SDO solar image - 4500 angstroms - Courtesy of NASA/SDO and the AIA, EVE, and HMI science teams.
satellite
radio propagation
Today's Space Weather
Thursday 27 August
last updated 27/0639 UT
Moderate solar flare activity with GONG H-alpha imagery indicating region 2403 (S16W44) to be the source of the recent M2.3 flare (as of 0544UT). Coronal hole effects likely to influence the solar wind over the next 12-24 hours. Geomagnetic conditions currently at Unsettled to Active levels due to sustained southward Bz during local day. Should Bz remain southward and/or solar wind velocity rises above Moderate levels (Co-rotating Interaction Region followed by Coronal Hole HSSW) Minor to Major Storm periods are possible with Aurora sightings likely from southernmost Australian regions. Short-wave radio fadeouts possible. High-frequency radio communications fair to normal at all latitudes.
What is Space Weather ?

Space weather refers to changes in the space environment, particularly the region between the Earth and Sun. The "solar wind" from the Sun stream past the Earth and is mostly deflected by the Earth's magnetic field, but variations in the solar wind cause changes in the Earth's magnetic field.

solar prominence

Occasionally, a huge release of magnetic energy, called a solar flare, occurs on the Sun. Flares can produce large quantities of x-rays which affect the Earth's atmosphere. They can also accelerate atomic particles (mostly protons) to very high speeds (a substantial fraction of the speed of light!). These high energy particles are dangerous to man and can reach the stratosphere where jetliners fly.

Most aspects of space weather affect us to some extent. The more our society becomes dependent on technology and the more we utilise space, the more we are affected by space weather. Some aspects of space weather are benevolent, and allow activities not otherwise possible such as long range radio communications. Some aspects are benign but fascinating such as the Aurora, and some are malevolent. Like terrestrial weather, it sometimes depends on the situation and the event.

The image below is an artists impression of the solar wind interacting with the Earth's magnetic field.

Solar wind
Collage of images - Power lines, Learmonth Observatory, pipeline, Magnetometer measurements , Aurora at Casey, an Ionogram, and Satellite.
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