A new set of logarithmic solar tables, calculated and constructed for determining the latitude at sea, By Taking Two Altitudes of the Sun, with the intermediate Time, by a common Watch; and that with Ease and Accuracy, independent of the Sun's meridional Altitude. This most excellent and useful Performance, not only produces the true Latitude at any Time between Nine O'Clock in the Morning, and Three in the Afternoon; but also gives the true Time of the Day, when the greatest Altitude was taken, to twenty Seconds; and if greater Accuracy is required, proportional Parts may be taken. Whence the Sun's Azimuth may be determined by one single Proportion. To which is added, a complete theory, illustrating the rationale of this most useful discovery
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| Sprache: | English |
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London
printed for J. Mount, T. Page, W. Mount, and T. Page, on Tower-Hill
M,DCC,LXXXI. [1781]
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| Ausgabe: | The sixth edition, with the tables enlarged |
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| 130 | 0 | |a New sett of logarithmic solar tables | |
| 245 | 1 | 0 | |a A new set of logarithmic solar tables, calculated and constructed for determining the latitude at sea, By Taking Two Altitudes of the Sun, with the intermediate Time, by a common Watch; and that with Ease and Accuracy, independent of the Sun's meridional Altitude. This most excellent and useful Performance, not only produces the true Latitude at any Time between Nine O'Clock in the Morning, and Three in the Afternoon; but also gives the true Time of the Day, when the greatest Altitude was taken, to twenty Seconds; and if greater Accuracy is required, proportional Parts may be taken. Whence the Sun's Azimuth may be determined by one single Proportion. To which is added, a complete theory, illustrating the rationale of this most useful discovery |
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| id | DE-604.BV049222136 |
| illustrated | Not Illustrated |
| index_date | 2024-09-19T15:57:26Z |
| indexdate | 2024-09-27T17:03:59Z |
| institution | BVB |
| language | English |
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| oclc_num | 1422373710 |
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| physical | Online-Ressource (38Seiten) 4° |
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| publishDate | 1781 |
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| publishDateSort | 1781 |
| publisher | printed for J. Mount, T. Page, W. Mount, and T. Page, on Tower-Hill |
| record_format | marc |
| spellingShingle | A new set of logarithmic solar tables, calculated and constructed for determining the latitude at sea, By Taking Two Altitudes of the Sun, with the intermediate Time, by a common Watch; and that with Ease and Accuracy, independent of the Sun's meridional Altitude. This most excellent and useful Performance, not only produces the true Latitude at any Time between Nine O'Clock in the Morning, and Three in the Afternoon; but also gives the true Time of the Day, when the greatest Altitude was taken, to twenty Seconds; and if greater Accuracy is required, proportional Parts may be taken. Whence the Sun's Azimuth may be determined by one single Proportion. To which is added, a complete theory, illustrating the rationale of this most useful discovery Logarithms Navigation |
| title | A new set of logarithmic solar tables, calculated and constructed for determining the latitude at sea, By Taking Two Altitudes of the Sun, with the intermediate Time, by a common Watch; and that with Ease and Accuracy, independent of the Sun's meridional Altitude. This most excellent and useful Performance, not only produces the true Latitude at any Time between Nine O'Clock in the Morning, and Three in the Afternoon; but also gives the true Time of the Day, when the greatest Altitude was taken, to twenty Seconds; and if greater Accuracy is required, proportional Parts may be taken. Whence the Sun's Azimuth may be determined by one single Proportion. To which is added, a complete theory, illustrating the rationale of this most useful discovery |
| title_alt | New sett of logarithmic solar tables |
| title_auth | A new set of logarithmic solar tables, calculated and constructed for determining the latitude at sea, By Taking Two Altitudes of the Sun, with the intermediate Time, by a common Watch; and that with Ease and Accuracy, independent of the Sun's meridional Altitude. This most excellent and useful Performance, not only produces the true Latitude at any Time between Nine O'Clock in the Morning, and Three in the Afternoon; but also gives the true Time of the Day, when the greatest Altitude was taken, to twenty Seconds; and if greater Accuracy is required, proportional Parts may be taken. Whence the Sun's Azimuth may be determined by one single Proportion. To which is added, a complete theory, illustrating the rationale of this most useful discovery |
