The Solar and Heliospheric Observatory (SOHO):
Exploring the Sun

**Please note: This ipcvision page has been designed to be viewed with a black background**
O holy virgin! clad in purest white,
Unlock heavn's golden gates, and issue forth;
Awake the dawn that sleeps in heaven; let light
Rise from the chambers of the east, and bring
The honied dew that cometh on waking day.

William Blake


SOHO Spacecraft

SOHO Spacecraft (courtesy ESA)


Return to the top of IPCVision Homepage

The SOHO Mission

Basic Information:

SOHO is a joint space mission of the European Space Agency (ESA) and NASA, and is designed to study the internal structure of the Sun, its extensive outer atmosphere and the origin of the solar wind, the stream of highly ionized gas that blows continuously through the solar system.

By operating around a point 1.5 million kms sunward of the Earth, at the point where the Sun's gravity balances the Earth's, SOHO provides scientists with their first long term uninterrupted view of Sun.

There are five instruments onboard SOHO to observe the Sun:
  • EIT solar flare image, Jan2000 - click for enlargement- size=21K EIT (Extreme Ultraviolet Imaging Telescope) - This highlights gas at between 80,000 to 2 million degrees and provides daily weather maps of the Sun.

  • CDS and EIT composite eruption analysis - click for enlargement- size=18K CDS (Coronal Diagnostics Spectrometer) - Scans small areas of the Sun, measuring intensities over a wide range of sharply defined wavelengths - has proved valuable for deducing temperatures and densities of the gas.

  • Example of SUMER Flare analysis - click for enlargement- size=27K SUMER (Solar Ultraviolet Measurements of Emitted Radiation) - Same process as CDS, but excels in measuring velocities of gas streams and detecting previously unknown ultraviolet emissions.

  • New comet discovery, Feb 2001 - click for enlargement- size=17K UVCS (Ultraviolet Coronagraph Spectrometer) - this masks out the solar disk itself, allowing analysis of ultraviolet emissions from the corona, from 350,000 to 14 million kms above the visible surface. It gauges the energy of atoms leaving the Sun in the solar wind.

  • LASCO C2 Coronal Mass Ejection 14.Jan.01 - click for enlargement, size=12K LASCO (Large Angle Spectrometric Coronagraph) - This observes visible light from the corona using three masked telescopes, covering a range of 140,000 kms to 20 million kms from the Sun's surface. Provides spectacular images of Coronal Mass Ejections (CMEs).



Links to more Comprehensive Information:


click here to return to Top of this Page ------ click here to return to Previous Page ------ click here to return to Contents list on IPCVision Home Page ------ click here to send me an E-Mail

- Please E-Mail any comments -
straight coloured line
< Site design by IPCVision; all non-acknowledged material © of IPCVision; All Rights Reserved >
** Page last updated Dec'07 **