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.
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.
Below shows the latest CME detections, courtesy of the CACTus CME catalog, generated and maintained by the SIDC at the Royal Observatory of Belgium.
Below shows the latest GOES x-ray flux measurments, courtesy of the GOES mission team, SWPC/NOAA.
Below shows the latest GOES x-ray flare detections, courtesy of the GOES mission team, SWPC/NOAA.
Created: 2024 Mar 29 1057 UT | ||||||||||
Date: 2024 03 29 | ||||||||||
#Event | Begin | Max | End | Obs | Q | Type | Loc/Frq | Particulars | Reg# | |
9430 | 0000 | //// | 0004 | PAL | C | RSP | 025-149 | VI/2 | ||
9440 | 0047 | 0054 | 0102 | G16 | 5 | XRA | 1-8A | C4.6 | 3.5E-03 | 3615 |
9440 | 0052 | //// | 0055 | PAL | C | RSP | 025-180 | V/3 | ||
9450 | 0148 | 0206 | 0217 | G16 | 5 | XRA | 1-8A | C9.4 | 1.4E-02 | 3615 |
9460 | 0217 | 0230 | 0242 | G16 | 5 | XRA | 1-8A | M3.2 | 3.4E-02 | 3615 |
9460 + | 0218 | //// | 0222 | LEA | C | RSP | 025-180 | III/3 | 3615 | |
9460 + | 0218 | 0219 | 0221 | LEA | G | RBR | 4995 | 200 | 3615 | |
9460 + | 0218 | 0218 | 0219 | LEA | G | RBR | 8800 | 160 | 3615 | |
9460 | 0219 | 0222 | 0250 | LEA | 3 | FLA | S15W63 | SF | 3615 | |
9450 | 0223 | //// | 0715 | LEA | C | RSP | 076-180 | CTM/1 | 3615 | |
9460 | 0225 | 0225 | 0226 | PAL | G | RBR | 245 | 750 | 3615 | |
9470 + | 0306 | //// | 0307 | LEA | C | RSP | 025-180 | III/1 | ||
9480 + | 0340 | //// | 0347 | LEA | C | RSP | 025-180 | III/2 | ||
9490 | 0437 | 0446 | 0454 | G18 | 5 | XRA | 1-8A | C3.1 | 2.9E-03 | 3615 |
9500 | 0500 | //// | 0500 | LEA | C | RSP | 025-160 | III/1 | ||
9510 | 0556 | 0556 | 0601 | SVI | 3 | FLA | S15W62 | SF | 3615 | |
9520 | 0607 U | 0630 | A0703 | SVI | 3 | FLA | S15W62 | SF | 3615 | |
9520 | 0627 | //// | 0627 | LEA | C | RSP | 025-114 | III/1 | 3615 | |
9530 + | 0725 | 0731 | 0737 | G16 | 5 | XRA | 1-8A | C3.4 | 2.4E-03 | 3615 |
9530 | 0726 U | 0726 | A0748 | SVI | 3 | FLA | S14W64 | SF | 3615 | |
9540 | 0755 | 0758 | 0801 | SVI | 3 | FLA | S12W69 | SF | 3615 | |
9550 | 0811 U | 0811 | A0820 | SVI | 3 | FLA | S15W63 | SF | 3615 | |
9560 | 0902 U | 0907 | A0918 | SVI | 3 | FLA | S13W69 | SF | ERU | 3615 |
Below shows the latest GOES Proton flux measurments, courtesy of the GOES mission team, SWPC/NOAA.
Below shows the latest Solar Radio Flux Report courtesy of DRAO, Penticton.
Observed Flux Density | 171.0 |
---|---|
Flux Density Adjusted for 1 A.U. | 170.4 |
Below shows the latest ACE space weather conditions courtesy of SWPC/NOAA.
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.
Below shows the latest simulation from ENLIL courtesy of SWPC/NOAA.
Below shows the latest Planetary K index courtesy of SWPC/NOAA.
Below shows the latest solar activity courtesy of SWPC/NOAA.
Solar X-rays : | |
---|---|
Geomagnetic Field : |
Below shows the latest SIDC Forecast.
Below shows the latest SWPC Forecast.
--- |
Solar Activity |
--- |
.24 hr Summary... |
Solar activity reached high levels. Region 3615 (S13W69, |
Fkc/beta-gamma-delta) produced the strongest events of the period, an |
X1.1/3b flare (R3 - Strong) at 28/2101 UTC and two impulsive M-class |
flares; an M7.1/1n flare (R2-Moderate) at 28/0629 UTC and an M6.1 flare |
(R2) at 28/1556 UTC. The region continued to develop and added area to |
its trailer spots while maintaining multiple deltas in the intermediate |
and trailer portion of the group. The remaining numbered regions were |
mostly stable or in decay. |
GOES-16 SUVI 304 angstroms imagery suggests that a C8.4 flare at 28/0943 |
UTC from Region 3615 did result in ejecta. Subsequent SOHO/LASCO C2 |
imagery contained a faint and narrow ejecta that is not suspected to be |
Earth-directed. With the X1.1 event at 28/2101 UTC, SOHO/LASCO imagery |
indicated slow-moving ejecta off the SW limb, first visible at 28/2124 |
UTC. Analysis is ongoing for any Earth-directed component. No other |
potentially Earth-directed CMEs were observed in available coronagraph |
imagery. |
--- |
.Forecast... |
Solar activity is expected to continue at moderate to high levels |
(R1-R2/Minor-Moderate), with a chance for an X-class flares (R3/Strong), |
over 29-30 Mar primarily due to the flare potential of Region 3615. |
As Region 3615 rotates beyond the western limb, R1 (Minor) or greater |
events are no longer likely. |
--- |
Energetic Particles |
--- |
.24 hr Summary... |
The greater than 10 MeV proton flux was near background levels. The |
greater than 2 MeV electron flux was at normal to moderate levels. |
--- |
.Forecast... |
A slight chance for S1 (Minor) solar radiation storms will persist |
through 30 Mar primarily due to the potential and location of AR 3615. |
As AR 3615 rotates off of the visible disk after 30 Mar, S1 or greater |
radiation storms will no longer be likely. There is a chance for the |
greater than 2 MeV electron flux to reach high levels beginning on 30 |
Mar. |
--- |
Solar Wind |
--- |
.24 hr Summary... |
Solar wind parameters returned to nominal levels. Total magnetic field |
strength was below 5 nT. Solar wind speeds ended the period near ~400 |
km/s. Phi angle was predominantly negative. |
--- |
.Forecast... |
Solar wind conditions may become slightly elevated by late 29 Mar |
under weak, negative polarity CH HSS influences, which may continue |
through 30 Mar. A possible weak enhancement from the periphery of a CME |
that left the Sun on 26 Mar is possible over 31 Mar. |
--- |
Geospace |
--- |
.24 hr Summary... |
The geomagnetic field was at quiet to isolated unsettled levels. |
--- |
.Forecast... |
The geomagnetic field is likely to be at mostly quiet levels, with |
potential isolated periods of unsettled conditions, over the next three |
days. |
Below shows the latest Stonyhurst Heliographic image, composed of STEREO EUVI observations. Data courtesy of the STEREO/SECCHI mission teams, NASA/GSFC.