Image

This page last updated December 11, 2019.

CURRENT SPACE WEATHER

Definition

The National Space Weather Program wrote, "Space weather refers to conditions on the Sun and in the space environment that can influence the performance and reliability of space-borne and ground-based technological systems, and can endanger human life or health."1

Current Space Weather

Note: External assets may fail to load in browsers that block mixed (HTTP and HTTPS) content; for example, Avast Secure Browser does not correctly display updated status symbols. Chrome, Opera, Firefox, and Microsoft Edge correctly display the status symbols. If the the word "Status" appears rather than the updated status symbols, simply click on nk3l.org to go to their site to view the status updates and graphs. Clicking on nk3l.org will open a new tab.


Solar X-rays:
Geomagnetic Field:
Status
Status
 

From: n3kl.org

Explanation of Space Weather Indicators Seen Above

An explanation of space weather indicators appears on a separate page.

Please go to Space Weather Indicators for the explanation. It will assist your understanding of space weather.

NOAA Space Weather Scale descriptions can be found at: NOAA Space Weather Scales.

Activity Level on the Sun

December 11, 2019

VERY LOW — No C-class flares in the past two days.

From: solarmonitor.org

Today's Sun!

Image


Photo Courtesy helioviewer.org

SIDC Info

SIDC reports visible side of the solar disc is spotless. There were no flares reported for number of days and we do not expect any flaring activity in the coming hours.

A narrow and slow, but well defined CME reported yesterday (observed in the SOHO LASCO C2 field of view at about 19:06 UT on December 09) and was associated with the brightening and small dimming at about 18:11 UT (situate at S05 W25). It is not probable that this CME will arrive to the Earth.

During last 24 hours there were no Earth directed CMEs and the solar protons remained at the background level.

The solar wind speed is presently about 420 km/s and the interplanetary magnetic field magnitude is 5 nT.

Finally, SIDC reports it is not completely clear what is the magnetic structure observed in the in situ data, and as reported yesterday. It seems like the arrival of the weak ICME was followed yesterday afternoon by the solar wind originating from the negative polarity coronal hole. The structure observed in the solar wind data did not induce disturbed geomagnetic conditions. The narrow and extended equatorial coronal hole of negative polarity reached central meridian yesterday evening. The fast solar wind associated with this coronal hole might arrive to Earth late on December 14. The geomagnetic conditions are presently quiet and we expect them to stay so in the coming hours.

Now . . . let's take a little tour into the realm of:

Image