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Rob48
You are reading and listening to people who were not actually there back in the day...they were somewhere else..."on the outside looking in"; and you think they are reporting everything correctly...you are truly funny!
The SOHO team were certainly there back in the day, when they wrote that handbook. And James Janesick seems to have been there too, based on that Sky & Telescope piece from 1987, written by one James Janesick of Caltech and Morley Blouke of, erm, Tektronix.edit on 17-4-2014 by Rob48 because: (no reason given)
tanka418
Rob48
In basic terms, energetic particles striking the silicon atoms in the CCD and "knocking the electrons out of orbit", liberating them into the pixel sites along the track of the particle. Electrons, of course, being what a CCD is recording. (Yes I know electrons aren't really "orbiting", but if an analogy is good enough for my chemistry professors it is good enough for me.)
(By the way, the CCD pictured is not the one used in SOHO. The ones used in the LASCO imagers are less than half that size, being 1024 x 1024 pixels with 21μm pixels.)
Thank you...21um technology...
Now, can you find the penetration depth of your typical atomic nuclei?
Then explain just how there are "streaks" longer than 2 pixels.
tanka418
Here is where your misunderstanding is coming from: Tektronix has never been a "chip maker", they are however, one of the best / most famous instrument makers n the industry. They have traditionally designed and manufactured instruments across a wide variety of industry and discipline. Thus they would be quite likely, and in fact seem to have designed and produced imaging systems using CCD devices. However, like most companies like that; all they really do is integrate existing technology into a useful system. That's what I do, along with virtually every other technology company (I own my own software house).
So...while SOHO and probably many other imaging systems may be based on an imaging system produced by Tek. Tek still did not product the actual CCD device, even IF it was originally a custom build for Tek.
The largest charged coupled-device currently available is made by Tektronix, Inc.
Tek have had problems with the flatness of their and devices. An approximately bow has been observed in their devices, this bow originating in the wafer itself during processing. The wafers take on the shape of part of a spherical surface and this results in a centre-to-edge change in flatness of, at worse, . This curvature should be easily seen in all our instruments, especially in optical systems with fast beams.
Rob48
tanka418
Rob48
In basic terms, energetic particles striking the silicon atoms in the CCD and "knocking the electrons out of orbit", liberating them into the pixel sites along the track of the particle. Electrons, of course, being what a CCD is recording. (Yes I know electrons aren't really "orbiting", but if an analogy is good enough for my chemistry professors it is good enough for me.)
(By the way, the CCD pictured is not the one used in SOHO. The ones used in the LASCO imagers are less than half that size, being 1024 x 1024 pixels with 21μm pixels.)
Thank you...21um technology...
Now, can you find the penetration depth of your typical atomic nuclei?
Then explain just how there are "streaks" longer than 2 pixels.
Homework time, is it?
OK, well, the penetration depth will depend on the energy of the particle, of course.
I've found a cite giving the mean rate of energy loss for cosmic ray particles in silicon as 387 eV per μm. [1]
So the energy loss across one pixel should be of the order of 387 eV x 21 = 8.1 keV.
Theoretically, assuming the particle came in completely parallel with the plane of the CCD, it seems to me that a particle with an energy above about 1024 x 8.1 keV = 8.3 MeV could make it across the entire CCD. Given that SOHO regularly encounters particles with energies well above 10 MeV, I'd say there should be plenty of streaks longer than two pixels.
[1] Radiation events in astronomical CCD images
Alan R. Smith ; Richard J. McDonald ; Donna C. Hurley ; Steven E. Holland ; Donald E. Groom ; William E. Brown ; David K. Gilmore ; Richard J. Stover ; Mingzhi Wei
Proc. SPIE 4669, Sensors and Camera Systems for Scientific, Industrial, and Digital Photography Applications III, 172 (April 26, 2002); doi:10.1117/12.463423
originally posted by: ngchunter
Rob48
Very nice citation. I think that settles it, both from the theoretical side, and from the observational side. I seriously doubt he'll ever admit he was wrong about it though. It's amusing that he thinks he'd "be the first" to admit he was wrong.
Yes, indeed it is a very nice citation.
Too bad I had to lead y'all by the hand so that you could find the proof that those streaks could be cosmic rays.
Y'all went round and round through so many misconceptions, misunderstandings...hell I bet y'all still don't quite understand what happened...that's okay...I do.
So, now that those streaks "might possibly" be cosmic rays, all you need to do is get past overall systems reliability, and of course probability.
originally posted by: tanka418
Yes, indeed it is a very nice citation.
Too bad I had to lead y'all by the hand so that you could find the proof that those streaks could be cosmic rays.
originally posted by: Rob48
Homework time, is it?
OK, well, the penetration depth will depend on the energy of the particle, of course.
