Lokaal brand risico:
CBI


Regionaal brand risico: Meer informatie


bezoek onze andere website:

Weerstation
Sluispark-Leuven



Space Weather Observations, Alerts, and Forecast

Forecast text

:Product: 3-Day Forecast
:Issued: 2017 Oct 22 1230 UTC
# Prepared by the U.S. Dept. of Commerce, NOAA, Space Weather Prediction Center
#
A. NOAA Geomagnetic Activity Observation and Forecast

The greatest observed 3 hr Kp over the past 24 hours was 3 (below NOAA
Scale levels).
The greatest expected 3 hr Kp for Oct 22-Oct 24 2017 is 5 (NOAA Scale
G1).

NOAA Kp index breakdown Oct 22-Oct 24 2017

            Oct 22     Oct 23     Oct 24
00-03UT        3          2          2     
03-06UT        2          1          2     
06-09UT        1          2          2     
09-12UT        1          1          2     
12-15UT        1          1          3     
15-18UT        2          1          3     
18-21UT        2          1          4     
21-00UT        2          2          5 (G1)

Rationale: G1 (Minor) geomagnetic storm conditions are likely on day
three (24 Oct) due to the anticipated onset of a positive polarity CH
HSS.

B. NOAA Solar Radiation Activity Observation and Forecast

Solar radiation, as observed by NOAA GOES-13 over the past 24 hours, was
below S-scale storm level thresholds.

Solar Radiation Storm Forecast for Oct 22-Oct 24 2017

              Oct 22  Oct 23  Oct 24
S1 or greater    1%      1%      1%

Rationale: No S1 (Minor) or greater solar radiation storms are expected.
No significant active region activity favorable for radiation storm
production is forecast.

C. NOAA Radio Blackout Activity and Forecast

No radio blackouts were observed over the past 24 hours.

Radio Blackout Forecast for Oct 22-Oct 24 2017

              Oct 22        Oct 23        Oct 24
R1-R2           20%           20%           20%
R3 or greater    1%            1%            1%

Rationale: There exists a slight chance for R1-R2 (Minor-Moderate) radio
blackouts over the next three days due to the flare potential from
Region 2685.

Sun Images


eit 171 eit 195 eit 284 eit 304
 

Images: From left to right: EIT 171, EIT 195, EIT 284, EIT 304 EIT (Extreme ultraviolet Imaging Telescope) images the solar atmosphere at several wavelengths, and therefore, shows solar material at different temperatures. In the images taken at 304 Angstrom the bright material is at 60,000 to 80,000 degrees Kelvin. In those taken at 171 Angstrom, at 1 million degrees. 195 Angstrom images correspond to about 1.5 million Kelvin, 284 Angstrom to 2 million degrees. The hotter the temperature, the higher you look in the solar atmosphere.

 
SDO/HMI
Continuum
SDO/HMI
Magnetogram
LASCO C2 LASCO C3
 

The MDI (Michelson Doppler Imager) images shown here are taken in the continuum near the Ni I 6768 Angstrom line. The most prominent features are the sun spots.
 

LASCO (Large Angle Spectrometric Coronagraph) is able to take images of the solar corona by blocking the light coming directly from the Sun with an occulter disk, creating an artificial eclipse within the instrument itself.

 for more information

Bigger versions of this page in a new window:
New regular size page, New 1280×1024 window, and New 1600×1200 window.

Solar cycle


Sunspot numbers F10.7CM Radio flux AP
 
 for more information

The Solar Cycle is observed by counting the frequency and placement of sunspots visible on the Sun. Solar minimum occurred in December, 2008. Solar maximum in May, 2013.

 
Solar wind Satellite impact Xray flux
 
 for more information for more information for more information

On the left: Real-Time Solar Wind data broadcast from NASA's ACE satellite. Middle: The Satellite Environment Plot combines satellite and ground-based data to provide an overview of the current geosynchronous satellite environment. Right: 3-days of 5-minute solar x-ray flux values measured on the SWPC primary and secondary GOES satellites.

Auroral activity


Northern Auroral map Southern Auroral map
 

Instruments on board the NOAA Polar-orbiting Operational Environmental Satellite (POES) continually monitor the power flux carried by the protons and electrons that produce aurora in the atmosphere. SWPC has developed a technique that uses the power flux observations obtained during a single pass of the satellite over a polar region (which takes about 25 minutes) to estimate the total power deposited in an entire polar region by these auroral particles. The power input estimate is converted to an auroral activity index that ranges from 1 to 10.

Alerts


Introduction Movie


Conditions on the Sun and in the solar wind, magnetosphere, ionosphere and thermosphere that can influence the performance and reliability of space-borne and ground-based technological systems and can endanger human life or health. This introduction movie in the English language will open on a new tab/window when you click on the image below.



Also in Quicktime format: Large (269M) and Small ( 60M).


Credits:

Space Weather Images and Information (excluded from copyright) courtesy of:
NOAA / NWS Space Weather Prediction Center, Mauna Loa Solar Observatory (HAO/NCAR), and SOHO (ESA & NASA).

u vindt ons ook hier:

WeatherCloud

Weather Underground

benelux weer netwerk

AWEKAS

WeatherlinkIP

Het Weer Aktueel

European Weather Network

apparatuur in gebruik:

weerstation
Davis VP2 weatherstation

weerprogramma
Meteobridge

weercomputer
Asus WL -330N3G

webleverancier
Robohost

Davis VP2 weatherstation

Meteobridge

Asus WL -330N3G

Robohost