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John August Anderson

John August Anderson (August 7, 1876 – December 2, 1959) was an American astronomer who made significant contributions to improving astronomical instruments in the early 20th century, especially diffraction gratings.

Biography edit

John August Anderson was born on August 7, 1876, in Rollag, Minnesota, a small unincorporated community in Clay County. He was the sixth child of Brede Andersen and Elen Martha Brevik .[1]

After completing his early education, Anderson attended Concordia College in Moorhead, Minnesota, from 1891 to 1893. He then pursued further studies at Minnesota State University Moorhead (formerly Moorhead Normal School) from 1893 to 1894. In January 1899, he enrolled at Valparaiso University in Indiana, where he obtained a B.S. degree in August 1900.[1]

Following the completion of his undergraduate degree, Anderson served as a teacher until 1904 when he decided to further his education. He enrolled at Johns Hopkins University, where he pursued graduate studies under the direction of Professor Joseph Sweetman Ames, on the Absorption and Emission Spectra of Neodymium and Erbium Compounds.[1][2] After receiving his PhD in 1907 he stayed at Johns Hopkins and became a professor of astronomy in 1908. He continued research on absorption and emission spectra and “was requested to take charge of the ruling engine constructed by Henry Rowland, the great American pioneer in spectroscopy. Anderson refined Rowland's machine to produce gratings of even finer resolving power”[2] and continued their production, as high quality diffraction gratings were in high demand during that time. In 1912 at the request of George E. Hale he took a one year leave of absence from Johns Hopkins to supervise and assist with the construction of a large ruling engine at the Mt. Wilson observatory. In 1913 he returned to Johns Hopkins, but in 1916, he left to work at Mt. Wilson. His most notable contribution was his adaptation of the Michelson's interferometer technique for measuring close double stars. He used a rotating mask at the focus to measure the separation of Capella.[1] In the 1920s, he collaborated with Harry O. Wood to develop the Wood–Anderson seismometer.[3] In 1928 after the California Institute of Technology received funds for the building of the 200-inch Palomar telescope he was asked by Hale to serve as executive officer of the newly formed Observatory Council, whose charge was to oversee all aspects of the project. Over the next twenty years, Anderson directed and participated in site selection, design and testing of the 200-inch mirror, the establishment and operation of an on-site optical shop, and the design and testing of the telescope structure and, especially, its instrumentation.[4] Anderson remained head of the Observatory Council up to the time of the telescope's dedication, in June 1948.[2]

He died on December 2, 1959, at the age of 83 in Altadena, California.[1] The crater Anderson on the Moon is named in his memory.

He was awarded the Franklin Institute's Howard N. Potts Medal in 1924.[5]

Bibliography edit

Unless otherwise noted, the following publications were by John A. Anderson.

  • "On the Application of the Laws of Refraction in Interpreting Solar Phenomena", Astrophysical Journal, vol. 31, 1910.
  • "A method of investigating the Stark effect for metals, with results for chromium", 1917.
  • "The vacuum spark spectrum of calcium", 1924.
  • "The Use of Long Focus Concave Gratings at Eclipses", Publications of the Astronomical Society of the Pacific, Vol. 38, 1926.
  • J. A. Anderson and Russell W. Porter, "Ronchi's Method of Optical Testing", Astrophysical Journal, vol. 70, 1929.
  • "Spectral energy-distribution of the high-current vacuum tube", 1932.
  • "On the application of Michelson's interferometer method to the measurement of close double stars", Astrophysical Journal, vol. 51, June 1920.
  • "Optics of the 200-inch Hale Telescope", Publications of the Astronomical Society of the Pacific, Vol. 60, 1948.

References edit

  1. ^ a b c d e Bowen, Ira S. (1962). "John August Anderson 1876–1959" (PDF). Biographical Memoir. National Academy of Sciences, Washington D.C. Retrieved 20 May 2023.
  2. ^ a b c "Guide to the Papers of John A. Anderson, 1914-1951". oac.cdlib.org. Retrieved 2023-05-22.
  3. ^ "THE TORSION SEISMOMETER". www.eas.slu.edu. Retrieved 2023-05-22.
  4. ^ Anderson, John A. (1948). "Optics of the 200-inch Hale Telescope". Publications of the Astronomical Society of the Pacific. 60: 221. doi:10.1086/126043. S2CID 121078506. Retrieved 2023-05-22.
  5. ^ . 2014-05-02. Archived from the original on 2014-05-02. Retrieved 2023-05-22.

