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2711
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Top 10
Flares
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01. X9.3
02. X8.2
03. X6.9
04. X5.4
05. X4.9
06. X3.3
07. X3.2
08. X3.1
09. X2.8
10. X2.7

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The Sun Today : Updated May 24, 2018

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Solar Flare Risk
M-Class: 05%
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Geomag. Storm    NO
Radiation Storm    NO

Solar X-Rays:
Status
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Status

3-Day Geomagnetic Forecast [Details]
May 24
May 25
May 26
4 (G0)
Max Kp
3 (G0)
Max Kp
3 (G0)
Max Kp
Prob-M 10%
Prob-H 40%
Prob-M 05%
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[Lasco] C2 >>
Latest Space Weather News and Updates
May 23, 2018 @ 09:30 UTC
New Active Region?
Things have been really quiet as of late on the sun, however a possible new active region is about to turn into view off the east limb. A number of very minor B-Flares are currently being detected and there will likely be a chance for an isolated C-Flare as well. We will know more about what lies behind the limb during the next few days. Image below by SDO/AIA..

May 17, 2018 @ 00:20 UTC
Geomagnetic Storm Watch
A small coronal hole is now facing Earth. A brief period of minor (G1) geomagnetic storming is in the forecast for the next 24 hours should an elevated solar wind stream skirt past our planet. Sky watchers should be alert for visible aurora at very high latitudes.


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REPORTS AND FORECAST | 30 Day DSD | Data Warehouse


Prepared jointly by the U.S. Dept. of Commerce, NOAA,
Space Weather Prediction Center.
UPDATED 2018 May 24 0030 UTC

.24 hr Summary...
Solar activity increased to low levels, due to a C2 flare at 23/1821 UTC
from an area of enhanced X-ray flux just beyond the NE limb at
approximately N15E90. This same active region also produced frequent
B-class flares during the reporting period.

Region 2710 (N18E38, Bxo/beta) underwent some decay and was inactive.
Region 2711 (N06W28, Dao/beta) grew in coverage and matured in
complexity. Despite the growth, the regions overall magnetic field
strength was minor and its magnetic gradient and shear were weak;
however, it did produce some minor B-level enhancements. No
Earth-directed CMEs were observed in available coronagraph imagery.

.Forecast...
Solar activity is expected to be very low, with a chance for isolated
occurrences of C-class flares all three days (24-26 May) due primarily
to persistence considerations from the active region just beyond the NE
limb. This region is anticipated to rotate onto the visible disk by day
one, allowing for a better analysis. Some additional flare contribution
is possible from Region 2711 through the forecast period.

[Report of Solar-Geophysical Activity]

NOAA SUNSPOT SUMMARY | SolarHam Sunspot Summary

A - Alpha (single polarity spot).
B - Beta (bipolar spot configuration).
G - Gamma (atypical mixture of polarities).
BG - Beta-Gamma (mixture of polarities in a dominantly bipolar configuration).
D - Delta (opposite polarity umbrae within single penumbra).
BD - Beta with a Delta configuration.
BGD - Beta-Gamma with a Delta configuration.

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