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The Very Latest SOHO Images - Solar and Heliospheric Observatory NOTICE: SDO HMI Continuum and SDO HMI Magnetogram image outage due to a cooling water line burst in the Joint Science Operations Center (JSOC) at Stanford University on 2024-11-26 Status updates are provided at SDO's JSOC Emergency Resources page
SOHO - Solar and Heliospheric Observatory Above the surface is a region of hot plasma called the corona The corona is about 2 million K (3 6 million degrees F), much hotter than the visible surface, and it is even hotter in a flare Why the atmosphere gets so hot has been a mystery for decades; SOHO's observations are helping to solve this mystery
Latest SOHO Images - Solar and Heliospheric Observatory The SOHO summary data is a collection of daily solar data obtained by different SOHO instruments For non-solar physicists, to learn some of the theory behind Solar observations, please visit our How do we observe the Sun page offered through SOHO Explore, our mission's educational resources
About the SOHO Mission - Solar and Heliospheric Observatory SOHO, the Solar Heliospheric Observatory, is a project of international collaboration between ESA and NASA to study the Sun from its deep core to the outer corona and the solar wind
SOHO Space Weather - Solar and Heliospheric Observatory Windows to the Universe: Space Weather Today Human Impacts of Solar Storms and Space Weather IPS Real-Time Space Weather Status SOHO Halo Alert Reports Solar Terrestrial Activity Report Space Weather Forecast from RWC Lund, Sweden Space Weather Resources from Rice University Northern Lights
SOHO Free Stuff - Solar and Heliospheric Observatory An interactive multimedia exploration of the Sun through the eyes of SOHO The CD covers topics ranging from the history of solar exploration to new scientific results and the Sun's influence on the Earth's environment
SOHO-Newsroom We are scientists from the Solar and Heliospheric Observatory (SOHO) mission, a satellite that's still studying the Sun after 25 years! Ask us anything about SOHO and solar science