Incredible Images of the Sun 239
shelterit writes "A new swedish telescope facility in La Palma uses a new technology to remove the blurriness of the atmosphere to snap new and astonishingly sharp images of the sun. Want to have a closer look at the surface of it? Reminds me of paintings I did as a kid."
Hmm (Score:2, Insightful)
\/eeoh
Re:Hmm (Score:5, Informative)
Re:Hmm (Score:5, Interesting)
The filaments' newly revealed dark cores are seen to be thousands of kilometers long but only about 100 kilometers wide. Resolving features 100 kilometers wide or less is a milestone in solar astronomy and has been achieved here using sophisticated adaptive optics, digital image stacking, and processing techniques to counter the blurring effect of Earth's atmosphere. At optical wavelengths, these images are sharper than even current space-based solar observatories can produce.
Re:Hmm (Score:4, Insightful)
By using new technology earth based observatories have made an advance over *current* space based observatories. Doesn't it follow that by using the same advances space based observatories will exceed earth based ones once they can be implemented? Also, they're be no need for correcting for the atmosphere ...
Re:Hmm (Score:2)
Re:Hmm (Score:2)
Actually adaptive optics in space is nothing new. Since weight is a major factor in placing any payload in orbit, optical face sheets are made as thin as possible. Once freed of gravitational constraints, the optics will deform. Thermal deformations also come into play.
do the mods actually read these posts ? (Score:2, Insightful)
MtViewGuy says : While this new system works great for the visible spectrum of the Sun's output, you still want a space-based observatory to monitor the Sun's output in the other parts of the electromagnetic spectrum You will note that he ignores the critical first 3 words in that Nasa sentence.
teridon says "no, on the contrary, thats not true", and provides this quote from nasa.gov to support his refutation. "At optical wavelengths, these images are sharper than even current space-based solar observatories can produce."
and gets modded up to 5 ?
Hello.... READ. teridon basically confirmed what the other dude said - it works great, but only for for VISIBLE spectrum.
optical != electomagnetic.
/me shakes his head and mutters...
Re:do the mods actually read these posts ? (Score:2)
Lighten up "dude".
Re:do the mods actually read these posts ? (Score:2, Interesting)
Last week someone posted an incorrect formula for Bayesian filtering and got modded up to 5, and before that someone posted a completely bogus discussion of processor pipelining which also got modded up to 5.
Seems like all you have to do is provide the illusion of information to get modded up.
Re:Hmm (Score:2, Interesting)
Link to not-slashdotted image (Score:2)
Anyway, NASA puts up a new image every day, which you can check out by bookmarking this URL. [nasa.gov]
GIFs??? (Score:5, Insightful)
Re:GIFs??? (Score:5, Informative)
Look at art! (Score:3, Funny)
If you scroll down to the "bottom" of that image, line yourself up with the very top of that monstrous sunspot and then cut directly left, you can see a nearly perfect image of a face.
*sigh*
Now I guess we sit back and wait for the conspiracy theories to fly.
Re:Look at art! (Score:4, Funny)
It's a miracle!!!
No, the Way of the Gourd! (Score:2)
Geez.
Re:Look at art! (Score:5, Funny)
Seriously though, this is just another example of how the human brain is hot-wired to see faces in everything - even a colon, a dash and a bracket.
Re:Look at art! (Score:2)
If you take this out of context, as I did when I first read that, it sounds really wrong. Be on the lookout for goatse.cx replies...
Pictures in the flames (Score:4, Informative)
It's a phenomenon known as pareidolia [skepdic.com], and is quite a fascinating subject in its own right. Briefly, the human mind tends to seek patterns that it recognizes. When faced with a chaotic input, the mind creates patterns where none exist. Carl Sagan argues that faces in particular are hardwired into our recognition centres.
Incidentally, I can't see the face you're talking about there. (I'm probably not tired enough, as I find I'm very prone to seeing faces everywhere after an all-nighter.)
I did find a yin/yang symbol, though...
