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The Sun Now!
Images of the sun updated several times a day,
http://www.esa.int/global_imgs/spacer.gifhttp://www.esa.int/global_imgs/spacer.gifhttp://www.esa.int/global_imgs/spacer.gifhttp://www.esa.int/global_imgs/spacer.gif http://www.esa.int/global_imgs/print_it.gifThe Sun now http://sohowww.nascom.nasa.gov/data/...nt/eit_304.jpg http://projectavalon.net/forum/pictu...pictureid=5382 Image from the Extreme ultraviolet Imaging Telescope (EIT) These SOHO images are automatically updated throughout the day. If the images you see do not show today's date please refresh your page. CCD Bake-out If the image above shows 'CCD BAKEOUT', then this means EIT images are temporarily unavailable. In this case, there is nothing wrong with SOHO's EIT instrument. It is routinely taken offline every three months or so for a procedure known as 'bakeout' in order to maintain the performance of the instrument. The images will resume within 2-3 weeks. The Sun's hot atmosphere today See the bright twisted clouds of hot gas, revealing storminess, and the dark, calm regions called 'coronal holes'. These images, obtained with invisible ultraviolet light, give the scientists their routine weather maps of the Sun. Occasionally a solar flare appears, as a small, intensely bright flash. Different colours denote various ultraviolet wavelengths, each emanating from gas at a particular temperature - orange, 80 000 degrees, blue 1 000 000 degrees, green 1 500 000 degrees and yellow 2 500 000 degrees. http://www.esa.int/esaCP/ASE08Y9KOYC_Protecting_0.html |
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Fascinating, Dan, thanks!
alys |
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There's alot more pictures at this link from ESA http://sohowww.nascom.nasa.gov/gallery/top10/
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Here's another one with an Earth inset to show size of the CME
http://projectavalon.net/forum/pictu...pictureid=5388 |
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A sun spot 13 times larger than the surface of the Earth
http://projectavalon.net/forum/pictu...pictureid=5389 |
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I like this site-every day you get a different astronomical upload-there are archives also that go back years.Some interesting shots.
http://apod.nasa.gov/apod/archivepix.html Astronomical picture of the day website. |
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Thanks A, very cool link with great pictures!, I'll remember that one.
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I was quite impressed with the solar flare shot you posted above-i've seen many but not quite as striking as that.
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go to the link in post #3 and there's some more pics!
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Here's a cool picture of the 11 year solar cycle, each picture was taken by the SOHO Observatory and shows what the minimum and maximum solar activity years were. The next maximum solar activity year should fall around 2012, hmmm imagine that.
The Solar and Heliospheric Observatory (SOHO) celebrates its 12th launch anniversary on December 2. In late 1996, shortly after its launch, SOHO was able to observe the last minimum of the roughly 11-year activity cycle of the Sun. The minimum was followed by a rapid rise in solar activity, peaking 2001 and 2002. Activity levels have slowly declined since then, but we haven't reached solar minimum yet, despite passing 11.1 years since the last minimum — the average length of a solar cycle. In fact, the sunspot cycles measured since the mid-18th century vary in length from 9.0 to 13.5 years, and while a team of experts assembled by NOAA, NASA, and ISES has attempted to predict when the next solar minimum will be, we won't really know until we get there. The experts, in fact, were sharply divided about the time of the next minimum and the intensity of the next maximum, which should arrive about 2012 or 2013 http://www.projectavalon.net/forum/p...pictureid=5450 |
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This is a picture of one of the largest solar flares on record,
