After college, Rowland worked for the Western New York railway, but he did not like the work. He became an instructor in natural science at the
University of Wooster in
Wooster, Ohio. He resigned in order to return to Troy as assistant professor of physics at Rensselaer. Rowland was considered one of the most brilliant American scientists of his day. However, initially his merits were not perceived in his own country. He was unable to secure the publication of many of his early scientific papers; but
James Clerk Maxwell at once saw their excellence, and had them printed in
Philosophical Magazine. When the managers of
Johns Hopkins University in
Baltimore,
Maryland, asked advice in Europe as to whom they should make their professor of physics, Rowland was overwhelmingly recommended as the best choice. In 1876, he became the first occupant of the chair of physics at Johns Hopkins University, a position which he retained until his death in Baltimore on April 16, 1901. In the interval between his selection to Johns Hopkins and the assumption of his duties there, he studied physics under
Hermann von Helmholtz in Berlin (1875–76), and carried out a well-known research on the effect of an electrically charged body in motion, showing it to give rise to a magnetic field. After settling in Baltimore, Rowland focused on two important pieces of work. One was a redetermination of the
ohm. For this he obtained a value which was substantially different from that ascertained by the committee of the
British Association appointed for the purpose, but ultimately he had the satisfaction of seeing his own result accepted as the more correct of the two. The other was a new determination of the mechanical equivalent of heat. In this he used
J. P. Joule's paddle-wheel method, though with many improvements, the whole apparatus being on a larger scale and the experiments being conducted over a wider range of temperature. He obtained a result distinctly higher than Joule's final figure. Additionally, he made many valuable observations on the thermodynamics involved, and on the variation of the specific heat of water, which Joule had assumed to be the same at all temperatures. In 1882, before the
Physical Society of London, Rowland gave a description of the
diffraction gratings, with which his name is specially associated, and which have been of enormous advantage to astronomical spectroscopy. These gratings consist of pieces of metal or glass ruled by means of a diamond point with a very large number of parallel lines, on the extreme accuracy of which their efficiency depends. For their production, therefore, dividing engines of extraordinary trueness and delicacy were required, and in the construction of such machines Rowland's engineering skill brought him conspicuous success. The results of his labors may be found in the elaborate
Photographic Map of the Normal Solar Spectrum (1888) and the
Table of Solar Wave-Lengths (1898). In his later years, Rowland was engaged in developing a system of multiplex
telegraphy. He authored
A Plea for Pure Science, in 1883 an important document for the understanding of the relationship between science in university and in commercial contexts in the late nineteenth and early twentieth century. ==Honors and awards==