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GOES Electron Flux Showing Electron Bombardment Radiation Storm Levels - Space Weather Watch

2,173 views · Published 3 November 2017 · 12:32 · Indexed 12 November 2026

Channel: Oppenheimer Ranch Project · 2017 · People & Blogs

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Solar radiation storm
S3 solar radiation storm is classified as STRONG radiation storm that can cause isolated reboots of computers onboard Earth-orbiting satellites and made noise in imaging systems, reduction of efficiency in solar panel, it can degraded HF radio propagation through the polar regions and caused errors at navigation position. S3 solar radiation storm can also influenced passengers and crew in  high-flying aircraft at high latitudes due to radiation exposure. At this level of solar radiation astronauts on EVA are reccomended to take radiation hazard avoidance. High energy particle measurements (greater than 100 MeV) are a better indicator of radiation risk to passenger and crews. Pregnant women are particularly susceptible. NASA routinely monitors space weather conditions to determine any potential hazards to the astronauts aboard the International Space Station. Based on the agency's assessment, the six spaceflyers currently living and working on the orbiting outpost are not in any danger. https://watchers.news/2012/01/24/increased-solar-activity-after-strongest-solar-radiation-storm-since-2006/

SOLAR RADIATION STORM
Solar radiation storms occur when a large-scale magnetic eruption, often causing a coronal mass ejection and associated solar flare, accelerates charged particles in the solar atmosphere to very high velocities. The most important particles are protons which can get accelerated to 1/3 the speed of light or 100,000 km/sec. At these speeds, the protons can traverse the 150 million km from sun to Earth in just 30 minutes. When they reach Earth, the fast moving protons penetrate the magnetosphere that shields Earth from lower energy charged particles. Once inside the magnetosphere, the particles are guided down the magnetic field lines such that they penetrate the atmosphere near the north and south poles.

NOAA categorizes Solar Radiation Storms using the NOAA Space Weather Scale on a scale from S1 - S5. The scale is based on measurements of energetic protons taken by the GOES satellite in geosynchronous orbit. The start of a Solar Radiation Storm is defined as the time when the flux of protons at energies (greater or equal to) 10 MeV equals or exceeds 10 proton flux units (1 pfu = 1 particle*cm-2*s-1*ster-1). The end of a Solar Radiation Storm is defined as the last time when the flux of (greater or equal to) 10 MeV protons is measured at or above 10 pfu. This definition allows multiple injections from flares and interplanetary shocks to be encompassed by a single Solar Radiation Storm. A Solar Radiation Storm can persist for time periods ranging from hours to days.

Solar Radiation Storms cause several impacts near Earth. When energetic protons collide with satellites or humans in space, they can penetrate deep into the object that they collide with and cause damage to electronic circuits or biological DNA. During Solar Radiation Storms at the S2 or higher level passengers and crew in high flying aircraft at high latitudes may be exposed to radiation risk. When the energetic protons collide with the atmosphere, they ionize the atoms and molecules thus creating free electrons. These electrons create a layer near the bottom of the ionosphere that can absorb High Frequency (HF) radio waves making radio communication difficult or impossible.
http://www.swpc.noaa.gov/phenomena/solar-radiation-storm


Solar Electron Flux - Dark Electrons Found by NASA
 http://electric-cosmos.org/SolarElecFlux2013.pdf

GOES Electron Flux Graph:
http://legacy-www.swpc.noaa.gov/rt_plots/elec_3d.html

http://legacy-www.swpc.noaa.gov/alerts/warnings_timeline.html

http://onlinelibrary.wiley.com/doi/10.1002/2014SW001069/pdf

https://ntrs.nasa.gov/archive/nasa/casi.ntrs.nasa.gov/20140012586.pdf

https://arxiv.org/ftp/arxiv/papers/0906/0906.3884.pdf

https://www.spaceweatherlive.com/images/help/protonenstorm/EN_protonenstorm.jpg

http://www.weather.gov/images/akq/Briefing/SolarRadiationStormScale.jpg

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