I've found a cite giving the mean rate of energy loss for cosmic ray particles in silicon as 387 eV per μm. [1]
So the energy loss across one pixel should be of the order of 387 eV x 21 = 8.1 keV.
Theoretically, assuming the particle came in completely parallel with the plane of the CCD, it seems to me that a particle with an energy above about 1024 x 8.1 keV = 8.3 MeV could make it across the entire CCD. Given that SOHO regularly encounters particles with energies well above 10 MeV, I'd say there should be plenty of streaks longer than two pixels.
originally posted by: ngchunter
Holy crap, all that and this is your response? So now you're going to pretend you knew all this already and you just spewed a bunch of false claims to "lead us around." All so that what, we'd come back to the same point we were at pages ago? Yeah, you must think we're idiots if you expect us to believe that. I want you to say the following words, "I was wrong, I'm sorry." Is that really so impossible for you? I guess so. Well gentlemen, I think this is as close as we're ever going to get to an admission from tanka that he was wrong and we were right. Adios, have yourselves a good easter.
Too bad I had to lead y'all by the hand so that you could find the proof that those streaks could be cosmic rays.
originally posted by: Rob48
a reply to: tanka418
Well, I wasn't going to bother to dignify this ridiculousness with a reply, but just on the off chance anyone doesn't recognise that this "old engineer" (who I suspect has never been within a hundred yards of a naked silicon chip) is an old troll, I'll leave this here.
Too bad I had to lead y'all by the hand so that you could find the proof that those streaks could be cosmic rays.
Sometimes, there just aren't enough faces and enough palms.
Now you can argue all you like, but especially "back in the day" setting up a chip manufacturing facility was quite expensive, so...many companies, even large ones, contracted someone else to do the actual manufacture... even the design aspect. And then of course the part would have their mane on it.
With its focus on scientific-grade CCD imaging components and modules, SITe provides standard designs, user defined custom CCDs, and foundry services. SITe's engineering and manufacturing team builds custom CCD
imagers for use in the most demanding applications including NASA programs, satellite platforms, and other
research projects. Device formats are available as front illuminated or thinned, back illuminated CCDs.
Innovation, process development, and design experience date back to the founding of the group in 1974.
In September 1999, the company completed construction of a new 2,600 square foot Class 100 clean room for packaging and testing of imaging sensors. Currently, the 36,000 square foot Tigard manufacturing facility is being expanded to include a Class 10 clean room environment capable of thinning four- and six-inch and larger wafers.
SITe focuses on the design and manufacture of scientific grade CCD imaging components and modules, providing both standard designs and custom CCDs for user-defined performance specifications. SITe also offers CCD fabrication services for customers with specialized imager designs.
originally posted by: Rob48
tanka418
Thank you...21um technology...
Now, can you find the penetration depth of your typical atomic nuclei?
Then explain just how there are "streaks" longer than 2 pixels.
Homework time, is it?
OK, well, the penetration depth will depend on the energy of the particle, of course.
I've found a cite giving the mean rate of energy loss for cosmic ray particles in silicon as 387 eV per μm. [1]
So the energy loss across one pixel should be of the order of 387 eV x 21 = 8.1 keV.
Theoretically, assuming the particle came in completely parallel with the plane of the CCD, it seems to me that a particle with an energy above about 1024 x 8.1 keV = 8.3 MeV could make it across the entire CCD. Given that SOHO regularly encounters particles with energies well above 10 MeV, I'd say there should be plenty of streaks longer than two pixels.
[1] Radiation events in astronomical CCD images
Alan R. Smith ; Richard J. McDonald ; Donna C. Hurley ; Steven E. Holland ; Donald E. Groom ; William E. Brown ; David K. Gilmore ; Richard J. Stover ; Mingzhi Wei
Proc. SPIE 4669, Sensors and Camera Systems for Scientific, Industrial, and Digital Photography Applications III, 172 (April 26, 2002); doi:10.1117/12.463423
originally posted by: ngchunter
And the troll goes right back to claiming the "long ones aren't cosmic rays" so I will again quote this awesome post showing that indeed it would not be abnormal for cosmic rays to even go through the ENTIRE image.
originally posted by: tanka418
Some of what you call cosmic rays are in fact system noise. Some of the Cosmic rays seen in NASA images are the result of image processing...that was why I asked if you had viewed raw data...apparently not. If you had you should know about the amplification process NASA uses and the fact that it can turn a black cell grey (change a pixel value from 0 (zero) to some value greater than 0. Then of course once you know that they do these things, it is important to understand "why".
originally posted by: tanka418
a reply to: Rob48
Okay...I see that...built all that in 1999...some time after SOHO was launched. And, a bit after the time frame we were discussing as well.