Current Space Weather

VOACAP Quick Guide: Home

Space Weather on 17 October 2017, 05:51 UTC

SN 0 | SFI 71 | Kp 1 | Ap 6 | Kt 1 | At 17 | Bz 1.2 | XRY 4.28 | Pf 0.1 | SW 477

Sunspot Numbers for VOACAP

Below is the source of (near-)current sunspot numbers to be used with VOACAP.


Propagation tools to aid short-term prediction

Real-Time Solar Wind, National Oceanic and Atmospheric Administration, Space Environment Center

Magnetogram: State of Earth's Magnetic Field

Variations in Earth's magnetic field are measured by magnetometers. Any strong and sudden variations (up or down) in the X component (uppermost graph) are indications of VHF radio-auroral activity (e.g. on 144 MHz when variations suddenly peak, say, 300 nT)., Sodankylä Geophysical Observatory

h, Utsjoki/Kevo

Real-Time K-Index

A 3-hourly index of geomagnetic activity expressed in the logarithmic units on a scale from 0 to 9., Tromso Geophysical Observatory

X-Ray Flux

Class M and X flares affect the sunlit area of the Earth, causing increased D-region absorption. Strong flares are source of Shortwave Fadeouts (SWF) and Sudden Ionospheric Disturbances (SID). Look for the 1-8 Angstrom graph (red).

Proton Flux

High-energy protons are guided into the polar cap by Earth's magnetic field. Strong proton bursts are source of Polar Cap Absorption (PCA), i.e. high D-region absorption on paths passing through the polar areas. A proton event is in progress if the red curve crosses the threshold (dotted line) in the uppermost graph.