Space Weather
Space Weather
Space weather describes changing environmental conditions in near-Earth space. Magnetic fields, radiation, particles and matter, which have been ejected from the Sun, can interact with the Earth’s upper atmosphere and surrounding magnetic field to produce a variety of effects.
Space weather notifications
There are currently no active notifications.
Aurora forecasts
Northern Hemisphere
Significant geomagnetic activity is not expected, with the aurora likely limited to normal background visibility levels.
Southern Hemisphere
Significant geomagnetic activity is not expected, with the aurora likely limited to normal background visibility levels.
Issued at:
Forecast overview
Space Weather Forecast Headline: Moderate class flares expected with a slight chance of X-class (Strong) flares.
Analysis of Space Weather Activity over past 24 hours
Solar Activity: Low, with a peak high Common class flare from a sunspot region in the northwest. A sunspot near the central meridian in the southern hemisphere remains the largest sunspot on the disc with occasional low-level Common-class flare activity. Some slight increase in overall size was observed, but also slight decay in its main trailer spot. Despite its size it maintains a fairly simple magnetic configuration. The sunspot in the northwest, responsible for the strongest flare of the period persisted with a large leader spot and strong magnetic field, but just limited small opposite polarity spots to its east and northeast and a relatively simple magnetic structure. A region in the far northwest was responsible for some low-level Common-class activity and remains moderately complex, however, became increasingly foreshortened in available solar imagery as it approached the western limb. Elsewhere there was some emergence of small sunspot groups, but these were largely inactive.
Disappearing filaments (eruption of lines of the Sun's plasma) in the southeast disc around 19/2300 UTC and 20/0515 UTC were observed, however, no definitive Coronal Mass Ejections (CMEs) were in evidence following either event. Therefore no clear Earth-directed CMEs have been observed.
Solar Wind / Geomagnetic Activity: Ongoing fast winds from a coronal hole were observed. Solar wind speed increased from slightly elevated to become strong, reaching 600-650km/s by the end of the period. Interplanetary Magnetic field, Bt, was Weak to Moderate with the north-south component also Weak to Moderate, with no single orientation (direction) favoured. Geomagnetic activity was Quiet to Active (Kp2-4).
Energetic Particles / Solar Radiation: The count rate of energetic particles (high energy protons) persisted at Background with no Solar Radiation Storms occurring.
Four-Day Space Weather Forecast Summary
Solar Activity: Moderate activity is forecast, with isolated Moderate-class flares expected. There is a slight chance of Strong flares.
Solar Wind / Geomagnetic Activity: There are no CME arrivals expected at Earth, however a glancing impact from the Coronal Mass Ejection (CME) early on 18 Jan cannot be completely ruled out late on Day 1 (20 Jan) or early Day 2 (21 Jan). Otherwise, current strong fast winds from a coronal hole are expected to continue before gradually easing from Day 2 (21 Jan) onward, likely becoming near background by the end of Day 4 (23 Jan). Mainly Quiet to Unsettled geomagnetic activity is expected, with a chance of Active intervals, these most likely on Day 1 and 2 (20 and 21 Jan).
Energetic Particles / Solar Radiation: The count rate of energetic particles (high energy protons) is expected to persist at Background with no Solar Radiation Storms occurring. However, there is a slight chance of this rising in response to any significant flares that occur.
Issued at:
Solar imagery
SDO AIA-193
This channel highlights the outer atmosphere of the Sun - called the corona - as well as hot flare plasma. Hot active regions, solar flares, and coronal mass ejections will appear bright here. The dark areas - called coronal holes - are places where very little radiation is emitted, yet are the main source of solar wind particles.
Issued at:
SDO AIA-304
This channel is especially good at showing areas where cooler dense plumes of plasma (filaments and prominences) are located above the visible surface of the Sun. Many of these features either can't be seen or appear as dark lines in the other channels. The bright areas show places where the plasma has a high density.
Issued at: