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10 Years of SOHO - Nasa

10 Years of SOHO - Nasa

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<strong>SOHO</strong>dynamics <strong>of</strong> Earth’s upper atmosphere.Water vapour and ozone are especiallysensitive to changes in the Sun’s UVoutput. Fortunately, Earth’s atmosphereprotects us from this harmful radiation.This also means that we have to leaveEarth’s atmosphere behind and observethe Sun from space.<strong>SOHO</strong>’s Extreme ultraviolet ImagingTelescope (EIT) provides us with stunningimages <strong>of</strong> the Sun’s corona, showingdelicate coronal loops, bright flares andintriguing coronal holes. EIT and the UVspectrometers SUMER and CDS show usthat the outer solar atmosphere isextremely dynamic and changing, and thatplasma flows play an extremely importantrole.Gone With the Solar WindThe solar wind is a stream <strong>of</strong> mainlyelectrons and protons flowing from theUsing advanced analysis techniques, <strong>SOHO</strong>/MDI can reveal the temperature and flow structure beneath sunspotsJust a little over 4 years after the launch<strong>of</strong> <strong>SOHO</strong>, scientists published anastonishing result: the first successfulholographic reconstruction <strong>of</strong> features onthe far side <strong>of</strong> the Sun. An active regionon the far side reveals itself because itsstrong magnetic fields speed up the soundwaves. The difference becomes evidentwhen sound waves shuttling back andforth fall out <strong>of</strong> step with one another. Inthe meantime, the astonishing has becomeroutine, and MDI <strong>of</strong>fers daily far-sideimages online, at http://soi.stanford.edu/data/full_farside/.Violent solar activity occasionallydisrupts satellites, radio communicationsand power systems. Advancewarning <strong>of</strong> magnetic storms brewing onthe far side that could rotate with theSun and threaten Earth is therefore <strong>of</strong>vital importance for space weatherforecasting.The Sun’s Dynamic CoronaThe outer atmosphere <strong>of</strong> the Sun, thecorona, has a typical temperature <strong>of</strong> about1 million K and emits light mainly in theultraviolet (UV) part <strong>of</strong> the spectrum. It isthis radiation from the Sun’s hot coronathat controls the composition andHolographically reconstructed side view <strong>of</strong> the Sun showing thetwo large active regions <strong>10</strong>486 and <strong>10</strong>488 as they rotate fromthe far side (left) to the hemisphere visible from Earth (right).During the previous rotation, these two active regions were thesource <strong>of</strong> the powerful ‘Halloween’ storms in 2003, whichincluded the largest ever recorded X-ray flarewww.esa.int esa bulletin 126 - may 2006 27

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