Ancient civilizations did not have technology to observe solar flares as we do today. However, they may have witnessed increased solar activity such as auroras caused by solar flares, which would have been visible in the night sky.
Solar flares, sunspots and prominences are features of the sun that have some effects on Earth: 1. Sunspots- Dark areas around the surface of the sun that are cooler than surrounding areas. They appear and disappear over a period of time. The period from minimum to maximum number of appearances of sunspots is the sunspot cycle, which occurs every 11 years. Sunspots are believed to have effects on Earth's weather and climate. Low temperatures in some countries and drought in other countries were observed during a period when very few sunspots appeared on the sun's surface. 2. Prominences- Arches of gas that rise from the sun's surface and flow back to it caused by magnetic fields of sunspots. Some prominences are in the forms of loops, curtains, or funnels. Solar prominences may last for many hours and can extend millions of kilometers above the surface of the sun. 3. Solar flares- Violent eruptions that are suddenly released and are caused by magnetic energy stored in the corona. Ultraviolet light and X rays from solar flares cause disruption of radio signals, making communication by radio and telephone difficult. Magnetic storms occur on Earth when electrically charged particles from the corona and solar flares ae added to the solar wind produced by the corona. When this happens, Earth's atmosphere radites beautiful lights called aurora borealis or northern lights. This same light is called the aurora australis in the southern hemisphere.
Solar flares are difficult to predict accurately, but they tend to occur at the peak of the 11-year solar cycle. The current solar cycle, Solar Cycle 25, is expected to peak around 2025-2026, so there may be an increased likelihood of solar flares around that time. However, exact timing of solar flares is uncertain.
Solar flares often occur near sunspots because sunspots are areas of intense magnetic activity on the Sun's surface. These strong magnetic fields can become twisted and stressed, leading to the release of energy in the form of solar flares. The interaction between the magnetic fields in sunspots creates conditions that are conducive to the production of solar flares.
Vehicles that are not affected by solar flares are those that do not rely heavily on electronic systems for operation, such as older model cars without extensive computerized components or manual transmission vehicles. Additionally, vehicles that are shielded from electromagnetic interference, such as military vehicles designed for use in high-electromagnetic environments, may also be less affected by solar flares.
Corona
Ancient civilizations did not have technology to observe solar flares as we do today. However, they may have witnessed increased solar activity such as auroras caused by solar flares, which would have been visible in the night sky.
Solar prominence are seen in the photosphere of the sun that goes further in the corona. These prominences can reach out over thousands of kilometers.
Solar flares, sunspots and prominences are features of the sun that have some effects on Earth: 1. Sunspots- Dark areas around the surface of the sun that are cooler than surrounding areas. They appear and disappear over a period of time. The period from minimum to maximum number of appearances of sunspots is the sunspot cycle, which occurs every 11 years. Sunspots are believed to have effects on Earth's weather and climate. Low temperatures in some countries and drought in other countries were observed during a period when very few sunspots appeared on the sun's surface. 2. Prominences- Arches of gas that rise from the sun's surface and flow back to it caused by magnetic fields of sunspots. Some prominences are in the forms of loops, curtains, or funnels. Solar prominences may last for many hours and can extend millions of kilometers above the surface of the sun. 3. Solar flares- Violent eruptions that are suddenly released and are caused by magnetic energy stored in the corona. Ultraviolet light and X rays from solar flares cause disruption of radio signals, making communication by radio and telephone difficult. Magnetic storms occur on Earth when electrically charged particles from the corona and solar flares ae added to the solar wind produced by the corona. When this happens, Earth's atmosphere radites beautiful lights called aurora borealis or northern lights. This same light is called the aurora australis in the southern hemisphere.
Solar flares are difficult to predict accurately, but they tend to occur at the peak of the 11-year solar cycle. The current solar cycle, Solar Cycle 25, is expected to peak around 2025-2026, so there may be an increased likelihood of solar flares around that time. However, exact timing of solar flares is uncertain.
Solar flares often occur near sunspots because sunspots are areas of intense magnetic activity on the Sun's surface. These strong magnetic fields can become twisted and stressed, leading to the release of energy in the form of solar flares. The interaction between the magnetic fields in sunspots creates conditions that are conducive to the production of solar flares.
Solar flares, coronal mass ejections (CMEs), and coronal holes are solar features that can increase the solar wind. These events release charged particles into space at high speeds, which contribute to the solar wind.
Solar flares are sudden brightening of the sun caused by ejection of huge energies. Solar flares will most likely not affect the colour light because solar flares produces radiation across the electromagnetic spectrum at all wavelengths, from radio waves to gamma rays. Thus, it is difficult to view solar flares on the visible spectrum and must be viewed with special instruments.In other words, photons (light particles/waves) from a solar flare are emitted at all frequencies along the electromagnetic spectrum and must be viewed with special equipment. Unless the solar flare interacts with anything else (maybe other atmospheres), they don't change the colour of light.
Vehicles that are not affected by solar flares are those that do not rely heavily on electronic systems for operation, such as older model cars without extensive computerized components or manual transmission vehicles. Additionally, vehicles that are shielded from electromagnetic interference, such as military vehicles designed for use in high-electromagnetic environments, may also be less affected by solar flares.
Corona
Solar flares are difficult to predict with high precision. Scientists can forecast general activity levels using models and monitoring sunspots, but the exact timing and strength of individual flares are challenging to predict accurately.
Solar flares can be predicted to some extent based on monitoring solar activity, such as the appearance of sunspots and changes in magnetic fields. However, accurately predicting the exact timing and magnitude of a solar flare remains a challenge due to the complex nature of solar dynamics.