Lite Forecasting Guide (No Big Movies)


Solar Disk Observations Section

Latest AIA Observations

Below shows the Latest HMI-B image (Top Image), Latest AIA 304Å image (Middle Image), and latest AIA 193Å image (Bottom Image). Data courtesy of the SDO/AIA/HMI mission teams, NASA.

HMIB


AIA_304


AIA_193

CMEs Section

CACTUS

Below shows the latest CME detections, courtesy of the CACTus CME catalog, generated and maintained by the SIDC at the Royal Observatory of Belgium.

Cactus detections

Flare Observations Section

GOES 3 Day Flux

Below shows the latest GOES x-ray flux measurments, courtesy of the GOES mission team, SWPC/NOAA.

Goes 3-day Plot

Latest GOES Flare Data

Below shows the latest GOES x-ray flare detections, courtesy of the GOES mission team, SWPC/NOAA.

Created: 2025 Jun 23 0537 UT
Date: 2025 06 23
#Event Begin Max End Obs Q Type Loc/Frq Particulars Reg#
3090 + 0040 0048 0055 G18 5 XRA 1-8A B9.6 1.0E-03 4118
3090 0052 //// 0056 PAL C RSP 025-152 III/1
3110 0052 //// 0125 LEA C RSP 025-114 VI/2
3100 + 0055 0059 0104 G18 5 XRA 1-8A C1.0 6.2E-04 4113
3110 0125 //// 0126 PAL C RSP 025-139 III/1
3120 + 0209 0217 0225 G18 5 XRA 1-8A C1.3 1.2E-03
3130 0258 //// 0258 LEA C RSP 029-101 III/1
3140 + 0327 0333 0353 G18 5 XRA 1-8A C1.4 2.0E-03 4118
3150 + 0456 0506 0516 G18 5 XRA 1-8A C2.0 2.0E-03 4118

Proton Observations Section

GOES Proton Flux

Below shows the latest GOES Proton flux measurments, courtesy of the GOES mission team, SWPC/NOAA.

3 Day Proton flux

F10.7 - Radio Indexes Section

DRAO Flux

Below shows the latest Solar Radio Flux Report courtesy of DRAO, Penticton.

Observed Flux Density124.3
Flux Density Adjusted for 1 A.U.128.4

The Solar Wind Conditions Section

ACE 24 hr Data

Below shows the latest ACE space weather conditions courtesy of SWPC/NOAA.

24 hour ACE data

DSCOVR data

Below shows the latest DSCOVR space weather conditions courtesy of SWPC/NOAA and the latest GFZ Postdam Kp measurement. The data is processed by the University of Graz.

Latest DSCOVR data

ENLIL Simulation

Below shows the latest simulation from ENLIL courtesy of SWPC/NOAA.

Latest ENLIL Simulation

The Geomagnetic Conditions Section

NOAA kp Values

Below shows the latest Planetary K index courtesy of SWPC/NOAA.

Latest NOAA kp Values

Forecast Center Section

Solar Activity Monitor

Below shows the latest solar activity courtesy of SWPC/NOAA.

Solar X-rays : Status
Geomagnetic Field : Status

Latest SIDC Forecast

Below shows the latest SIDC Forecast.


Latest SWPC Forecast

Below shows the latest SWPC Forecast.

---
Solar Activity
---
.24 hr Summary...
Solar activity was at low levels. A C1.5 flare at 22/1741 UTC from
beyond the W limb was the strongest event of the period. Some minor
development was observed in Regions 4118 (S13E22, Dai/beta) and 4117
(S15E11, Dsi/beta). The remaining spotted regions on the visible disk
were either stable or in gradual decay.
Other activity included a CME that was observed lifting off the NW
quadrant in the vicinity of Region 4115 (N22W66, Eso/beta) at around
22/1348 UTC. Analysis and modeling of the event is ongoing.
---
.Forecast...
There exists a chance for R1-R2 (Minor-Moderate) radio blackouts, with a
slight chance for X-class flares (R3-Strong), over 23-25 June.
---
Energetic Particle
---
.24 hr Summary...
The greater than 2 MeV electron flux was at low to moderate levels. The
greater than 10 MeV proton flux was at background levels.
---
.Forecast...
The greater than 2 MeV electron flux is likely to continue at low to
moderate levels over 23-25 Jun. There remains a slight chance for
the greater than 10 MeV protons to become elevated over 23-25 Jun due to
eruptive potential from multiple regions on the visible disk.
---
Solar Wind
---
.24 hr Summary...
Solar wind parameters continued to reflect a positive polarity CH HSS
regime. Total magnetic field strength was between 3-6 nT. The Bz
component reached as far south as -5 nT. Solar wind speeds varied from
~425-575 km/s. Phi angle was predominantly oriented in the positive
sector.
---
.Forecast...
Elevated solar wind parameters from the influence of multiple, recurrent
coronal holes is expected over 23-25 Jun.
---
Geospace
---
.24 hr Summary...
The geomagnetic field was at quiet to active levels.
---
.Forecast...
The geomagnetic field is likely to reach isolated periods of active
conditions over 23-24 Jun, and G1 (Minor) geomagnetic storm periods are
likely on 25 Jun, due to coronal hole effects.

Future Observations Section

Stonyhurst Heliographic image

Below shows the latest Stonyhurst Heliographic image, composed of STEREO EUVI observations. Data courtesy of the STEREO/SECCHI mission teams, NASA/GSFC.

Stonyhurst Image

Links Section

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Flare Links


Energetic Particle Links


Radio Links


CME Links


Solar Wind Links


Geomagnetism Links


Forecaster Center Links


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