More Information
About The Solar-Flares
Solar flares are relatively intense, localized emissions of electromagnetic radiation that occur in the Sun’s atmosphere. These explosive events release vast amounts of energy and are often associated with sunspots.The intensity of a solar flare determines its classification, with X-class flares being the most powerful, followed by M-, C-, and B-class flares
Solar flares are giant explosions on the sun that send energy, light and high speed particles into space. These flares are often associated with solar magnetic storms known as coronal mass ejections (CMEs). The number of solar flares increases approximately every 11 years, and the sun is currently moving towards another solar maximum, likely in 2013.
Discover More
What is FRADSCR??
The high school project known as FRADSCR, or Flare Radiation Assessment Detection System and Cubesat Response, is still changing the world. The main objective of this initiative is to mitigate Ethiopia's drought issues, which are caused by a solar cycle that occurs every ten years. East Africa is home to Ethiopia. The project's objective is to put in place a mechanism that would enable locals and the government to be adequately ready for upcoming shifts in space weather.
Based on data from NASA's RHESSI mission, this study developed a model that attempts to forecast solar flare strength for a specific year, either past or future. Use the button below to access the prediction.
Predict Now
Discover the most
known Solar-Flares
X-class
>10^-4(W/m^2)
M-class
10^-5-10^-4(W/m^2)
A-class
10^-7(W/m^2)With Our Research &
Scientists Discoveries
11
YearSolar Cycle
5
Categories ofSolar-Flares
With
DifferentStrength
Video Tour
Find out more with our video of the most beautiful Solar-Flares ever existed!!
See More Solar-Flares
A-Class
Solar-Flare
B-Class
Solar-Flare
C-Class
Solar-Flare
X-Class
Solar-Flare
M-class
Solar-FlareJoin Our
Community
Meet the T.E.A.M
