Warning: Use of undefined constant referer - assumed 'referer' (this will throw an Error in a future version of PHP) in /usr/home/essaywo/public_html/essays on line 102

Warning: Use of undefined constant host - assumed 'host' (this will throw an Error in a future version of PHP) in /usr/home/essaywo/public_html/essays on line 105

Warning: Cannot modify header information - headers already sent by (output started at /usr/home/essaywo/public_html/essays:102) in /usr/home/essaywo/public_html/essays on line 106

Warning: Cannot modify header information - headers already sent by (output started at /usr/home/essaywo/public_html/essays:102) in /usr/home/essaywo/public_html/essays on line 109
Electromagnetic Waves and Observation The Sun - Example Papers

Electromagnetic Waves and Observation The Sun

Solar telescopes make use of wavelength information in two ways. For one, certain instruments, known as spectrometers, observe many wavelengths of light simultaneously and can measure how much of each wavelength of light is present. This helps create a composite understanding of what temperature ranges are exhibited in the material around the sun. Spectrographs don't look like a typical picture, but instead are graphs that categorize the amount of each kind of light.
On the other hand, instruments that produce conventional images of the sun focus exclusively on light around one particular wavelength, sometimes not one that is visible to the naked eye. SDO scientists, for example, chose ...

Want to read the rest of this paper?
Join Essayworld today to view this entire essay
and over 50,000 other term papers

is really composed of low-density particles, EM waves, neutrinos, and magnetic fields, it can certainly be approximated as such. The average distance between the Earth and the Sun over one Earth orbit is one AU (about 150,000,000,000 m), then it will take about 8 minutes for radiation from the Sun to get to Earth.
The Sun emits radiation right across the electromagnetic spectrum, from extremely high-energy X-rays to ultra-long-wavelength radio waves, and everything in-between. The peak of this emission occurs in the visible portion of the spectrum.
Different wavelengths of light generally come from different regions of the Sunā€™s atmosphere or are due to particular atoms radiating at specific wavelengths (spectral emission lines). Visible light, for example, comes from the photosphere (or surface) whereas most infrared light comes from the lower chromosphere just above. Much of the high-energy UV and X-ray photons come from the Sunā€™s outer atmosphere (called the corona). ...

Get instant access to over 50,000 essays.
Write better papers. Get better grades.

Already a member? Login

CITE THIS PAGE:

APA
MLA
Chicago
Turabian

Electromagnetic Waves and Observation The Sun. (2020, February 22). Retrieved December 23, 2024, from http://www.essayworld.com/essays/Electromagnetic-Waves-and-Observation-The-Sun/107214

"Electromagnetic Waves and Observation The Sun." Essayworld.com. Essayworld.com, 22 Feb. 2020. Web. 23 Dec. 2024. <http://www.essayworld.com/essays/Electromagnetic-Waves-and-Observation-The-Sun/107214>

"Electromagnetic Waves and Observation The Sun." Essayworld.com. February 22, 2020. Accessed December 23, 2024. http://www.essayworld.com/essays/Electromagnetic-Waves-and-Observation-The-Sun/107214.

JOIN NOW

Join today and get instant access to this and 50,000+ other essays

PAPER DETAILS

Added: 2/22/2020 07:29:09 PM
Submitted By: pukkkeye
Category: Astronomy
Type: Premium Paper
Words: 698
Pages: 3

Save |

Report

SHARE THIS PAPER

SAVED ESSAYS

Save and find your favorite essays easier