SOLAR 001
A collection of huge clouds of relatively cool dense plasma seen suspended in the hot sun, thin corona. At a certain moment in the cloud can burst, regardless of the solar atmosphere. emission spectral line shows upper chromosphere at a temperature of 60,000 degrees K (over 100rb degrees F). Every part of this image traces magnetic field structure. section The hottest areas appear almost white, while the darker red areas indicate the cooler temperatures. (Courtesy of SOHO / EIT consortium). 
Close up detail of the magnetic structur above the surface of the sun, seen from theH-alpha wavelength on August 22, 2003
SOLAR 003 NASA's STEREO satellite captured the first images collision between the "storm" the sun, which called a coronal mass ejection (CME), and the comet on 4 April 2007. this tabarakan cause the release of the plasma tail of comet. Comet is the rest of solar systemformation billions of years ago. comet is usually located in the cold, distant from the solar system,but sometimes the pull of gravity from the planet, another comet or even a star near thecomet was brought into the solar system comet.
SOLAR 004 Images from the sun is active on 24 July 2002 taken near the eastern matahari.bagian highlight is a three-dimensional images of the photosphere if viewed from the angle of this magnitude. structure in the sunspot is darker at the top gambarmenunjukan difference in elevation above the middle of "the dark" of thesunspot. height of this structure has been estimated by Dr. Bruce Lites High Altitude Observatoryof the range between 200 and 450 km. separate small parts of the image size of about 70 km.Terdapat also some light "faculae" as seen from theend of the observation observatory overlooking granules. (Prof. Goran Scharmer / Dr.Mats G. Löfdahl / Institute for Solar Physics of the Royal Swedish Academy of Sciences)
SOLAR 005 Total solar eclipse on 16 February 1980 which was photographed from Palem, India byteam research from the High Altitude Observatory of the National Center for AtmosphericResearch. Photos of the solar corona was taken from a camera system developed by Gordon A.Newkirk, this particular Jr.Alat mangambil corona images in red light, 6400 A. (RhodesCollege, Memphis, Tennessee / High Altitude Observatory (HAO), UniversityCorporation for Atmospheric Research (UCAR))
A collection of huge clouds of relatively cool dense plasma seen suspended in the hot sun, thin corona. At a certain moment in the cloud can burst, regardless of the solar atmosphere. emission spectral line shows upper chromosphere at a temperature of 60,000 degrees K (over 100rb degrees F). Every part of this image traces magnetic field structure. section The hottest areas appear almost white, while the darker red areas indicate the cooler temperatures. (Courtesy of SOHO / EIT consortium).
SOLAR 002
SOLAR 003 NASA's STEREO satellite captured the first images collision between the "storm" the sun, which called a coronal mass ejection (CME), and the comet on 4 April 2007. this tabarakan cause the release of the plasma tail of comet. Comet is the rest of solar systemformation billions of years ago. comet is usually located in the cold, distant from the solar system,but sometimes the pull of gravity from the planet, another comet or even a star near thecomet was brought into the solar system comet.
SOLAR 004 Images from the sun is active on 24 July 2002 taken near the eastern matahari.bagian highlight is a three-dimensional images of the photosphere if viewed from the angle of this magnitude. structure in the sunspot is darker at the top gambarmenunjukan difference in elevation above the middle of "the dark" of thesunspot. height of this structure has been estimated by Dr. Bruce Lites High Altitude Observatoryof the range between 200 and 450 km. separate small parts of the image size of about 70 km.Terdapat also some light "faculae" as seen from theend of the observation observatory overlooking granules. (Prof. Goran Scharmer / Dr.Mats G. Löfdahl / Institute for Solar Physics of the Royal Swedish Academy of Sciences)SOLAR 005 Total solar eclipse on 16 February 1980 which was photographed from Palem, India byteam research from the High Altitude Observatory of the National Center for AtmosphericResearch. Photos of the solar corona was taken from a camera system developed by Gordon A.Newkirk, this particular Jr.Alat mangambil corona images in red light, 6400 A. (RhodesCollege, Memphis, Tennessee / High Altitude Observatory (HAO), UniversityCorporation for Atmospheric Research (UCAR))
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