Viewing archive of Thursday, 24 April 2003
Solar activity report
Any mentioned solar flare in this report has a scaling factor applied by the Space Weather Prediction Center (SWPC). Because of the SWPC scaling factor, solar flares are reported as 42% smaller than for the science quality data. The scaling factor has been removed from our archived solar flare data to reflect the true physical units.
Report of Solar-Geophysical Activity 2003 Apr 24 2200 UTCPrepared by the NOAA © SWPC and processed by SpaceWeatherLive.com
Joint USAF/NOAA Report of Solar and Geophysical Activity
SDF Number 114 Issued at 2200Z on 24 Apr 2003IA. Analysis of Solar Active Regions and Activity from 23-2100Z to 24-2100Z Solar activity was at moderate levels this period.
Region 338 (N18W45) produced an M3/1n at 24/1253Z with associated
Type II (830 km/s) and Type IV radio sweeps. A partial halo CME was
also detected on LASCO imagery. Region 339 (N16,L=337) was active
during the period, producing several C-class flares as it crossed
the west limb, the largest being a C8 flare at 24/1553Z. No
significant changes were observed in the remaining active regions.
New Regions 344 (N16E39), 345 (S17E74), and 346 (N16E74) were
numbered today.
IB. Solar Activity Forecast
Solar activity is expected to be at
moderate levels. Region 338 may produce futher M-class flares.
IIA. Geophysical Activity Summary 23-2100Z to 24-2100Z
The geomagnetic field was at unsettled to active levels with isolated
minor storm periods at high latitudes. Elevated solar wind speeds
up to near 600 km/s are responsible for the disturbed periods. The
greater than 2 MeV electrons at geosynchronous orbit reached high
levels today.
IIB. Geophysical Activity Forecast
The geomagnetic field is
expected to be at unsettled to minor storm levels. High speed
coronal hole flow may be enhanced by transient flow over the next
three days. Weak CME impact from an M5 flare on April 23 are
possible on days one and two. A CME impact produced by today's M3
flare may arrive on day three.
III. Event Probabilities 25 Apr to 27 Apr
| Class M | 40% | 40% | 30% |
| Class X | 05% | 05% | 05% |
| Proton | 05% | 05% | 05% |
| PCAF | green | ||
IV. Penticton 10.7 cm Flux
Observed 24 Apr 128 Predicted 25 Apr-27 Apr 130/135/135 90 Day Mean 24 Apr 125
V. Geomagnetic A Indices
Observed Afr/Ap 23 Apr 013/018 Estimated Afr/Ap 24 Apr 020/023 Predicted Afr/Ap 25 Apr-27 Apr 020/020-020/025-020/025
VI. Geomagnetic Activity Probabilities 25 Apr to 27 Apr
| A. Middle Latitudes | |||
|---|---|---|---|
| Active | 30% | 30% | 30% |
| Minor storm | 30% | 20% | 20% |
| Major-severe storm | 10% | 10% | 05% |
| B. High Latitudes | |||
|---|---|---|---|
| Active | 50% | 40% | 40% |
| Minor storm | 35% | 35% | 35% |
| Major-severe storm | 15% | 15% | 15% |
Latest news
Monday, 22 April 2024
Lot's of sunspots! Big chance for major flare activity?
Saturday, 23 March 2024
X1.1 solar flare with earth-directed CME
Wednesday, 20 March 2024
Sunspot region 3615, G1 watch
Latest forum messages
What are these long and thin eruptions? 1AR 3637, 3638, 3643 89Unproven theories 341Space Weather Memes 338Filaments and prominences 55
More topicsSupport SpaceWeatherLive.com!
A lot of people come to SpaceWeatherLive to follow the Sun's activity or if there is aurora to be seen, but with more traffic comes higher server costs. Consider a donation if you enjoy SpaceWeatherLive so we can keep the website online!
Space weather facts
| Last X-flare | 2024/03/28 | X1.1 |
| Last M-flare | 2024/04/25 | M1.0 |
| Last geomagnetic storm | 2024/04/19 | Kp7 (G3) |
| Spotless days | |
|---|---|
| Last spotless day | 2022/06/08 |
| Monthly mean Sunspot Number | |
|---|---|
| March 2024 | 104.9 -19.8 |
| Last 30 days | 133.9 +26.6 |