| title_exact_search | A new set of logarithmic solar tables, calculated and constructed for determining the latitude at sea, By Taking Two Altitudes of the Sun, with the intermediate Time, by a common Watch; and that with Ease and Accuracy, independent of the Sun's meridional Altitude. This most excellent and useful Performance, not only produces the true Latitude at any Time between Nine O'Clock in the Morning, and Three in the Afternoon; but also gives the true Time of the Day, when the greatest Altitude was taken, to twenty Seconds; and if greater Accuracy is required, proportional Parts may be taken. Whence the Sun's Azimuth may be determined by one single Proportion. To which is added, a complete theory, illustrating the rationale of this most useful discovery |
| title_exact_search_txtP | A new set of logarithmic solar tables, calculated and constructed for determining the latitude at sea, By Taking Two Altitudes of the Sun, with the intermediate Time, by a common Watch; and that with Ease and Accuracy, independent of the Sun's meridional Altitude. This most excellent and useful Performance, not only produces the true Latitude at any Time between Nine O'Clock in the Morning, and Three in the Afternoon; but also gives the true Time of the Day, when the greatest Altitude was taken, to twenty Seconds; and if greater Accuracy is required, proportional Parts may be taken. Whence the Sun's Azimuth may be determined by one single Proportion. To which is added, a complete theory, illustrating the rationale of this most useful discovery |
| title_full | A new set of logarithmic solar tables, calculated and constructed for determining the latitude at sea, By Taking Two Altitudes of the Sun, with the intermediate Time, by a common Watch; and that with Ease and Accuracy, independent of the Sun's meridional Altitude. This most excellent and useful Performance, not only produces the true Latitude at any Time between Nine O'Clock in the Morning, and Three in the Afternoon; but also gives the true Time of the Day, when the greatest Altitude was taken, to twenty Seconds; and if greater Accuracy is required, proportional Parts may be taken. Whence the Sun's Azimuth may be determined by one single Proportion. To which is added, a complete theory, illustrating the rationale of this most useful discovery |
| title_fullStr | A new set of logarithmic solar tables, calculated and constructed for determining the latitude at sea, By Taking Two Altitudes of the Sun, with the intermediate Time, by a common Watch; and that with Ease and Accuracy, independent of the Sun's meridional Altitude. This most excellent and useful Performance, not only produces the true Latitude at any Time between Nine O'Clock in the Morning, and Three in the Afternoon; but also gives the true Time of the Day, when the greatest Altitude was taken, to twenty Seconds; and if greater Accuracy is required, proportional Parts may be taken. Whence the Sun's Azimuth may be determined by one single Proportion. To which is added, a complete theory, illustrating the rationale of this most useful discovery |
| title_full_unstemmed | A new set of logarithmic solar tables, calculated and constructed for determining the latitude at sea, By Taking Two Altitudes of the Sun, with the intermediate Time, by a common Watch; and that with Ease and Accuracy, independent of the Sun's meridional Altitude. This most excellent and useful Performance, not only produces the true Latitude at any Time between Nine O'Clock in the Morning, and Three in the Afternoon; but also gives the true Time of the Day, when the greatest Altitude was taken, to twenty Seconds; and if greater Accuracy is required, proportional Parts may be taken. Whence the Sun's Azimuth may be determined by one single Proportion. To which is added, a complete theory, illustrating the rationale of this most useful discovery |
| title_short | A new set of logarithmic solar tables, calculated and constructed for determining the latitude at sea, By Taking Two Altitudes of the Sun, with the intermediate Time, by a common Watch; and that with Ease and Accuracy, independent of the Sun's meridional Altitude. This most excellent and useful Performance, not only produces the true Latitude at any Time between Nine O'Clock in the Morning, and Three in the Afternoon; but also gives the true Time of the Day, when the greatest Altitude was taken, to twenty Seconds; and if greater Accuracy is required, proportional Parts may be taken. Whence the Sun's Azimuth may be determined by one single Proportion. To which is added, a complete theory, illustrating the rationale of this most useful discovery |
| title_sort | a new set of logarithmic solar tables calculated and constructed for determining the latitude at sea by taking two altitudes of the sun with the intermediate time by a common watch and that with ease and accuracy independent of the sun s meridional altitude this most excellent and useful performance not only produces the true latitude at any time between nine o clock in the morning and three in the afternoon but also gives the true time of the day when the greatest altitude was taken to twenty seconds and if greater accuracy is required proportional parts may be taken whence the sun s azimuth may be determined by one single proportion to which is added a complete theory illustrating the rationale of this most useful discovery |
| topic | Logarithms Navigation |
| topic_facet | Logarithms Navigation |
| url | http://nl.sub.uni-goettingen.de/id/1077800600?origin=/collection/nlh-ecc |
| work_keys_str_mv | UT newsettoflogarithmicsolartables |