Mars Face (Score:2)
Re:GIFs??? (Score:3, Funny)
You can see all the horns at the top! Just above the central blackness! It's Satan and his minions! Reverend Bobby was RIGHT! It's the SCIENTISTS and all of their TECNOLOGY have finally!!! opened the DOOR TO HELL!!!!! He said they put DAEMONS in our computers, and on the InterNet, but I didn't believe!
Oh, JESUS, I am heartily sorry for the sins I have committed, and I reject the **EVIL** TECNOLOGY of the SCIENTISTS and their DAEMONS! Have Mercy On ME, oh LORD, and on my brother, Willum Jeffry Scraggins, who now lives in New York under the name of Will Craig, and also on his wife Rachel (though she is an Unbeliever, if you know what I mean).
Re:GIFs??? (Score:3, Interesting)
But, when I loaded it up, the color is just too intense. I tend to like softer blue patterns for my desktop (NT/W2k "Soap Bubbles" usually does the trick).
I used to have one that was rendered in blue (think it was an x-ray image or something) of the whole sun, made a nice soothing wallpaper on my CDE desktop. Wonder if I can find that one again (think it was originally linked from Blues News).
Re:GIFs??? (Score:4, Interesting)
APOD: January 6, 1997 - Blue Sun Glaring [nasa.gov]
Explanation: The Sun is a bubbling ball of extremely hot gas. In this false-color picture, light blue regions are extremely hot - over 1 million degrees, while dark blue regions are slightly cooler. The camera filter used was highly sensitive to the emission of highly charged iron ions, which trace the magnetic field of the Sun. The rich structure of the image shows the great complexity of the Sun's inner corona. A small active region can be seen just to the right and above center. This picture was taken in ultraviolet (extremely blue) light by the Extreme-ultraviolet Imaging Telescope (EIT) on board the Solar and Heliospheric Observatory (SOHO) spacecraft, which is orbiting the Sun just ahead of the Earth, at the L1 point. SOHO was launched in 1995 and will continually monitor the Sun for several years.
I just think that's one of the coolest things I've ever seen. I'll use that for my desktop again, now that I've found it again.
GIFs quite common in sat imaging (Score:5, Interesting)
GIFs were often used because it is a very stable way of doing lossless compression at 8bit, stable as in almost any image program can read them.
This is not the case with TIFFs as there are a number of variants and options in the file format.
TIFFs are however a better medium for storage of composite images, either spatially or spectorally (montages or multichannel pseudo colour in english).
Due to its general lack of use as a data storage format most of the tools I used/wrote to proccess image data files generally did not have JPEG support or other common 'display' options as the file is regarded as data, not an image - its a subtle difference but explains the mindset.
When I published stuff on the web I'd run our raw large images through Photoshop to get pleasing images but compact file sizes.
It may not have occured for them to do this, and anyway they may regard this as publishing data for other interested parties to download and process themselves.
Re:GIFs??? (Score:2)
Re:GIFs??? (Score:2)
Re:GIFs??? (Score:2)
Well, given the beating their site is getting right now, I'll bet they wish they had used a better format. :)
Re:GIFs??? (Score:3, Informative)
The sun?! Where?! (Score:5, Funny)
Re:The sun?! Where?! (Score:5, Funny)
Of course, I also live in Sweden and post on Slashdot, so I know that of which I speak.
Also on MSNBC (Score:5, Informative)
Re:Also on MSNBC One Question from article. (Score:2, Informative)
The highest resolution solar image ever shows part of the largest sunspot in Active Region 10030. The central region is dark because the strong magnetic fields there stop upwelling hot gas from the solar interior.
Ok, so that's SUPPOSED to explain why it's dark.. by I thought fire gave off light. While I can see a strong magnetic field blocking gas, shouldn't the surrounding gas give off enough light to see in the hole itself?
Or is the hole just THAT BIG? (But light from the sun gets to us, you'd think it could light a hole from all sides..)
Re:Also on MSNBC One Question from article. (Score:4, Informative)
The real reason they are "dark" is that they are cooler than the gas aronud them. Not that they are cold of course. From one of my astro textbooks:
Temperature of sunspot: 3900K
Temperature of surrounding photosphere: 5780K
Resulting in approximately 1/5 the flux (bolometric flux goes as T^4).
