News on the Sun
- The Sun has shifted ppolarity
- Huge tornadoes discovered on the Sun
- The Sun got bigger
- Last solar minimum was unusual
- The sound of a solar storm
- Earth’s magnetic field provides vital protection
- The Sun's magnetosphere
- IBEX detects "alien" particles
- Cold Hydrogen gasses recycles sunspots
- Thin layers of cosmic chok-waves
- The Solar cycles
- Comet hits the Sun
- Solar eruption causes massive Aurora's
- Our Solarsystem had a fifth Gas-giant planet
- 6 Coronal Mass Ejections in 24hours!
- New Characteristics of Solar flares discovered
- 40 year old Mariner 5 solar wind problem solved
- Solar wind traced in 3D from Sun to Earth
- Detection of emerging sunspot regions
- SDO Spots Extra Energy in the Sun's Corona
- New images of Vesta from DAWN
- New way to measure magnetism around the Sun
- Solar eruption "blew half the sun to pieces"
- Sun and planets constructed differently
- Solar storm reaches Earth today
|
Massive solar ejection
Wednesday, 08 December 2010 11:58
|
|
| Solar system - The Sun |
|
So you think the Sun i quiet these days? This image from the SOHO shows the eruption of a coronal mass ejection (CME) an energized bubble of plasma from the Sun's atmosphere in the general direction of Earth on August 7, 2010. The white circle in the middle shows the diameter and placement of the Sun behind the disk of the coronagraph (smooth gray circle), which creates an artificial eclipse to reveal the Sun's faint atmosphere. The white and black curves on the left show the halo effect of the plasma bubble as it pinches off from the eastern limb.
Unlike other SOHO images that show the Sun is bright reds, greens, and other artificial colors, this is a “difference image”; that is, it is a composite of two images where the earlier image is subtracted from a later one. The technique allows solar physicists to see the propagation of the plasma cloud across space, with the brightest whites showing areas of the highest density. The image is taken by the Large-Angle Spectrometric Coronagraph (LASCO) on SOHO CMEs carry energized particles across the solar system, and when they cross paths with Earth, the result can be auroras (northern and southern lights), charging of the Van Allen radiation belts, and disturbances in the ionosphere, a layer of our atmosphere that is critical for the relay of radio signals. These space weather events can distort satellite communications and earth-based radio transmissions, cause satellite parts to fail, and create surges of current in electrical power lines—and sometimes blackouts. Before SOHO and the International Solar Terrestrial Physics program of the 1990s, scientists and engineers couldn’t do much to prepare for space weather. But by providing a full-time view of solar activity, SOHO afforded earthlings as much as two or three days notice of an impending storm. Though its instruments have aged and newer satellites now have a better view, SOHO is still building a long-term record of solar observations. Image courtesy of the Solar and Heliospheric Observatory / LASCO consortium. Caption by Michael Carlowicz. |





