Preliminary Table of Solar Spectrum Wave-Lengths, Part 1
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"Preliminary Table of Solar Spectrum Wave-Lengths, Part 1" by Henry Augustus Rowland presents detailed data on solar spectrum wave-lengths as observed and measured in the late 19th century. This work is a significant contribution to the field of astrophysics and spectroscopy, offering valuable insights into the composition and characteristics of the sun. Rowland's meticulous measurements and observations provide a historical record that remains relevant for researchers and historians of science. This early study laid the groundwork for future advancements in solar physics and our understanding...
"Preliminary Table of Solar Spectrum Wave-Lengths, Part 1" by Henry Augustus Rowland presents detailed data on solar spectrum wave-lengths as observed and measured in the late 19th century. This work is a significant contribution to the field of astrophysics and spectroscopy, offering valuable insights into the composition and characteristics of the sun. Rowland's meticulous measurements and observations provide a historical record that remains relevant for researchers and historians of science. This early study laid the groundwork for future advancements in solar physics and our understanding of stellar phenomena. It is an essential resource for anyone interested in the development of astronomical spectroscopy. This work has been selected by scholars as being culturally important, and is part of the knowledge base of civilization as we know it. This work was reproduced from the original artifact, and remains as true to the original work as possible. Therefore, you will see the original copyright references, library stamps (as most of these works have been housed in our most important libraries around the world), and other notations in the work. This work is in the public domain in the United States of America, and possibly other nations. Within the United States, you may freely copy and distribute this work, as no entity (individual or corporate) has a copyright on the body of the work. As a reproduction of a historical artifact, this work may contain missing or blurred pages, poor pictures, errant marks, etc. Scholars believe, and we concur, that this work is important enough to be preserved, reproduced, and made generally available to the public. We appreciate your support of the preservation process, and thank you for being an important part of keeping this knowledge alive and relevant.
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