john, august, anderson, august, 1876, december, 1959, american, astronomer, made, significant, contributions, improving, astronomical, instruments, early, 20th, century, especially, diffraction, gratings, biography, edit, born, august, 1876, rollag, minnesota,. John August Anderson August 7 1876 December 2 1959 was an American astronomer who made significant contributions to improving astronomical instruments in the early 20th century especially diffraction gratings Biography editJohn August Anderson was born on August 7 1876 in Rollag Minnesota a small unincorporated community in Clay County He was the sixth child of Brede Andersen and Elen Martha Brevik 1 After completing his early education Anderson attended Concordia College in Moorhead Minnesota from 1891 to 1893 He then pursued further studies at Minnesota State University Moorhead formerly Moorhead Normal School from 1893 to 1894 In January 1899 he enrolled at Valparaiso University in Indiana where he obtained a B S degree in August 1900 1 Following the completion of his undergraduate degree Anderson served as a teacher until 1904 when he decided to further his education He enrolled at Johns Hopkins University where he pursued graduate studies under the direction of Professor Joseph Sweetman Ames on the Absorption and Emission Spectra of Neodymium and Erbium Compounds 1 2 After receiving his PhD in 1907 he stayed at Johns Hopkins and became a professor of astronomy in 1908 He continued research on absorption and emission spectra and was requested to take charge of the ruling engine constructed by Henry Rowland the great American pioneer in spectroscopy Anderson refined Rowland s machine to produce gratings of even finer resolving power 2 and continued their production as high quality diffraction gratings were in high demand during that time In 1912 at the request of George E Hale he took a one year leave of absence from Johns Hopkins to supervise and assist with the construction of a large ruling engine at the Mt Wilson observatory In 1913 he returned to Johns Hopkins but in 1916 he left to work at Mt Wilson His most notable contribution was his adaptation of the Michelson s interferometer technique for measuring close double stars He used a rotating mask at the focus to measure the separation of Capella 1 In the 1920s he collaborated with Harry O Wood to develop the Wood Anderson seismometer 3 In 1928 after the California Institute of Technology received funds for the building of the 200 inch Palomar telescope he was asked by Hale to serve as executive officer of the newly formed Observatory Council whose charge was to oversee all aspects of the project Over the next twenty years Anderson directed and participated in site selection design and testing of the 200 inch mirror the establishment and operation of an on site optical shop and the design and testing of the telescope structure and especially its instrumentation 4 Anderson remained head of the Observatory Council up to the time of the telescope s dedication in June 1948 2 He died on December 2 1959 at the age of 83 in Altadena California 1 The crater Anderson on the Moon is named in his memory He was awarded the Franklin Institute s Howard N Potts Medal in 1924 5 Bibliography editUnless otherwise noted the following publications were by John A Anderson On the Application of the Laws of Refraction in Interpreting Solar Phenomena Astrophysical Journal vol 31 1910 A method of investigating the Stark effect for metals with results for chromium 1917 The vacuum spark spectrum of calcium 1924 The Use of Long Focus Concave Gratings at Eclipses Publications of the Astronomical Society of the Pacific Vol 38 1926 J A Anderson and Russell W Porter Ronchi s Method of Optical Testing Astrophysical Journal vol 70 1929 Spectral energy distribution of the high current vacuum tube 1932 On the application of Michelson s interferometer method to the measurement of close double stars Astrophysical Journal vol 51 June 1920 Optics of the 200 inch Hale Telescope Publications of the Astronomical Society of the Pacific Vol 60 1948 References edit a b c d e Bowen Ira S 1962 John August Anderson 1876 1959 PDF Biographical Memoir National Academy of Sciences Washington D C Retrieved 20 May 2023 a b c Guide to the Papers of John A Anderson 1914 1951 oac cdlib org Retrieved 2023 05 22 THE TORSION SEISMOMETER www eas slu edu Retrieved 2023 05 22 Anderson John A 1948 Optics of the 200 inch Hale Telescope Publications of the Astronomical Society of the Pacific 60 221 doi 10 1086 126043 S2CID 121078506 Retrieved 2023 05 22 The Franklin Institute Awards Laureate Search 2014 05 02 Archived from the original on 2014 05 02 Retrieved 2023 05 22 Retrieved from https en wikipedia org w index php title John August Anderson amp oldid 1213179467, wikipedia, wiki, book, books, library,

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