Doug
Re:Also on MSNBC One Question from article. (Score:2)
Ahh so there's just isn't a 'void' there as "stop upwelling hot gas from the solar interior", would seem to suggest. I guess 'cold' gas is upwelling from the interior :).
That's what I was wondering. Thanks!
Re:Also on MSNBC One Question from article. (Score:2)
Not quite, but almost. :-)
The magnetic fields are forcing upwelling gas away from the spot (hot as well as cold). However, the effect can only be so strong. Even the magnetic fields of the sun can't cause a complete vacuum in the sunspot. Gass will diffuse in from every direction.
The end result is that the region simply has a somewhat lower density than surrounding regions. Lower density==lower temperature==(much) lower luminosity.
re Paintings as a kid (Score:5, Funny)
Buried in the site (Score:5, Informative)
Re:Buried in the site (Score:2)
Re:Buried in the site (Score:3, Insightful)
That being said, I would be very surprised if there weren't military spy satellites, and perhaps reconnaisance planes, already using this.
Re:Buried in the site (Score:2)
Re:Buried in the site (Score:2, Interesting)
Re:Buried in the site (Score:2)
I see (Score:5, Funny)
Re:I see (Score:2)
Probably something about it being a star, though...
Bloody slashdotting (Score:2, Informative)
Slashdotted. (Score:2)
So will some kind hearts who can still access it copy the pages FTTB? I would myself, but I can't get in...
But it's nice the general scientific community still shares its assets, instead of copyrighting it and hiding it behind massive fees, like Craig Venter did.
<Offtopic> ;-)
Now if only I could find a geological map of the Netherlands without the usual atlas texts all over them, so i can make a nice RT2 simulation of the Dutch railways growth since trains got invented.
</Offtopic>
Stefan
Re:Slashdotted. (Score:4, Interesting)
sunspot [shacknet.nu]
you should do it fast though , it is my home machine and i cant hold on for long.
ill try to put the other page as sun.html
Appology (Score:5, Funny)
Re:Appology (Score:2)
Sorry for the spelling mistake my concious is moonlight powered.
Comment removed (Score:5, Funny)
Re:Appology (Score:2)
Re:Appology (Score:2)
Isn't this one of thos I was able, era I saw Elba thingys?
It's kinda mirrory all by itself!
Summer Fun (Score:5, Funny)
another link (Score:5, Informative)
This article [space.com] has the links.You can also zoom in and use the viewer.
Just what we need (Score:5, Funny)
Photos like these will show us where the potential landing sites are. Very useful since the lander will have to find somewhere that's not only flat but free of excessive RF noise so that we can communicate with Earth.
So, obviously, someone will ask - How can we possible build something to get to the sun? Well, this is quite simple, Firstly we use regrigeration devices. These will require some considerable energy, as well as a decent fusion power source to keep them going. Secondly, we avoif reflective surfaces. The other thing to remember is that we only need to travel during the night. During the day is when the sun is hottest, so travel at night should help cool us considerably. This will require better propulsion mechanisms that can do the bulk of the travelling in the 12 hours of night.
Re:Just what we need (Score:2)
Re:Just what we need (Score:2)
Mirror (Score:5, Funny)
Do you have a screen wipe? (Score:3, Funny)
Re:Mirror (Score:4, Funny)
Re:Mirror (Score:2, Funny)
Re:Mirror (Score:2, Funny)
mirror! (Score:5, Informative)
Re:mirror! (Score:2)
of course we shall see what optimium online has to say about this tomorrow...
Finally (Score:2, Funny)
Re:Finally (Score:2)
Bah, burn your pupils. What sort of teacher are you?
extra link. (Score:4, Informative)
Site is slow -- here's the content (Score:5, Funny)
____
/ \
| |
| |
\____/
Hope that helps to beat the Slashdotting.
