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Aurora Dashboard (Experimental) | NOAA NWS Space Weather Prediction . . . HF Radio: Weak or minor degradation of HF radio communication on sunlit side, occasional loss of radio contact Navigation: Low-frequency navigation signals degraded for brief intervals When and where can you see the northern and southern lights also known as the aurora?
Live Data - See The Aurora The real time solar wind data on this graph comes from NASA’s Deep Space Climate Observatory (DSCOVR) Satellite DSCOVR is positioned at the L1 Lagrange Point about 1 5 million km from Earth in the direction of the sun
Aurora Activity Data – Real-Time Northern and Southern Lights The aurora borealis (Northern Lights) and aurora australis (Southern Lights) are beautiful natural phenomena caused by solar particles colliding with Earth's atmosphere This page provides the current probability of auroral activity based on real-time space weather data
Scientists close in on solving the mystery behind intense auroral storms “Particles ejected from the Sun flow out through the solar system carrying the Sun’s magnetic field with them, and this ‘solar wind’ is the source of energy for the aurora “Auroral substorms are caused by the accumulation and then release of magnetic energy stored in Earth’s magnetosphere during its interaction with the solar wind
Aurorasaurus - Reporting Auroras from the Ground Up This graph shows the strength of solar wind power, a real-time indicator of how strong aurora will be in about one hour The solar wind power corresponds to the energy released by the sun over time The more energy released, the higher the power and the stronger the aurora will be
Real Time Solar Wind | NOAA NWS Space Weather Prediction Center Real-time Solar Wind and Magnetometer data is now available in JSON format for up to the past 7 days from the SWPC Data Service These JSON files will automatically include the data from the active RTSW spacecraft
Sky and Solar - Aurora Forecast That is one hour ahead forecasted amount of solar wind energy in gigawatts around Earth poles Having the value around 130-140 GW almost certainly means a visual aurora in higher mid-latitudes