Född Kurkslätts socken i Finland d. 2 april 1779.
Militär, tecknare. Föräldrar: kapellanen Mikael Thersner och Johanna Dorph. - T. begynte redan vid sju års ålder sin militära bana, i det han då vardt antagen till skeppsgosse, i hvilken egenskap han tjänstgjorde under ryska kriget 1788-90. Sergeant vid arméns flotta 1794 och fänrik 1799, var han såsom informationsofficer vid Göteborgs eskader 1804 anställd att förrätta hydrografiska mätningar i Bohuslän. 1808 löjtnant i Fältmätningskåren, dit han blifvit förflyttad året förut, deltog han på skilda håll krigsoperationerna 1808-09, blef kapten 1810 och medverkade s. å. vid gränsregleringen mellan Sverige och Ryssland. Sedan han i 1813-14 års krig haft åtskilliga kommenderingar och sistnämnda år befordrats till major i Fältmätningsbrigaden, förrättade han bl. a. 1815-17 fältmätningar i Skåne. 1825 tog han afsked ur krigstjänsten med öfverstlöjtnants rang. - Bland elementen i hans ungdomsbildning hörde bl. a. att med grafstickeln frambringa åtskilliga småstycken. På egen hand förkofrade han sig gradvis i tecknin...
Bland arbeten.
Fordna och närvarande Sverige
Svenskt biografiskt handlexikon.Nordisk Familjebok, första utgåvan.
1600-1684.
One of Sweden's first surveyors. Worked in the provinces of Östergötland and Värmland.
Jean de Rogier (1600-84) var en produktiv och skicklig lantmätare. Han föddes i Frankrike men var från l630-talet verksam som lantmätare, huvudsakligen i Östergötland. Under perioden 1636-50 utgav han geometriska kartor över Norrköpings stad,bergslagen Vånga, Hällestad, Tjällmo och Godegård samt häraderna Östkind, Bråbo, Björkekind, Memming och Hammarkind.
Rogier fortsatte sedan med en geografisk kartläggning av landskapet. Fyra delar i skala ca 1:50 000 utgavs:
Östanstång, landskapet mellan Stångån, Motala ström, Östersjön och Småland (1653).
Västanstång, Östgötaslätten väster om Stångån (1657). Originalet finns i Stifts- och landsbiblioteket i Linköping. En andra upplaga utkom 1660.
Ydre och Kinda härader (1660), omfattar även de sydligaste delarna av Hanekinds, Valkebo, Vifolka och Göstrings härader. (Ydre och Kinda härader hade så sent som 1645 införlivats med Östergötlands län.)
Bergslagen, dv...
Sveriges sjökartor – A. Hedin.
1779-1868.
Son till Fredrik A. Akrel. Militär, kopparstickare, f. 13 jan. 1779 i Stockholm, inskrefs 1793 i Landtmäterikontoret, men öfvergick snart till Fortifikationen, där han 1796 utnämndes till konduktör. Under de följande tio åren utmärkte han sig som ingenjör vid åtskilliga viktiga arbeten, såsom Trollhätte (gamla) kanal- och slussverksbyggnad samt befästningsarbetena i Stockholms skärgård och vid Stralsund. 1806 fick han löjtnants grad vid den då inrättade Fältmätningskåren samt utnämndes 1807 till kapten i armén och lärare i fortifikation vid krigsakademien på Karlberg. På sistnämnda post inlade han genom förträffliga föreläsningar och afhandlingar stor förtjänst om den svenska militärbildningen. En öfversättning af hans Föreläsningar i fortifikation (1811) nyttjades en tid äfven vid militärskolorna i Ryssland. 1812 befordrades han till major i armén. Under Karl Johan deltog han såsom öfveradjutant i 1813 års tyska fälttåg mot Napoleon och var med i slagen vid Grossbeeren, Dennewitz och Leipzig, där han vid sto...
Bland arbeten.
Fordna och närvarande Sverige.
Voyage pittoresque au Cap Nord.
Resa i Propontiden.
Bref om Förenta staterna.
Reise durch Schweden.
Nordisk Familjebok, Uggleupplagan.
Amiral Häggs flaggkarta. - Stockholm 1888.
'Süd-Amerika in 6 Blättern.' - A. Petermann.
"The Mapping of Mars."
by Peter J. K. Louwman.
