There are two ways to look at the Sun safely: by direct viewing, with a proper filter over the front of the telescope, or by projecting the Sun's image onto a piece of paper. They protect the eye against both visible and invisible radiations and the telescope itself against heat.
Specialized tools such as spectroscopes and spectrohelioscopes are used to examine sunspots and sunspot areas.
Scientists study the Sun number in a number of ways including ground based telescopes and satellites to obtain as much information as possible. The atmosphere of the Sun varies in temperature so a whole range of wavelengths are needed to make complete observations.
By examining pictures of the sun in a variety of wavelengths – as is done through such telescopes as NASA's Solar Dynamics Observatory (SDO), NASA's Solar Terrestrial Relations Observatory (STEREO) and the ESA/NASA Solar and Heliospheric Observatory (SOHO) -- scientists can track how particles and heat move through the ...
Sunspots are often precursors to solar flares – intense outbursts of energy from the surface of the Sun – so monitoring sunspots is important to understanding why and how flares occur. Additionally, understanding the frequency of flares on other stars is one of the keys to understanding their chance of harboring life.
Surveying sunspots with daily hand-drawn drawings is the most basic of ways we study how solar activity rises and falls over time, and it's the basis of how we track the solar cycle.
Sunspots are areas that appear dark on the surface of the Sun. They appear dark because they are cooler than other parts of the Sun's surface. Solar flares are a sudden explosion of energy caused by tangling, crossing or reorganizing of magnetic field lines near sunspots.
Engineers make telescopes, imaging systems and satellites to view the Sun and its events. They also make solar panel collectors and other solar-powered devices used on Earth.
Magnetic field lines come out of the surface of the Sun through one sunspot, and go back in through the other. The strong magnetic field around the sunspots stops heat being moved by convection. Convection moves heat from deeper inside the Sun to the surface.
There are two ways that solar telescopes can gather information from the light emitted by the sun. There are spectrometers that can simultaneously observe different wavelengths of light, generating graphs that give a composite picture of the temperature ranges in the material around the sun.
The Sun is an almost perfectly spherical ball of hot plasma interwoven with magnetic fields. It has a diameter of about 1,392,000 km, about 109 times that of Earth, and its mass (about 330,000 times that of Earth) accounts for about 99.86% of the total mass of the Solar System.
Those telescopes are very similar to the ones we use on the ground, but they have special filters that allow only this extreme ultraviolet light to get through. And then they have a CCD [an image sensor] where the pictures are taken.