Solar flares are large explosions on the Sun's surface caused by a sudden release of magnetic energy. They are known to cause local short-lived oscillations traveling away from the explosion like water rings. This means that the flares drive global oscillations in the Sun in the same way that the entire Earth is set ringing for several weeks after a major earthquake such as the 2004 December Sumatra-Andaman one. http://www.projectavalon.net/forum/p...pictureid=5451 |
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SOHO TOP 30
http://sohowww.nascom.nasa.gov/galle...eC3_proton.jpg The "Bastille Day" particle storm and Earth-directed CME as seen by LASCO C3. More about this http://sohowww.nascom.nasa.gov/galle...lleEIT_195.jpg The "Bastille Day" flare as seen by EIT in the 195 Å emission line. More about this http://sohowww.nascom.nasa.gov/galle...gspot_crop.jpg A sunspot thirteen times larger than the surface of the Earth. More about this http://sohowww.nascom.nasa.gov/galle...lueEIT171A.jpg This EIT 171 Å image shows emission from ionised iron at about 1 million degrees C, revealing diffuse corona and magnetic loops. http://sohowww.nascom.nasa.gov/galle...T_Nov8_00A.jpg An impressive double set of CMEs observed by LASCO C2, with an EIT 304 Å inset in the middle. http://sohowww.nascom.nasa.gov/galle...c2fireball.jpg This fiery Coronal Mass Ejection (CME) shows stunning details in the ejected material. More about this http://sohowww.nascom.nasa.gov/galle...Nov00blast.jpg This spectacular Coronal Mass Ejection observed by LASCO C2 was interpreted as "Happy Birthday Fireworks" for the 5th anniversary of SOHO's launch. More about this http://sohowww.nascom.nasa.gov/galle.../C2seq_of3.jpg A sequence of LASCO C2 images showing the evolution of a Coronal Mass Ejection over a time span of about an hour http://sohowww.nascom.nasa.gov/galle...stNov26_01.jpg A Coronal Mass Ejection (CME) observed by LASCO C3 http://sohowww.nascom.nasa.gov/galle...3bulb_crop.jpg This "lightbulb" Coronal Mass Ejection (CME) shows the classical parts of a CME: leading edge, void, and core. More about this http://sohowww.nascom.nasa.gov/galle...3series_02.jpg An Earth-directed Coronal Mass Ejection (CME) seen by LASCO C3. http://sohowww.nascom.nasa.gov/galle...t171_loops.jpg This EIT 171 Å image shows a wide variety of loops and active regions (lighter areas on the surface) http://sohowww.nascom.nasa.gov/galle...5loop_serA.jpg This EIT 195 Å series shows evolving loops stretched out above the edge of the Sun http://sohowww.nascom.nasa.gov/galle...EIT5colorA.jpg An EIT 304 Å image showing an unusual collection of prominences http://sohowww.nascom.nasa.gov/galle...omposMercA.jpg These EIT composite images show the passage of Mercury across EIT's field-of-view during the transit on 7 May 2003. More about this http://sohowww.nascom.nasa.gov/galle...t_MDIcompA.jpg This combination of an EIT 195 Å image and a computed cutaway model of the Sun's interior shows "peculiarities" in the sound speed compared with theoretical models. More about this http://sohowww.nascom.nasa.gov/galle...0/EITplume.jpg A particularly beautiful erupting prominence seen by EIT in 304 Å emission http://sohowww.nascom.nasa.gov/galle.../EITquadsA.jpg An "EIT colour wheel", showing images in the four filters of EIT. Clockwise from upper left: 171 Å, 304 Å, 284 Å, 195 Å. http://sohowww.nascom.nasa.gov/galle...bopp_shadA.jpg Comet Hale-Bopp and its shadow - cast on the diffuse material flowing into the solar system from the intergalactic wind. More about this http://sohowww.nascom.nasa.gov/galle...c2blasred2.jpg This unusual and clearly helical Coronal Mass Ejection (CME) was observed by LASCO C2 http://sohowww.nascom.nasa.gov/galle...co_planets.jpg This image shows no less than four planets, the constellation Pleiades, and a halo Coronal Mass Ejection (CME). More about this http://sohowww.nascom.nasa.gov/galle...0/mdi_comp.jpg This MDI composite shows the passage of Mercury across the solar disk during the transit on 7 May 2003. More about this http://sohowww.nascom.nasa.gov/galle...n304_earth.jpg A closeup of an erupting Coronal Mass Ejection (CME) with Earth inset at the approximate scale of the image. http://sohowww.nascom.nasa.gov/galle...10/NEAT_c3.jpg