Extreme-ultraviolet Imaging Telesco

Extreme-ultraviolet Imaging Telescope (EIT), observing the Sun in Fe XII at 195 Angstroms. Light at this wavelength is chiefly emitted by Fe XII (iron ionized 11 times) at 1.4 million degrees K.

Because very little UV light penetrates the Earth’s atmosphere, we have to go into space to take images like these. It is not possible for the human eye to see ultraviolet light directly. Thus, the colors of these images are just ways to represent them so we can see them. To keep the images straight, we assign certain colors to EUVI images taken in particular extreme ultraviolet (EUV) wavelengths, so usually the 195 Å images are in green.

ผลลัพธ์ (อังกฤษ) 1:

extreme-ultraviolet imaging telescope (eit), observing the sun in fe xii at 195 angstroms. light at this wavelength is chiefly emitted by fe xii (iron ionized 11 times) at 1.4 million degrees k.

because very little uv light penetrates the earth's atmosphere, we have to go into space to take images like these. it is not possible for the human eye to see ultraviolet light directly. thus,.

ผลลัพธ์ (อังกฤษ) 3:

Extreme - ultraviolet Imaging Telescope (EIT), observing the Sun in Fe XII at 195 Angstroms.Light chiefly at this wavelength is emitted by Fe XII (11 times ionized iron) at 1.4 million degrees K.

Because UV very little light penetrates the Earth' s atmosphere, we have to go into space to take images like these. It is not possible for the human eye to see ultraviolet light directly. Thus,The colors of these images are just ways to represent them so we can see them. Keep the To images straight, we assign certain colors to EUVI images taken in particular extreme ultraviolet (EUV) wavelengths, so usually the 195 workspace A images are in green.