad.co.uk> wrote in <ti8jcv$1pnk$2@gioia.aioe.org>: >>>> >>>>> It is a stupid design of content management system that gives each new >>>>> entity a more or less random but unique filename from some rule. To >>>>> avoid typo collisions they populate its namespace sparsely. >>>> >>>> This image impressed me today: >>>> &nbsp;&nbsp; https://www.space.com/solar-orbiter-5th-sun-flyby-video >>>> &nbsp;&nbsp;&nbsp; Of course I downloaded the animated gif, it has a similar >>>> cryptic name... >>> >>> Of the recent JWST images these are particularly cool >>> >>> star >>> >>> https://webbtelescope.org/contents/media/images/01GEJB2906TM9VR2FSJ4TFMNQM >>> >>> >>> planet Neptune & rings >>> >>> https://webbtelescope.org/contents/media/images/2022/046/01GCVNBC11Z11KDTJ5CFGTMX72 >>> >>> >>> Again note random content management strings at work :( >> >> Lots to be discovered in the near infrared! > > It could be a real boon for cosmology. They can almost see back to the > very first stars by using foreground Abell galaxy clusters as magnifying > lenses (and accepting a lot of distortion). The sparkler galaxy is one > such where the globular clusters around it are visible too. > > https://iopscience.iop.org/article/10.3847/2041-8213/ac90ca > > >> Maybe with so many images of the same object around they _have_ to >> resort to some extra code in the filenames, >> I mean how many images of Neptune are around, thousands if not more? > > I'd still prefer them named something like: > > <catalogue_name>_<YYYYMMDDHHMMSS>_<wavelength>_<lead observer> >> >
The naming mess is typically the product of data intended for machine processing being served for human consumption. Like say the file names in unix world, they are case sensitive - which is OK as long as they are not meant for humans, which of course they are.
On 2022-10-13 12:40, Martin Brown wrote:
> On 13/10/2022 11:24, Jan Panteltje wrote: >> On a sunny day (Thu, 13 Oct 2022 09:48:31 +0100) it happened Martin Brown >> <'''newspam'''@nonad.co.uk> wrote in <ti8jcv$1pnk$2@gioia.aioe.org>: >> >>> It is a stupid design of content management system that gives each new >>> entity a more or less random but unique filename from some rule. To >>> avoid typo collisions they populate its namespace sparsely. >> >> This image impressed me today: >> https://www.space.com/solar-orbiter-5th-sun-flyby-video >> Of course I downloaded the animated gif, it has a similar cryptic name... > > Of the recent JWST images these are particularly cool > > star
A very cool picture indeed. The Wikipedia article claims that the periodic bands are shells of matter expulsed by periodic He fusion oscillations at an 8 year period, whereas the description with the JWST picture says it's a binary star with that period. I suppose the periodic bands would be a flat spiral then instead of a series of concentric shells. It's hard to be sure, but it looks like the bands are concentric. Jeroen Belleman
Gerhard Hoffmann wrote:
> Am 13.10.22 um 10:12 schrieb Martin Brown: >> On 13/10/2022 05:40, olaf wrote: >>> John Larkin <jlarkin@highlandsnipmetechnology.com> wrote: >>> >>> >>> &nbsp; >Everyone should just supply LT Spice models. A few semi makers do. >>> >>> I told that the TI guys every time. I also told them how nice parts I >>> can buy from Linear/Analog. You can hear teeth grinding in this >>> moments. :-D >> >> If the salesmen take that message of lost sales back home eventually >> the suits that want to keep them all encrypted will get the message. > > The TI op amp models work better in LT spice than those from AD, > as far as I have used them. > ADA4898 - THE HORROR! > > The first model got about everything wrong. Phase, > noise densities in Volts... > > Years later came a 2nd edition, it still has convergence > problems when you insert a second ADA4898 into your circuit, > completely unrelated. > I would not know how to create that behaviour if I wanted it. > > That design went TI.
The push to get native models for AD parts seems to have stalled since Mike Engelhardt left. A pity. Cheers Phil Hobbs -- Dr Philip C D Hobbs Principal Consultant ElectroOptical Innovations LLC / Hobbs ElectroOptics Optics, Electro-optics, Photonics, Analog Electronics Briarcliff Manor NY 10510 http://electrooptical.net http://hobbs-eo.com
On 13/10/2022 14:53, Jeroen Belleman wrote:
> On 2022-10-13 12:40, Martin Brown wrote: >> On 13/10/2022 11:24, Jan Panteltje wrote: >>> On a sunny day (Thu, 13 Oct 2022 09:48:31 +0100) it happened Martin >>> Brown >>> <'''newspam'''@nonad.co.uk> wrote in <ti8jcv$1pnk$2@gioia.aioe.org>: >>> >>>> It is a stupid design of content management system that gives each new >>>> entity a more or less random but unique filename from some rule. To >>>> avoid typo collisions they populate its namespace sparsely. >>> >>> This image impressed me today: >>> &nbsp; https://www.space.com/solar-orbiter-5th-sun-flyby-video >>> &nbsp;&nbsp; Of course I downloaded the animated gif, it has a similar cryptic >>> name... >> >> Of the recent JWST images these are particularly cool >> >> star > > A very cool picture indeed. The Wikipedia article claims that the > periodic bands are shells of matter expulsed by periodic He fusion > oscillations at an 8 year period, whereas the description with the > JWST picture says it's a binary star with that period.
I think W-R stars are pretty much already down to burning helium in their cores so that sounds implausible to me (but its not my area). I think the latter explanation is much more plausible and fits with observations in the X-ray here: https://academic.oup.com/pasj/article/67/6/121/2470041
> > I suppose the periodic bands would be a flat spiral then instead of > a series of concentric shells. It's hard to be sure, but it looks > like the bands are concentric.
Not necessarily. When the two stars are at their closest their strong solar winds tear across their surfaces and the weaker one loses lots of material. Weaker probably meaning the one with lowest surface gravity FWIW I see concentric shells of material too. Slightly odd shape though - I'd expected an oval symmetry like with planetary nebulae like M57. -- Regards, Martin Brown