Our most breathtaking shots of a comet featured Comet NEAT (C/2002 V1) in the LASCO C3 field-of-view. More about this http://sohowww.nascom.nasa.gov/galle...spotmdiG_b.jpg Using advanced analysis techniques, SOHO's MDI instrument can reveal the temperature and flow structure beneath sunspots. More about this,and yet more about this http://sohowww.nascom.nasa.gov/galle...SuperpromA.jpg This magnificent erupting prominence was captured by EIT in 304 Å emission. More about this http://sohowww.nascom.nasa.gov/galle...0/TRICOLOR.jpg Composite image with three EIT wavelengths (171 Å, 195 Å and 284 Å) combined to show solar features unique to each wavelength. http://sohowww.nascom.nasa.gov/galle...omp_EIT195.jpg These three images show the incredible changes in the Sun's corona from near solar minimum to near solar maximum. http://sohowww.nascom.nasa.gov/galle.../twinpromA.jpg Two large eruptive prominences captured by EIT in 304 Å emission. More about this http://sohowww.nascom.nasa.gov/galle...XMAScometA.jpg This LASCO C2 image from 23 December 1996 shows the "Christmas Comet" (Comet SOHO-6) streaking towards the Sun </SPAN> |
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Spotless Sun: Blankest Year of the Space Age
10.06.08 Astronomers who count sunspots have announced that 2008 is now the "blankest year" of the Space Age. As of Sept. 27, 2008, the sun had been blank, i.e., had no visible sunspots, on 200 days of the year. To find a year with more blank suns, you have to go back to 1954, three years before the launch of Sputnik, when the sun was blank 241 times. "Sunspot counts are at a 50-year low," says solar physicist David Hathaway of the NASA Marshall Space Flight Center. "We're experiencing a deep minimum of the solar cycle." A spotless day looks like this (below left): http://www.nasa.gov/images/content/2..._2shot_452.jpg Left: A photo of the sun taken Sept. 27, 2008. The face of the sun is "blank," i.e., completely unmarked by spots. Right: The sun on Sept. 27, 2001. The sun's face is peppered with colossal sunspots, all crackling with solar flares. Credit: ESA/NASA Solar and Heliospheric Observatory (SOHO) http://www.nasa.gov/images/content/2...hs_226x249.jpg Top: A histogram showing the blankest years of the last half-century. The vertical axis is a count of spotless days in each year. The bar for 2008, which was updated on Sept. 27th, is still growing. Bottom: A histogram showing the blankest years of the last century. As in the above histogram, the bar for 2008 is still growing. |
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Oh that wonderful Sun!! Lets hope that when 2012 comes it doesn't bake us with cosmic ray particles and cosmic dust! A nice gentle massage will do instead...
__________________________________________________ __ The End is the Beginning and the Beginning is the End...(Nothing New Under The Sun) |
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Nice Sun photos Dan http://www.clicksmilies.com/s1106/na...smiley-015.gif
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Coronal Holes: http://www.spaceweather.com/images/spacer.gifhttp://www.spaceweather.com/images20...e_soho_163.gif http://www.spaceweather.com/images/spacer.gifA solar wind stream flowing from the indicated coronal hole should reach Earth on or about Jan. 25th or 26th. Credit: SOHO Extreme UV Telescope
Geomagnetic Storms: Probabilities for significant disturbances in Earth's magnetic field are given for three activity levels: active, minor storm, severe storm Updated at: 2009 Jan 22 2201 UTC Mid-latitudes 0-24 hr 24-48 hr ACTIVE 01 % 01 % MINOR 01 % 01 % SEVERE 01 % 01 % High latitudes 0-24 hr 24-48 hr ACTIVE 05 % 05 % MINOR 01 % 01 % SEVERE 01 % 01 % |
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Solar Storms</B>
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Aurora</B>
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What are the black squares? Peace Iain |
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square UFO's LOL!, no not really, just a blotch in the camera image, every once in awhile you'll see a defect of some sort. Oh I see they're gone now, they must've corrected it! I guess they come and go.