Wow...that went fast. (Score:5, Funny)
Surfaces of extrasolar planets (Score:2)
Adaptive Optics (Score:5, Interesting)
This technology has been around for awhile, and was first seriously developed by the military at the Starfire Optical Range
Recently it has been used in such telescope projects as the WM Keck Observatory [hawaii.edu] and Gemini Project [gemini.edu]. I know AO is also used for measurement of eye aberrations, with projects being conducted at several Universities. For more information about Adaptive Optics, I suggest the Center for Adaptive Optics [ucolick.org]
My personal experience with AO was as an intern for Gemini this past summer. I helped write parallel code for a program that simulates current and future adaptive optics systems planned for the next generation of extremely large telescopes.
Re:Adaptive Optics (Score:4, Insightful)
Then you can chuck a frisbee like object through the beam and watch it get zapped
Did I say this was seriously frowned on, I think I should
Adaptive Optics in a Nutshell:
1) You use a single point source as a reference.
2) You know the aberation caused by the atmosphere will spread the point image when you receive it.
3) You know that as your source is a point source, then the resultant spread in your image is entirely due to aberation, so use the image to calculate the Point Spread Function
4) Using the PSF apply a correction to the light path by altering something in the imaging system, usually a mirror.
5) Repeat several hundred times a second
Of course the great side effect is this also removes distortion caused by the imaging system itself, allowing you to use bigger mirrors with a lower tolerance than you otherwise might be able to do.
Originally point sources were strong and predictable stars in the field of view that you wanted - hence the term 'guide stars'
With a laser generated guide star you project a spot onto the upper surface of the atmosphere with a powerful laser of an appropriate frequency - close to your obsering frequency, but far enough out that you don't effect the observation. The subtlety here is to account for the fact that the point source will be spread twice, once on the way up and once on the way down.
Anyone working in AO I apologise to for the somewhat oversimplification - follow the links in the parent to better details if your interest is fired.
Cooling question (Score:4, Interesting)
Btw, I tried to stare at the sun once when I was a kid, that was stupid. I was told too late that one can go blind for doing that -- that must explain the glasses today...
Re:Cooling question (Score:5, Interesting)
More light is collected. (Since astronomical telescopes are usually used to look at dim objects this is normally considered an advantage.)
To reduce the diffraction effects and so increase the spatial resolution.
When observing the sun, the second of these is still required but the first is a problem. The sun provides too much light, especially in the infrared, to observe safely.
The solution is to place a filter over the front of the telescope which cuts down the amount of light entering the scope. This reduction generally needs to be of the order of 1:1,000,000.
Filters at the back end of the telescope, directly in front of the eyepiece/camera, are not safe. All the heat from the sun passes the scope through and is focused through this small filter. They can then easily crack or melt.
Safety notice: The only safe filters for observing the sun are those designed for the job. They are usually thin plastic, sometimes glass, with a metal coating on both sides. Always check the filter is firmly fixed in place and has no scratches or pinholes. It is this filter type which was used in the eclipse safety glasses a few years back. When observing by eye, with no telescope, binoculars or other magnification, welder's No 14 glass or fully exposed and developed black and white film negatives are also safe. (Not colour film or b&w film developed with a colour process - it is the deposited metallic silver used in the b&w process which provides the protection.) NOTHING else is considered safe.
You can get cooled CCD cameras, and the astrophotographical community has been using them for years. (Well, those than can afford them anyway.) The cooling is required to reduce the 'dark current' within the camera itself during long exposures, not to remove incoming heat.
'Dark' Current explanation (Score:2, Informative)
Any matter will radiate energy according to its temperature - you've heard of this as Black Body Radiation.
Now in remote sensing you are often working in the IR region, because
a) this is where the 'windows' in the atmospheres absorption curve are
b) comparision of two bands give us intresting information - eg NVDI tells us the approximate vegitation cover from a simple comparisson of 2 channels.
In this case the detector must be cooler then the thing it is observing, otherwise your detector will respond to radiation emitted by itself and the equipment around it.
In the case of astronomical CCDs a similar effect is at work. CCDs work by creating small pockets in silicon that work very much like capacitors. The energy of photons (light particles) striking the material causes charge to build up in these pockets.
When enough charge has built up you can then 'read' the charge level in a similar way you can read memory (though clearly with more than a binary state) and infer the brightness of each pixel from the charge level.
This is fine for Video/Digital Photography use as a short exposure gets plenty of photons and you have an image.
