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: 2020 Jul 05 2012 UT
Date: 2020 07 05
#Event Begin Max End Obs Q Type Loc/Frq Particulars Reg#
NO EVENT REPORTS.

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 Density68.8
Flux Density Adjusted for 1 A.U.71.1

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.

SIDC URSIGRAM 00705
SIDC SOLAR BULLETIN 05 Jul 2020, 1255UT
SIDC FORECAST (valid from 1230UT, 05 Jul 2020 until 07 Jul 2020)
SOLAR FLARES : Quiet conditions (<50% probability of C-class flares)
GEOMAGNETISM : Quiet (A<20 and K<4)
SOLAR PROTONS : Quiet
PREDICTIONS FOR 05 Jul 2020 10CM FLUX: 070 / AP: 013
PREDICTIONS FOR 06 Jul 2020 10CM FLUX: 070 / AP: 008
PREDICTIONS FOR 07 Jul 2020 10CM FLUX: 069 / AP: 006
---
COMMENT: There is only one active region presently observed on the visible
side of the solar disc, NOAA AR 2766. This newly emerged region is
potential source of the B-class flares in the coming hours, while C-class
flares are possible but not very probable.
The eruption from the NOAA AR 2766 observed at about 05:00 UT this morning
was associated with the coronal dimming (on disc signature of the CME)
indicating possibly associated CME. As the NOAA AR 2766 is presently
situated on the center of the solar disc, the CME from this region would be
Earth-directed. More will be reported later when more observations will be
available.
During last 24 hours solar protons have remained at background level.
The in situ observations indicate arrival of the fast solar wind associated
with the low latitude extension of the northern polar coronal hole
(positive polarity) that started its passage across the central meridian in
the afternoon of July 01. At about 15:00 UT on July 04 the interplanetary
magnetic field (IMF) magnitude started to increase simultaneously with the
increase of the solar wind speed and temperature. During the passage of the
compression region between the slow and fast solar wind the IMF reached its
maximum value of 11 nT.
The solar wind speed is presently 500 km/s and the IMF magnitude is about 5
nT.
Due to intervals of the negative value of the Bz component (down to -8 nT),
unsettled geomagnetic conditions were reported before midnight on July 4
and after 09:00 UT this morning (local station at Dourbes reported interval
with K=3 and NOAA reported interval of Kp=3).
The geomagnetic conditions are presently unsettled and we expect quiet to
unsettled geomagnetic conditions in the coming hours.
---
TODAY'S ESTIMATED ISN : 006, BASED ON 19 STATIONS.
SOLAR INDICES FOR 04 Jul 2020
WOLF NUMBER CATANIA : ///
10CM SOLAR FLUX : 070
AK CHAMBON LA FORET : 016
AK WINGST : 010
ESTIMATED AP : 008
ESTIMATED ISN : 007, BASED ON 21 STATIONS.
NOTICEABLE EVENTS SUMMARY
DAY BEGIN MAX END LOC XRAY OP 10CM Catania/NOAA RADIO_BURST_TYPES
NONE
END
BT

Latest SWPC Forecast

Below shows the latest SWPC Forecast.

---
Solar Activity
---
.24 hr Summary...
Solar activity was very low. Region 2766 (N05E10, Axx/alpha) decayed
from a bi-pole group to a single spot during the period. No
Earth-directed CMEs were observed.
---
.Forecast...
Solar activity is expected to continue at very low levels 05-07 Jul.
---
Energetic Particles
---
.24 hr Summary...
The greater than 2 MeV electron flux was normal to moderate and the
greater than 10 MeV proton flux was steady at background levels.
---
.Forecast...
Both the greater than 2 MeV electron and 10 MeV proton fluxes are
expected to remain below event thresholds over 05-07 Jul.
---
Solar Wind
---
.24 hr Summary...
Solar wind parameters were enhanced due to CIR effects in advance a
positive polarity extension off the northern crown CH HSS. Total field
increased to 10 nT while the Bz component reached a maximum southward
extent of -8 nT. Solar wind gradually increased through the period from
a low of about 335 km/s to a peak of 530 km/s at about 05/0730 UTC. Phi
angle was oriented in a predominately positive solar sector.
---
.Forecast...
Solar wind enhancements are likely to persist on 05 Jul due to influence
of a positive polarity CH HSS. A more nominal solar wind environment is
expected to slowly prevail later on 06 Jul into 07 Jul.
---
Geospace
---
.24 hr Summary...
The geomagnetic field was at quiet to unsettled levels.
---
.Forecast...
The geomagnetic field is expected to be at quiet to unsettled levels,
with an isolated active interval, for the remainder of 05 Jul due to
continued positive polarity CH HSS effects. Isolated unsettled levels
are possible on 06 Jul due to diminishing CH HSS influence. A return to
mostly quiet conditions is expected on 07 Jul.

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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