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Forecast
The geomagnetic field is expected to be quiet to active on February 5 due to effects from CH358 and quiet on February 6-11. Active solar regions (Recent map) http://www.solen.info/solar/images/AR_CH_20090204.jpg Data for all numbered solar regions according to the Solar Region Summary provided by NOAA/SWPC. Comments are my own, as is the STAR spot count (spots observed at or inside a few hours before midnight) and data for regions not numbered by SWPC or where SWPC has observed no spots. SWPC active region numbers in the table below and in the active region map above are the historic SWPC/USAF numbers. A small recurrent coronal hole (CH358) in the southern hemisphere was in an Earth facing position on January 30-31. http://www.solen.info/solar/images/e...0000_coron.jpg Processed SOHO/EIT 195 image at 00:00 UTC on February 5. The darkest areas on the solar disk are likely coronal holes |
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http://www.esa.int/global_imgs/spacer.gifhttp://www.esa.int/images/Clusters_Earth2_S.jpg
The Cluster constellation Cluster — the Sun-Earth connection in focus The Cluster constellation was launched in summer 2000 and started operating in early 2001. Since then, this four-satellite mission is performing the first and best ever stereo investigation of the Earth’s magnetosphere — the magnetic bubble surrounding our planet. Thanks to Cluster, scientists have reached an unprecedented understanding of the way solar activity affects the near-Earth environment. Cluster has provided the first 3D observation of magnetic reconnection in space — a phenomenon that reconfigures the magnetic field and releases high amounts of energy. Cluster pioneered measurements of electric currents in space, revealed the nature of black aurorae, and discovered that plasma — a gas of charged particles surrounding Earth — makes ‘waves’. The Cluster mission has been extended twice in the past, up to June 2009. The new extension will make it possible to study the auroral regions above Earth’s poles and widen the investigations of the magnetosphere — its inner region in particular. |
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This is a great post Dan, I've never seen pictures of the sun like that. Unfortunately I'm ignorant to what it means. I may take an astronomy class this summer, looks like I know who can help me with my homework. :wink2:
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Yeah Luana those are all real pictures from the ESA (European Space Agency), and basically it tells all about sun spots, solar flares, and CME's ( Coronal Mass Ejections), also that we're in a lull now for solar activity and the next maximum solar activity period just happens to fall around 2012, hmmm imagine that!
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:original: Solar Observing Glossary
CHROMOSPHERIC NETWORK An constant patchy network of long thin sinuous chains of tiny low contrast brighter points called Filigree (also found in plages) extending over much of the solar disk in H-Alpha. These points, or "network elements", often have darker spicules or short fibrils sticking out of, or running past them (part of the fine disk detail known as the Dark Mottles), making the actual network harder to see. ELLERMAN BOMBS Bright transient pin-points of light (usually last less than 5 minutes), most often found in Emerging Flux Regions or on the edges of sunspots where the magnetic field is breaking the surface. They are best seen in the wings of H-alpha (nearly 5 Angstroms wide). EMERGING FLUX REGION (EFR) A magnetic area on the sun where "flux tube" is surfacing on the disk, eventually producing a bipolar sunspot group. In H-alpha, EFRs usually appear as a small oval area of bright plage (typically about 7000 km across) often containing a series of short-lived narrow fibrils (Arch Filament System (AFS)) running roughly from one end of the dipole to the other. Each pole of an EFR is often marked by pores or small developing sunspots. Surges or even small solar flares can sometimes occur in EFRs. EPHEMERAL REGIONS (ER's) Small magnetic dipoles with lifetimes of about a day which contain no sunspots. Ephemeral regions can develop anywhere on the sun, but are more common at mid and lower solar latitudes. They appear as small brighter elements in the chromospheric network but are fainter than active region plage. They also can occasionally produce small surges or sub flares. FACULAE Patchy white light blotches in the photosphere (not visible in H-alpha), usually seen mainly towards the limb due to limb darkening. Faculae are most often found near active regions or where one is about to form, and can last well after the sunspots in the active region have decayed (best seen in blue light). FIBRILS Small fine filament-like darker features which tend to run along magnetic field lines. Often, they are connected to or part of the structure of larger