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The celestial mechanics approach : theoretical foundations / Gerhard Beutler in Journal of geodesy, vol 84 n° 10 (October 2010)
[article]
Titre : The celestial mechanics approach : theoretical foundations Type de document : Article/Communication Auteurs : Gerhard Beutler, Auteur ; Adrian Jäggi, Auteur ; L. Mervart, Auteur ; U. Meyer, Auteur Année de publication : 2010 Article en page(s) : pp 605 - 624 Note générale : Bibliographie Langues : Anglais (eng) Descripteur : [Vedettes matières IGN] Géodésie physique
[Termes IGN] antenne GPS
[Termes IGN] champ de pesanteur terrestre
[Termes IGN] constellation GPS
[Termes IGN] mécanique orbitale
[Termes IGN] orbitographieRésumé : (Auteur) Gravity field determination using the measurements of Global Positioning receivers onboard low Earth orbiters and inter-satellite measurements in a constellation of satellites is a generalized orbit determination problem involving all satellites of the constellation. The celestial mechanics approach (CMA) is comprehensive in the sense that it encompasses many different methods currently in use, in particular so-called short-arc methods, reduced-dynamic methods, and pure dynamic methods. The method is very flexible because the actual solution type may be selected just prior to the combination of the satellite-, arc- and technique-specific normal equation systems. It is thus possible to generate ensembles of substantially different solutions - essentially at the cost of generating one particular solution. The article outlines the general aspects of orbit and gravity field determination. Then the focus is put on the particularities of the CMA, in particular on the way to use accelerometer data and the statistical information associated with it. Numéro de notice : A2010-417 Affiliation des auteurs : non IGN Thématique : POSITIONNEMENT Nature : Article nature-HAL : ArtAvecCL-RevueIntern DOI : 10.1007/s00190-010-0401-7 Date de publication en ligne : 24/08/2010 En ligne : https://doi.org/10.1007/s00190-010-0401-7 Format de la ressource électronique : URL article Permalink : https://documentation.ensg.eu/index.php?lvl=notice_display&id=30610
in Journal of geodesy > vol 84 n° 10 (October 2010) . - pp 605 - 624[article]Réservation
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Code-barres Cote Support Localisation Section Disponibilité 266-2010101 SL Revue Centre de documentation Revues en salle Disponible A study of trajectory models for satellite image triangulation / Inseong Jeong in Photogrammetric Engineering & Remote Sensing, PERS, vol 76 n° 3 (March 2010)
[article]
Titre : A study of trajectory models for satellite image triangulation Type de document : Article/Communication Auteurs : Inseong Jeong, Auteur ; J. Bethel, Auteur Année de publication : 2010 Article en page(s) : pp 265 - 276 Note générale : Bibliographie Langues : Anglais (eng) Descripteur : [Vedettes matières IGN] Acquisition d'image(s) et de donnée(s)
[Termes IGN] image ALOS-PRISM
[Termes IGN] image EO1-Hyperion
[Termes IGN] image EROS
[Termes IGN] image Quickbird
[Termes IGN] image SPOT-HRV
[Termes IGN] image Terra-ASTER
[Termes IGN] implémentation (informatique)
[Termes IGN] orbite
[Termes IGN] point d'appui
[Termes IGN] spatiotriangulationRésumé : (Auteur) Many spaceborne imagery products are provided with metadata or support data having diverse types, representations, frequencies, and conventions. According to the variability of metadata, a compatible physical sensor model approach must be constructed. Among the three component of the sensor model, i.e., trajectory model, projection equations, and parameter subset selection, the construction of the position and attitude trajectory is closely linked with the availability and type of support data. In this paper, we show how trajectory models can be implemented based on support data from six satellite image types: QuickBird, Hyperion, SPOT-3, ASTER. PRISM, and EROS-A. Triangulation for each image is implemented to investigate the feasibility and suitability of the different trajectory models. The results show the effectiveness of some of the simple models while indicating that careful use of dense ephemeris information is necessary. These results are based on having a number of high quality ground control points. Copyright ASPRS Numéro de notice : A2010-088 Affiliation des auteurs : non IGN Thématique : IMAGERIE Nature : Article DOI : 10.14358/PERS.76.3.265 En ligne : https://doi.org/10.14358/PERS.76.3.265 Format de la ressource électronique : URL article Permalink : https://documentation.ensg.eu/index.php?lvl=notice_display&id=30284
in Photogrammetric Engineering & Remote Sensing, PERS > vol 76 n° 3 (March 2010) . - pp 265 - 276[article]Annuaire du Bureau des longitudes, Guide de données astronomiques 2011 pour l'observation du ciel / Bureau des longitudes (2010)
