Joannis Kepleri astronomi Opera omnia: Joannis Kepleri astronomi Opera omnia

Frisch, Christian; Kepler, Johannes

Bibliographic data

Monograph

Persistent identifier:: 1067490280

Title:: Systems for data processing, anaylsis and representation

Sub title:: ISPRS Commission II Symposium : June 6 - 10, Ottawa, Canada

Scope:: 1 Online-Ressource (XX, 530 Seiten)

Year of publication:: 1994

Place of publication:: Ottawa

Publisher of the original:: The Surveys, Mapping and Remote Sensing, Natural Resources Canada

Identifier (digital):: 1067490280

Illustration:: Illustrationen

Signature of the source:: ZS 312(30,2)

Language:: English

Additional Notes:: Erscheinungsdatum des Originals ist aus dem Copyrightjahr ermittelt.

Usage licence:: Attribution 4.0 International (CC BY 4.0)

Editor:: Allam, Mosaad; Plunkett, Gordon

Corporations:: Symposium Systems for Data Processing, Analysis and Representation, 1994, Ottawa; International Society for Photogrammetry and Remote Sensing; International Society for Photogrammetry and Remote Sensing, Commission Instrumentation for Data Reduction and Analysis; Kanada, Surveys, Mapping and Remote Sensing Sector

Adapter:: Symposium Systems for Data Processing, Analysis and Representation, 1994, Ottawa; International Society for Photogrammetry and Remote Sensing; International Society for Photogrammetry and Remote Sensing, Commission Instrumentation for Data Reduction and Analysis; Kanada, Surveys, Mapping and Remote Sensing Sector

Founder of work:: Symposium Systems for Data Processing, Analysis and Representation, 1994, Ottawa; International Society for Photogrammetry and Remote Sensing; International Society for Photogrammetry and Remote Sensing, Commission Instrumentation for Data Reduction and Analysis; Kanada, Surveys, Mapping and Remote Sensing Sector

Other corporate:: Symposium Systems for Data Processing, Analysis and Representation, 1994, Ottawa; International Society for Photogrammetry and Remote Sensing; International Society for Photogrammetry and Remote Sensing, Commission Instrumentation for Data Reduction and Analysis; Kanada, Surveys, Mapping and Remote Sensing Sector

Publisher of the digital copy:: Technische Informationsbibliothek Hannover

Place of publication of the digital copy:: Hannover

Year of publication of the original:: 2019

Document type:: Monograph

Collection:: Earth sciences

Chapter

Title:: [Tuesday, June 7, 1994]

Document type:: Monograph

Structure type:: Chapter

Chapter

Title:: [Session D-1 Commission II - Special Project - Upgrading Photogrammetric Instruments]

Document type:: Monograph

Structure type:: Chapter

Chapter

Title:: Perfectionnement des instruments pphotogrammetriques [Patrick Wong]

Document type:: Monograph

Structure type:: Chapter

410 De Motibus Stellae Martis planetae justus, et I cum N connectatur. Quia ergo ut YD ad DF, sic XG ad GI (per 1.); ut vero VI) ad 1)11, sic XG ad GN, propter simili tudinem triangulorum: ut igitur FD ad DH, sic IG ad GN, et sunt aequales FDH et IGN. Aequales igitur etiam FHD et ING. Et H est centrum eccentrici, N vero centrum Solis. Angulus igitur (ffc. q. e. d. V. Anguli, quo coaequata fictitia, quae circulo nititur, differt a coae quata vera, quae ellipsi innititur, mensura genuina et verissima est rectan- gulum sub sinu anomaliae coaequatae fictitiae et sinu complementi ano maliae coaequatae verae. In schemate eodem, multiplicato sinu anguli AI1D in sinum anguli VFII, proditura erat genuina mensura anguli FHD per III. At per IV. angulorum YI 1 D et XNG aequalium sinus est idem, itemque et YFH, XIN sinus idem. Ergo multiplicato sinu anguli XNG, anomaliae coae quatae fictitiae, in sinum anguli XIN complementi ipsius XNI, qui est coaequata vera, prodit mensura genuimi anguli FI1 D; hoc est per IV. anguli ING, differentiae inter XNG et XNI. Corollarium. Quia paria est differentia ING, et nuspiam major 8 ', multo adhuc minor in effectu fiUura est differentia inter rectangula per XIN et per XGN sinum constituta. Hinc praxis liet ista. Dato angulo anomaliae coaequatae verae, multi plicetur ejus sinus in sinum complementi. Facti duplum, abjectis 5 ultimis, multiplicetur in maximum ingressus angulum ad anomaliam 45°. Prodibit angulus ingressus ad datam anomaliam. Qui additus ad coaequatam veram XNI, dat ffctitiam XNG. Per quem angulum et latera NH, HG nota invenitur AHG anomalia eccentri, et HGN valor trianguli, ut hactenus. Maximum vero angulum ad anomaliam 45° inquirere non est difficile. Sit VHD 45°. Ergo ut totus sinus ad 70711, sic 429 vel correctius 432 maximus ingressus, videlicet maxima latitudo lunulae, ad FD 315. Cumque jam in 45 u sint aequales I1V, YD; aufer FD 315 ab VD 70711, remanet VF, 70396, quae cum HV dat angulum YHF 44° 52' 19", qui differt a 45° 0' 0" tantum per 7' 41". Atque'hic est maximus angulus ING. 102 J Sequitur alter modus per analysin, cujus haec fundamenta sunt. In schemate 118. dato angulo MNL, datur proportio linearum MN, NL: et scio, quod MN et LN sint compositae ex partibus notae et permutatae proportionis. Nam in MN inest sinus totus, notus; in LN inest HN, eccentricitas nota. Residuum de MN ad residuum de LN, hoc est ad LH, eam habet proportionem, quam habet eccentricitas HN ad sinum totum. (Vide, si mavis, etiam schema 117.) Ergo sit MN 100000 —j— 1 Hr, LN «* angulo MNL 30° «ft 2—G * 6 ^ * NH 9265 vel ut sit HL J—J“« 1L Ut vero HN 9265 ad 1 V, sic 100000 ad LII. Igitur IIL secunda vice est id est V; prius 7733800000 f 86603 100000 1 L Ablatis denominatoribus, et quae possunt utrinque aequaliter auferri, restant 992717 aequales numero 7733800000. Itaque una radix valet 7744, estque MN 107744. Et quia ut HN ad hanc radicem, sic totus ad LH, erit igitur LH 83583, sinus ipsius KE 56° 42' complementi anomaliae eccentri AK 33° 46'. ,o:! ) Qua inventa, jam ut paulo prius invenitur et area AKN, mensura temporis seu anomalia

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