PPA Roadmap

[Former PPARC Particle Physics and Astronomy Roadmap]

SOHO
Temperature map of the Sun's corona. Credit: SOHO/EIT (ESA & NASA)
Temperature map of the Sun's corona. Credit: SOHO/EIT (ESA & NASA)

Addressing these questions:
Project Status:
  • In Operation

UK Involvement
Project Web Site:
Related Projects:
The Solar and Heliospheric Observatory (SOHO) is an ESA/NASA mission launched in 1995. The objective of SOHO is improve our understanding of the processes involved in heating the corona, creating coronal mass ejections and accelerating particles in the solar wind.

Scientific Impact

SOHO carries three sets of instruments designed to explore the solar interior using a method known as helioseismology which involves monitoring small vibrations of the Suns surface by exploiting the Doppler Effect (a shift in wavelength of emitted light due to motion) or variations in intensity. The application of a consistent synoptic programme for SOHO has resulted in a dataset which is ideal for solar cycle and long-term variation studies.

Strategic Priority

The mission addresses the two themes of energy flow in the solar system and how the interior of the Sun couples with the solar surface and atmosphere.

Timeliness

The extended ESA/NASA mission runs to December 2009.

Track Record

The UK has unique hardware capabilities as demonstrated by PI participation in all major solar missions, as well as requests from US teams for UK collaborators.

Momentum

The SOHO mission has been extended several times, the nominal end date is 2009 and the mission has been operating for over 10 years. the current end date allows significant overlap between SOHO and Solar-B and STEREO (both with launch dates in 2006) and Solar Dynamic Observatory (SDO) (launch 2008). This provides UK scientists with an outstanding complement of instrumentation for solar research.

UK Involvement

The UK involvement is as PI on the Coronal Diagnostic Spectrometer (CDS) through the CCLRC's Rutherford Appleton Laboratory with the assistance of UCL's Mullard Space Science Laboratory. The CDS is one of the main instruments on SOHO. UK theoreticians played an important role in the design of the Global Oscillations at Low Frequencies (GOLF), Solar Oscillations Investigation (SOI) and the Variability of Irradiance and Gravity Oscillations (VIRGO). The UK Post Launch Support concentrates on CDS operations.

Risk

 



Cost

The UK Post Launch Support cost £5M from launch to April 2005