In astronomy however you take exposure on a timescale of hours, sometimes your image maybe formed from a handful of photons. The problem here is that thermal processes in the CCD material itself can also deposit charge in the pockets by causing small stray currents and from phonon interaction in the silicon lattice itself.
If you cool the CCD in a dewar of liquid nitrogen, you limit these thermal issues, and have long exposures. The cost comes from building electronics that can survive the thermal shock of going from 25 Centigrade to -197 Centigrade in 10 minutes or so, and also having very very high quality CCDs to start with.
Been there, done that to extend the life of the 16inch telescope at my old Uni.
BTW - its not just an astronomy issue, consumers are starting to see it in digital cameras, especially SLR replacements. Take a look at a long exposure and you will see speccles - this is in part due to dark current, and in part due to increasing the gain of the CCD to try and limit the exposure length and therefore dark current issues - a tricky balance to get right, and some are better than others.
Re:Cooling question (Score:2, Informative)
Oddly enough, the CCD's generally are not cooled at all. The amount of light falling on the detector is actually not that great. Remember that each pixel corresponds to less than 0.1 x 0.1 arcsec, which means it covers about one-billionth of the solar surface (and hence the flux is one billion times less than integrated sunlight). Then you start taking very small slices in wavelength (0.01 nm or less, compared to the 100's of nanometers over the sun's emission peak in the visible wavelengths). Toss in a polarizer too (though they didn't use one in these observations), and next thing you know, you are running out of photons! That's why we need a big (by solar telescope standards) 4-meter telescope like the ATST ( http://atst.nso.edu [nso.edu]).
The exposure times in observations like these are also very short, on the order of 20 milliseconds or less, so there is no time for the dark current to build up during a long exposure (this is why nighttime CCD's, with exposures of minutes or hours, are often cooled). For some applications, even simple video rate CCD's can be used (the problem often being the small number of pixels).
As you might surmise, even if the detector isn't getting hit with that many photons, a lot of extra light is going through the telescope. Getting rid of waste heat IS a problem, and, as is the case with the Swedish Tower, often the main body of the telescope (entrance aperture -> main mirror -> instrument feed) is kept in a vacuum to reduce currents from heated air in the optical path. However, the Swedish Tower appears to be at the limit for the size of the entrance window (must be of optical quality and with minimal stress) that can be used (the entrance window is the size of the main lens on the Yerkes telescope [uchicago.edu] - the world's biggest refractor). That is why bigger telescopes like the GREGOR (1.5 m) and ATST (4 m) will be open, like nighttime telescopes, and will have to use different methods of thermal control. We can't go bigger than four meters now because of the limits of our thermal control capabilities.
Wish it was live. (Score:2)
Then I could actually finally have a decent use for transparent Term windows, I guess...
Hubble? (Score:2)
Re:Hubble? (Score:5, Informative)
Re:Hubble? (Score:2)
childhood pictures (Score:2, Funny)
Reminds me of paintings I did as a kid."
You painted pictures of 404 errors as a kid? Wow. We slashdotted the sun.
Slashdotted (Score:3, Funny)
It's amazing how (Score:3, Funny)
What?
Why are you all looking at me like that?
Mom always told you to not look into the Sun.. (Score:5, Funny)
Warning: Potentially Off-Topic Mirroring Comment (Score:2)
The Slashdot Effect is well known, and it seems like only the strongest sites are able to handle it. One of those sites, clearly, is Slashdot itself. Seems like there could be some mirroring done on Slashdot before a story is posted. Of course, the obvious problem with this idea is that Slashdot has never been about actual hosted content (other than the comments, which are arguably the best part about the site), but rather links to content on other servers. But it has become pretty much standard procedure to link to a site with extra cool content every two to three days only to find that the site is completely unable to hang (or all-too-able to "hang", if you know what I mean). Mirrors often pop up on their own, which is great, but I always wonder why Slashdot doesn't just mirror the extra cool content anyway (I would imagine we can all guess what kind of content qualifies for pre-mirroring... super-cool pictures of the Sun, for example).