filaments, curving into or running along the filament's main axis. FIELD TRANSITION ARCHES (FTA) Filament-like fibrils which cross the polarity inversion line (a line marking the halfway point between two opposite polarity areas) of a bipolar magnetic region. Unlike AFS fibrils, they show little or no Doppler shifts and tend to be rather thin and not very dark. FTA tend to arch directly between localized areas of opposite magnetic polarity, and often mark magnetically stable regions. FILAMENTS Prominences seen against the face of the sun, appearing as long narrow dark streamers or diffuse complex dark areas in H-alpha light. Filaments often mark areas of magnetic shearing (see Prominences). GRANULATION Tiny convective cell structures visible in white light ("rice grains"), best seen in apertures over three inches, and in green light. Each cell consists of a brighter polygonal area of hot rising gas typically about 1100 km across, and a cooler edge or "channel" of descending gas about 230 km wide. MORETON WAVE A shock wave seen on the chromosphere that is occasionally seen expanding outward from large impulsive solar flares, moving over the surface at about 1000 km/sec. It usually appears as a slowly moving diffuse arc of brightening in the centerline of H-alpha, or as a faint diffuse slightly darker arc in the blue wing. PROMINENCES H-Alpha emission features that resemble "flames" projecting beyond the edge of the sun, consisting of complex clouds or streamers of gas above or in the chromosphere. They generally come in two broad classes: Active (limb flares, surges, sprays, loops), and Quiescent (Quiet Region Filaments, Active Region Filaments). PLAGE Patchy brightenings on the solar disk seen in H-Alpha light, usually found in or near active regions, which can last for several days. Plage is irregular in shape and variable in brightness, marking areas of nearly vertical emerging or reconnecting magnetic field lines (from French word for "beach" with the "a" being a short one). PORES Tiny darker spots under 2500 km in size, often having fairly short lifetimes. Pores occasionally form where several granulation channels meet and can sometimes precede the development of sunspots. RECONNECTION A realignment of magnetic fields, where an area of one magnetic polarity breaks earlier links, and connects with the nearest region of opposite polarity. On the sun, this often happens when a new magnetic dipole emerges near another pre-existing one. For example, if the north pole of the new dipole emerges close to the south pole of the old dipole, the lines of force may reconnect these two nearby poles configuring them as a new lower energy dipole and releasing energy, often in the form of plage brightening or a solar flare. SOLAR FLARE Extremely bright moderate to large transient emission feature lasting from a few minutes to over four hours. Flares are a rapid and violent release of energy in the chromosphere due to extreme magnetic field stress and can occasionally result in material leaving the sun in the form of a Coronal Mass Ejection (CME). SPICULES Small jets of gas under 10,000 km long, usually seen as a mass of tiny brighter spike-like features at the limb or as tiny darker spikes coming out of network elements, but are not usually seen over bright plage. SPRAY A transient prominence formed by the explosion of pre-flare elevated material which sends debris flying off in many directions. Usually produced only by the most violent flares, as overlying filaments are blown away. SUNSPOT Dark long-lived photospheric feature, typically from 2500 to 50,000 km in size. Moderate to large spots usually consist of a darker central region (umbra) and a lighter halo consisting of many short fine fibrils (penumbra). Sunspots have strong concentrated magnetic fields which tend to inhibit energy transfer from below, making them at the center about 2500 degrees K cooler than the photosphere. In the Umbra, the fields tend to be nearly vertical in orientation while in the penumbra, the magnetic fields become more horizontal. SURGE A transient prominence produced by flares or very active regions, appearing as a moderate to large collimated jet of gas rising up from the surface. Surge ejected gas will often fall or draw back onto the sun tending to follow magnetic field lines, while at other times it will rise and disperse, fading from view. "WINGS" OF H-ALPHA Doppler-shifted features of the sun can be viewed at wavelengths slightly off of 6562.8 Angstroms (up to +/- 2 Angstroms). The "blue" wing is a shorter wavelength and the "red" is on the longer side. http://Luminari.fileave.com/sunfeature.jpg |
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Nice, thanks Luminari!
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Astronomers once thought they understood how the Sun worked. A large ball of gas, generating energy by nuclear fusion, it also created a magnetic field enclosing Earth and the other planets in a gigantic magnetic bubble.