Amateur astronomer, Louwman Collection of Historic Telescopes, Wassenaar, The Netherlands.
The most familiar type of globe is the terrestrial one. Also familiar, but less common is the celestial. For a true globe collector it is most desirable, of course, to own a pair of these globes, identical in size, by the same maker. For me, as an enthusiastic amateur astronomer, two even rarer types of globe have always attracted me: globes of the Moon and of Mars. Technically, these globes share many details with the terrestrial globe, but they offer some curious differences worth looking at.
A Moon globe that was published before the time of the “Space Age”, for instance, shows us surface details as seen with the help of a telescope, of only one half of the Moon. The other half was blank, because no surface details could be observed. This is due to the fact that the Moon, during its revolution around the Earth in one month, always presents the same side of its surface towards the Earth.
When the first spacecrafts made the voyages to, and later travelled around the Moon, the features of the hidden side could be charted. The first pictures of that part of the surface were successfully made by the Russian “Luna 3” in October 1959. This led to the production of Moon globes with all details of the entire surface by publishers in the U.S.A., Russia and elsewhere. Ever since the discovery of the telescope, the surface of the planet Mars has been observed intensively. At first, only crude sketches of surface detail were all that could be achieved. Later on, with better telescopes and observing techniques, more and more details could be charted.
Unlike the Moon, Mars rotated in about 24 ½ hours and thus gradually presents its entire surface towards the Earth. Observations made at intervals enables astronomers to compile maps of the whole surface. Consequently, it was possible to convert the surface details of the two-dimensional maps onto the three-dimensional surface of a sphere to create a Mars globe.
A further important difference between the Moon and Mars is that where the surface characteristics of the Moon are permanent, those of Mars change with time. The reason for this difference lies in the fact that Mars has an atmosphere and the Moon does not. Winds and dust storms on Mars constantly change the appearance of certain parts of its surface. Well-known temporary changes occur at the with-capped North and South poles, which change dramatically in size during the cycle of seasons of approximately 687 days. The polar caps consist of water ice and carbon dioxide. In the summer season of the northern hemisphere for instance, the cap on the North Pole shrinks to a very small area, while that of the South Pole increases. These changes are due to the evaporation and sublimation of carbon dioxide in particular. On modern Mars globes the polar caps are illustrated at their minimum size so that no surface features are hidden under the caps.
To modern astronomers , familiar only with the beautifully illustrated Mars maps compiled from the information gathered by Mars space missions, it might come as an unexpected, perhaps even annoying, surprise that old maps and globes show the North Pole at the bottom and the South Pole at the top. The explanation for this representation lies in the fact that astronomical telescopes give an inverted image: “up” and “down” are viewed as “down” and “up”.
As a matter of fact all old astronomical books, maps and journal publication (until around 1960, but in some cases after that year also) always illustrate pictures of heavenly bodies upside-down. This is also the case with drawings, maps and photographs of stellar objects like stars and nebulae. Why bother to turn it around, astronomers reason, when the inverted image is the way one actually sees and observes it through a telescope?
To me, a Mars globe with the traditional astronomical orientation is very appealing. Recently, I was lucky enough to acquire one; this globe is a product of a tremendously interesting period in Mars research and I was very glad to add it to my private collection of astronomical objects of historical significance and cultural importance.
This Mars globe was made by Ingeborg Brun of Norway in about 1920. For the making of it, she used information that is entirely based on the work of the famous American astronomer Percival Lowell. Lowell built his observatory in Flagstaff, Arizona in 1895 and devoted much of his time and money to observing Mars and doing research on its canals, which were at that time very popular with the general public.
Unfortunately, Lowell’s world-famous observations of the canals and of the supposedly seasonal growth of vegetation along them eventually proved to be caused by optical illusions. On modern pictures obtained by space probes, nothing resembling “canals” has ever been found, nor any clues to water on the planet’s surface. Nor have the Mars landers found any additional clues.
Nevertheless, the research of Lowell and others, undertaken some 100 years ago now, belongs to a short but very fascinating period in astronomical research.
Gazing at my wonderfully detailed and exquisite Lowell Mars glob continues to impress me and helps me to understand this fascinating period of astronomy and globe it produced.
Christie’s, London. Fine Globes and Planetaria, Tuesday 5 November 2002.