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: 2023 Mar 20 2237 UT
Date: 2023 03 20
#Event Begin Max End Obs Q Type Loc/Frq Particulars Reg#
9070 + 0057 0114 0119 G16 5 XRA 1-8A C4.1 3.3E-03 3256
9080 + 0119 0148 0226 G16 5 XRA 1-8A M1.2 4.2E-02 3256
9070 0124 0124 0124 PAL G RBR 410 100
9070 0124 //// 0208 PAL C RSP 045-180 VI/1
9140 A0253 //// A0539 LEA 3 DSF N10E60 8
9090 0441 //// 0441 LEA C RSP 100-180 III/1
9100 0524 //// 0528 SVI C RSP 115-180 III/1
9110 0551 //// 0807 SVI C RSP 025-180 CTM/1
9120 + B0731 U0805 A0857 SVI 3 FLA S20E54 SF 3259
9150 0924 0937 0949 G16 5 XRA 1-8A C5.2 5.5E-03 3256
9130 + 0927 //// 0936 SVI C RSP 025-180 III/2 3256
9130 0928 0933 0947 LEA 3 FLA S25E39 1F DSF 3256
9130 + 0932 0932 0932 SVI G RBR 245 100 3256
9130 0933 0933 0933 LEA G RBR 410 58 3256
9180 1407 1534 1814 G16 5 XRA 1-8A C4.4 4.7E-02 3258
9160 1507 //// 1510 SAG C RSP 113-152 III/1
9170 1901 //// 1902 SAG C RSP 116-149 III/1

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 Density156.1
Flux Density Adjusted for 1 A.U.154.8

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 reached moderate levels. Region 3256 (S23E48, Eko/beta)
produced a long-duration M1 flare at 20/0148 UTC; the largest event of
the period. Region 3256 exhibited growth and had some intermediate spots
develop. Minor growth was also observed in Region 3259 (S16E66,
Bxo/beta). The remaining regions were stable. No Earth-directed CMEs
were detected.
---
.Forecast...
Solar activity is expected to be low with a chance for M-class flares
over 20-22 Mar.
---
Energetic Particle
---
.24 hr Summary...
The greater than 10 MeV proton flux was slightly enhanced at around 1
pfu this period. The greater than 2 MeV electron flux was normal to
moderate.
---
.Forecast...
The greater than 10 MeV proton flux is likely to remain slightly
elevated above background levels through late 20 Mar or early 21 Mar.
The greater than 2 MeV electron flux is expected to be normal to
moderate throughout the forecast period.
---
Solar Wind
---
.24 hr Summary...
A mostly nominal solar wind environment prevailed. Solar wind speed
varied between 400-480 km/s, total field strength was steady near 5-7
nT, and Bz reached -6 nT late in the period.
---
.Forecast...
Elevated solar wind conditions are expected on 20-21 Mar due to the
influence of a positive polarity CH HSS and the glancing blow arrival of
a CME from 17 Mar. Nominal conditions are expected on 22 Mar.
---
Geospace
---
.24 hr Summary...
The geomagnetic field was quiet and unsettled.
---
.Forecast...
The geomagnetic field is expected to reach active levels on 20-21 Mar
due to the influence of a positive polarity CH HSS and the glancing blow
arrival of a CME from 17 Mar. Quiet conditions are expected to prevail
on 22 Mar.

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