Las emisiones solares llegaron a vientos de más de 800Km/s – 5 Abril – . (Actualizado)

En tiempo real:

Hiraiso Geomagnetic Activity PlotsSEC NOAA Kp Index plotsTromsø K-indices

Otra información:

Potsdam: Indices of global geomagnetic activity

Geomagnetic Data Service WDC-C Kyoto

BGS Geomagnetism Information and Forecast Service

SEC Boulder: overview of K-indices of last seven days

Geomagnetic indices ISGI

Magnetograms from Ny-Aalesund, Tromso, Leknes, Dombaas

Fuerstenfeldbruck Geomagnetic Observatory

WDC Kyoto GEOMAG QL test page

GEO-MAGNETOGRAMAS- Simuladores en Tiempo Real:

Wingst

Izmiran

Kiruna

Ny-Aalesund, Tromsø, Leknes, Dombaas

SAMNET

INTERMAGNET Kakioka

AURORAS

POES latest auroral oval position

PIXIE/POLAR latest active aurora

PIXIE/POLAR latest auroral image

UVI/POLAR current image

VIS/POLAR current image

USA Today: Understanding auroras

The Aurora: Information and Images (University of Alaska Fairbanks Geophysical Institute)

Aurorawatch UK

Aurora Forecast from the University of Alaska Fairbanks

RADIO ESTACIONES

Nobeyama Radio Heliograph

Hiraiso: latest spectrographic solar observations

Zurich Radio Spectrometer

NANCAY Radio Heliograph

Solar Radio Laboratory Izmiran

SAO Solar Radio Observations

AIP – Radio Observations Potsdam

IPS AUSTRALIA

Bruny Island Radio Spectrometer Data

Ondrejov Solar Radio Archive Info RT3/1998

Ondrejov Solar Radio Event Database

NRC Solar Radio Monitoring Programma

Trieste Astronomical Observatory: Solar Radio Emission Measurements

Solar radio astronomy at Metsahovi

Por tanto los eventuales picos superiores a 10MHz en la Ionosfera implican riesgo sísmico persistente en las zonas donde la densidad TEC, alcanza cotas de base superiores a los 10MHz.