This bubble protected us from the dusty cosmic debris that shoots through space beyond the Solar System. But thanks to ESA's solar polewatcher Ulysses, that picture is changing... 11-year switch Ulysses has revealed a complexity to the Sun's magnetic field that astronomers had never imagined. The Sun's magnetic field consists of a north pole, where the field flows out of the Sun and a south pole, where the field re-enters. Usually, these line up, more-or-less, with the rotation axis of the Sun. Every 11 years the Sun reaches a peak of activity that triggers the magnetic poles to exchange places. The reversal was thought to be a rapid process but, thanks to Ulysses, astronomers now know it is gradual and could take as much as seven years to complete. During this slow-motion reversal, the line connecting the poles - known as the magnetic axis - comes close to the Sun's equator and is swept through space like the beam of a light house. Eventually it passes through this region and lines up with the opposite pole. Imagine if this happened on Earth! Compasses would become useless, given that they rely on the fact that Earth's magnetic axis is roughly coincident with its rotation axis, which passes through the North and South geographic Pole. Although it seems surprising, magnetic pole reversals have happened on Earth also. The last time was about 740 000 years ago. After studying magnetic rocks, scientists conclude that field reversals on Earth take place once every 5000 to 50 million years (but are impossible to predict). Reversals on the Sun, however, are almost as regular as clockwork - every 11 years, with its magnetic axis changing position for most of that time. Earth's magnetic field is more stable because it arises in the metal-dominated regions in the deep interior of the planet. The Sun's field, however, comes from a high-temperature, electrified gas called plasma so it is a much more volatile thing. Loops of the magnetic field can burst through the surface of the Sun and when they do, they create the dark patches known as sunspots. Astronomers are still studying the precise reasons behind the Sun's 11-year magnetic flips. However, using Ulysses, they have now shown that, when the Sun's magnetic axis points near its equator, it allows much more cosmic dust to enter the Solar System than normal. What does that mean for us? If there is more dust in the Solar System, more of it will fall on Earth also. Scientists estimate that in the coming years, about 40 000 tonnes of dust could fall on Earth every day. However, most of it will be so small that it will burn up in the atmosphere before reaching the ground. This will certainly increase the number of faint shooting stars during the next 11 years, but fortunately the Earth will not become a dustier place! http://www.esa.int/esaSC/SEMVB3ZO4HD_index_0.html |
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The Earth has a magnetic field with north and south poles. The Earth's magnetic field reaches 36,000 miles into space.
The magnetic field of the Earth is surrounded in a region called the magnetosphere. The magnetosphere prevents most of the particles from the sun, carried in solar wind, from hitting the Earth. Some particles from the solar wind can enters the magnetosphere. The particles that enter from the magnetotail travel toward the Earth and create the auroral oval light shows. The Sun and other planets have magnetospheres, but the Earth has the strongest one of all the rocky planets. The Earth's north and south magnetic poles reverse at irregular intervals of hundreds of thousands of years. The Earth's Magnetic Field http://www.windows.ucar.edu/earth/im...th_magneto.jpg |
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Amazing how quiet and calm the sun is!
To the people interpreting cropcircles as pointing to a massive solar flare in early july (3 weeks away) I must say this look extremely unlikely, near impossible considering the Sun is currently blissed out in peaceful contemplation of itself. |
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All it takes is one, pointed in the right direction :mfr_lol:
alys |
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we saw a couple small spots not long ago up at the observatory through the 14".
still wikked quiet tho. i never got to watch Sol thru a scope before, until a couple weeks ago. if you guys havent gotten to, and ever get the chance.. dont pass it up!! :wub2: |
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I am an avid space and Sol observer. I got tired of going to different sites everyday for the info I wanted to monitor so I put it all together on one page. I think some of you may find it as useful as I do.
http://2012info.ca/EarthWatch/?page_id=1147 |
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I also like how you can see who's visited and where they came from, that is cool huh. Though it says I came from Brisbane even though that is over 2000kms away from my location, I guess it was the softwares closest point of reference. Im going to buy a CORONADO at some point so I can view the sun myself, I think when we get near solar maximum it will be quite a show. Have you used one of those? Is there other better options in the way of filter-lenses to fit on my meade telescope I will have? |
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Awsome site ! I'll use it ans share it with others . Kindness mudra |
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With respect to the perceived threats from Nibiru, World War 3, the NWO, Galactic Alignments etc. The real threat and one I firmly believe is going to decimate (not destroy) life on Earth in the next few years comes from our life source. Here's the pitch, the hit comes around or before 2012. :shocked:
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