The other issue is one of advance notice, which has already been mentioned in this story's comments. I realize that some information is timely and advance notice is not always possible, but the sun's not going anywhere and there could be advanced notification workflow built into the story approval process (ugh, I said "workflow" and "process" in the same sentence). I would suggest that a "site contact" e-mail address or maybe even a phone number be included with story submissions. The "author" (I've never understood why they're called authors when generally they are administrators or approvers only) could then determine in their best judgement whether they think the site is likely to withstand a good slashdotting and, if not, they can have an e-mail message sent to the contact address, which will advise them of the impending slashdotting and give them some options:
I realize this complicates the process, but Slashdot is no doubt aware of it's impact on sites that it links to, and an otherwise good site that gets killed by a terribly unusual load could be made to look like it's run by incompetents, even if it's in perfectly good hands. I wonder how many sites were actually negatively affected by the Slashdot effect, in either the short or the long term.
So that's my two cents.
Hmm (Score:2)
Re:Hmm (Score:2)
How is that contrast interesting again?
do it yourself (Score:4, Informative)
I actually do this sometimes for a whole class of students, and for that I need a big, bright image they can all see, so I use the full aperture of my 8-inch scope. You just have to be careful to limit how long you have it pointed at the sun, because the heat can destroy your eyepiece (melts the glue).
Images from The Sun? (Score:2)
OH NO!!!! (Score:5, Funny)
If only we had known this before, maybe we could have done something about it!
11:15) Restate my assumptions (Score:3, Funny)
Is there a better song written about our Sun? (Score:2)
by They Might Be Giants
The sun is a mass of incandescent gas
A gigantic nuclear furnace
Where hydrogen is built into helium
At a temperature of millions of degrees
Yo ho, it's hot, the sun is not
A place where we could live
But here on Earth there'd be no life
Without the light it gives
We need its light
We need its heat
We need its energy
Without the sun, without a doubt
There'd be no you and me
The sun is a mass of incandescent gas
A gigantic nuclear furnace
Where hydrogen is built into helium
At a temperature of millions of degrees
The sun is hot
It is so hot that everything on it is a gas: iron, copper, aluminum, and many others.
The sun is large
If the sun were hollow, a million Earths could fit inside. And yet, the sun is only a middle-sized star.
The sun is far away
About 93 million miles away, and that's why it looks so small.
And even when it's out of sight
The sun shines night and day
The sun gives heat
The sun gives light
The sunlight that we see
The sunlight comes from our own sun's
Atomic energy
Scientists have found that the sun is a huge atom-smashing machine. The heat and light of the sun come from the nuclear reactions of hydrogen, carbon, nitrogen, and helium.
The sun is a mass of incandescent gas
A gigantic nuclear furnace
Where hydrogen is built into helium
At a temperature of millions of degrees
I found it! (Score:2)
Latency (Score:2)
Canal (Score:2)
Sometimes the oldest jokes... (Score:3, Funny)
Re:Thanks michael (Score:2)
Err... Oops
Unwarranted (Score:3, Interesting)
Seriously they chose to put large size images linked from a press release - I mean they're not even deep links, nor is this one near the bottom of the page. Its probably one of the most likely links everyone will click on if they read the story. Its linked from a press release they expect this too be read, its not like we slashdotted a tiny departmental server.
Does moving it from a 2 click (slashdot story - press release image - gif) to 1 click[1] (slashdot story) really justify a personal broadside against the editorial integerity of one the slashdot team?
Comment on the fact that maybe they should be warned so they remove the high res links until the slashdotting is over, maybe comment on the poor web design approach of the academic team involved, any number of these are valid responses to this story.
Your response adds nothing to the story, nor is what I would expect from someone (judging by you name and email) who is experienced at proffesionally critiquing and assess others work in thier career. Or do peer reviews in Academia these days descend to personal attacks, unwarranted sarcasm and flamewars too?
It seems a strange contrast to your statement about stupidity on the site, did you mean the content of the site or the quality and relevance of the posts on it?
[1]1-Click is of course patented by Amazon, so we must be careful...
Re:Wow (Score:3, Funny)
The web server seem to be running "hot" as well.
Re:Where is the 1600x1200 version? (Score:3, Informative)
whoops