Data lite forecasting tools (No big movies)

The purpose of this page is to provide a data-lite set of forecasting tools, it has been designed to be use on a phone, when data bandwidth is restricted or when a fast data connection is not available .


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: 2022 Jun 25 2022 UT
Date: 2022 06 25
#Event Begin Max End Obs Q Type Loc/Frq Particulars Reg#
3240 0035 0037 0041 LEA 3 FLA S13W75 SF 3035
3250 + 0053 0057 0101 G16 5 XRA 1-8A B6.5 2.9E-04 3035
3260 + 0112 0121 0132 G16 5 XRA 1-8A B6.7 7.4E-04 3038
3270 0238 0238 0238 PAL G RBR 245 130
3280 + 0409 0421 0426 G16 5 XRA 1-8A B6.8 5.7E-04 3040
3300 0413 0414 0419 LEA 3 FLA N01W79 4F 3034
3280 + 0413 //// 0416 LEA C RSP 025-180 III/2 3040
3290 0426 0433 0438 G16 5 XRA 1-8A B8.1 5.3E-04 3035
3310 + 0720 0726 0733 G16 5 XRA 1-8A B6.4 4.7E-04 3038
3320 + 0819 //// 0819 LEA C RSP 025-180 III/2
3360 0908 //// 0952 SVI C RSP 115-180 CTM/1
3330 0912 0912 0912 SVI G RBR 410 150
3340 0938 0938 0939 SVI G RBR 245 880
3340 + 0938 //// 0939 SVI C RSP 025-180 III/1
3360 0942 //// 1122 SAG C RSP 114-180 III/1
3350 1017 1017 1017 SAG U RBR 245 100
3370 + 1039 1039 1039 SVI G RBR 245 150
3380 + 1114 1122 1133 G16 5 XRA 1-8A B6.7 6.6E-04
3390 + 1352 1402 1406 G16 5 XRA 1-8A C1.2 5.5E-04 3040
3390 + 1357 //// 1401 SAG C RSP 025-180 III/2 3040
3390 1400 1400 1400 SAG U RBR 245 120 3040
3390 1401 1402 1404 SVI 3 FLA S15E20 SF 3040
3400 1456 //// 1517 SAG C RSP 025-180 VI/2 3040
3400 1514 1515 1517 HOL 3 FLA S14E20 SF 3040
3410 + 1626 //// 1630 SAG C RSP 025-154 III/1
3420 1638 1646 1650 HOL 3 FLA S12E19 SF ERU 3040
3430 + 1711 //// 1712 SVI C RSP 115-180 III/2
3440 + 1753 //// 1814 PAL C RSP 025-085 VI/1
3450 1845 1845 1845 SAG U RBR 245 120

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 Density106.5
Flux Density Adjusted for 1 A.U.110.0

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 very low to low. The largest flare was a C1 at
24/1844 UTC from plage Region 3035 (S17, L=073). Regions 3038 (N16W68,
Eho/beta) and 3040 (S13E21, Cso/beta) continued to decay over the
period.
STEREO A COR2 imagery displayed a narrow CME slightly north of the
ecliptic at 24/1838 UTC that likely was associated with coronal dimming
in the NW quadrant around 24/1800 UTC. SOHO/LASCO coronagraph imagery
was inconclusive. Preliminary modelling of the CME indicated a potential
grazing blow mid to late on 28 Jun, however confidence in the run is
low.
---
.Forecast...
Solar activity is likely to be low with a slight chance for M-class
flares (R1-R2, Minor-Moderate) through 27 Jun.
---
Energetic Particle
---
.24 hr Summary...
The greater than 2 MeV electron flux was at normal to moderate levels.
The greater than 10 MeV proton flux continued at background levels.
---
.Forecast...
The greater than 2 MeV electron flux is expected to reach moderate
levels through 27 Jun. The greater than 10 MeV proton flux is expected
to continue at background levels.
---
Solar Wind
---
.24 hr Summary...
Solar wind parameters were enhanced over the period with total field
increasing from 6 nT to 14 nT. Solar wind speed was mostly in the
400-450 range. Phi was oriented in a negative sector.
---
.Forecast...
Enhancements to the solar wind parameters are expected to continue
through 27 Jun due to CH HSS influence.
---
Geospace
---
.24 hr Summary...
The geomagnetic field was at quiet to unsettled levels.
---
.Forecast...
The geomagnetic field is likely to reach active conditions on 25-26 Jun
due to anticipated interaction with a negative polarity CH HSS.
Unsettled conditions are expected on 27 Jun as CH influence wanes.

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

Viewers Links


Regions Links


Flare Links


Energetic Particle Links


Radio Links


CME Links


Solar Wind Links


Geomagnetism Links


Forecaster Center Links


Other Links