Titre : Annuaire du Bureau des longitudes, Guide de données astronomiques 2011 pour l'observation du ciel : calendriers, soleil, lune, planètes, astéroïdes, satellites, comètes, étoiles Type de document : Dictionnaire / Usuel Auteurs : Bureau des longitudes, Auteur Editeur : Les Ulis : EDP Sciences Année de publication : 2010 Importance : 371 p. Format : 15 x 24 cm ISBN/ISSN/EAN : 978-2-7598-0541-9 Langues : Français (fre) Descripteur : [Vedettes matières IGN] Astronomie fondamentale
[Termes IGN] astéroïde
[Termes IGN] calendrier
[Termes IGN] comète
[Termes IGN] coordonnées astronomiques
[Termes IGN] éphémérides astronomiques
[Termes IGN] étoile
[Termes IGN] Lune
[Termes IGN] planète
[Termes IGN] satellite galiléen
[Termes IGN] soleil (étoile)Résumé : (Editeur) Destiné aux astronomes, professionnels ou amateurs, cet ouvrage se décompose de la façon suivante : Les trois premiers chapitres de cet ouvrage contiennent : les données sur les différents calendriers et leur concordance, les fêtes légales en France, les différentes échelles de temps, les dates de décrets sur les heures légales en France métropolitaine parues au Journal Officiel depuis 1916 ; des notions nécessaires à la compréhension et à l'emploi des éphémérides contenues dans l'ouvrage. Les chapitres suivants fournissent des éphémérides astronomiques : les positions du Soleil et de la Lune ; les positions des planètes et de leurs satellites ; les positions des astéroïdes et des comètes ; les explications et des données pour l'observation de la surface du Soleil, de la Lune et des planètes ; des cartes du ciel, une liste de constellations et les positions et occultations des étoilés ; des données sur les éclipses de Soleil et de Lune et sur les phénomènes astronomiques ; la liste des observatoires astronomiques les plus connus. Numéro de notice : 20497 Affiliation des auteurs : non IGN Thématique : POSITIONNEMENT Nature : Usuel En ligne : https://gallica.bnf.fr/ark:/12148/bpt6k9614055r?rk=21459;2 Format de la ressource électronique : URL Permalink : https://documentation.ensg.eu/index.php?lvl=notice_display&id=34939 Global gravity field determination using the GPS measurements made onboard the low Earth orbiting satellite CHAMP / Lars Prange (2010)
Titre : Global gravity field determination using the GPS measurements made onboard the low Earth orbiting satellite CHAMP Type de document : Rapport Auteurs : Lars Prange, Auteur Editeur : Zurich : Schweizerischen Geodatischen Kommission / Commission Géodésique Suisse Année de publication : 2010 Collection : Geodätisch-Geophysikalische Arbeiten in der Schweiz, ISSN 0257-1722 num. 81 Importance : 212 p. Format : 21 x 30 cm ISBN/ISSN/EAN : 978-3-908440-25-3 Note générale : Bibliographie Langues : Anglais (eng) Descripteur : [Vedettes matières IGN] Géodésie physique
[Termes IGN] champ de pesanteur terrestre
[Termes IGN] données CHAMP
[Termes IGN] données GPS
[Termes IGN] Global Positioning System
[Termes IGN] gravimétrie spatiale
[Termes IGN] modèle de géopotentiel
[Termes IGN] orbite basse
[Termes IGN] orbitographie
[Termes IGN] positionnement par GPS
[Termes IGN] validation des données
[Termes IGN] variation saisonnièreIndex. décimale : 30.40 Géodésie physique Résumé : (Auteur) The major goal of this work was to to generate "the best possible" static CHAMP-only gravity field model using most of the openly available CHAMP data. Firstly we wanted to assess the full potential but also the limitations of CHAMP data and a CHAMP-like satellite mission for gravity field determination. Secondly we wanted to gain as much insight as possible in determining gravity fields (static and time variable) from space-based GNSS data in general, because several current and future satellite missions (dedicated to gravity field research, but also non-dedicated) equipped with GNSS receivers could benefit from improvements made here. We believe to have come close to achieving these goals by generating, validating, and publishing the static Earth gravity field models AIUB-CHAMPOIS, AIUB-CHAMP02S, and AIUB-CHAMP03S. Furthermore, the largest constituents of the seasonal gravity field variations could be retrieved from CHAMP data, as well. The Celestial Mechanics Approach (CMA) was successfully applied for gravity field determination. Note de contenu : 1 Introduction
2 Measuring the Earth's gravity field
2.1 Terrestrial geodesy
2.2 Satellite geodesy
2.2.1 Optical observations
2.2.2 Microwave methods
2.2.3 Satellite Laser Ranging (SLR)
2.2.4 Satellite altimetry
2.2.5 High-low SST of CHAMP
2.2.6 Low-low SST with GRACE
2.2.7 Satellite gradiometry with GOCE
3 Orbit determination and gravity field recovery
3.1 Least squares adjustment
3.1.1 Basic concept
3.1.2 LSA techniques
3.2 Coordinate systems
3.2.1 Geocentric quasi-inertial system
3.2.2 Earth-fixed coordinate system
3.2.3 Satellite-fixed coordinate system
3.3 Satellite orbits
3.3.1 Dynamic orbits
3.3.2 Reduced-dynamic orbits
3.3.3 Kinematic orbits
3.4 The equation of motion
3.5 Spherical harmonic representation of the gravitational potential
3.6 Orbit and gravity field determination
3.6.1 Numerical integration of the primary equations
3.6.2 Numerical integration of the variational equations
4. Global Positioning System - GPS
4.1 History
4.2 Basic measurement principle
4.3 GPS orbit constellation and satellites
4.4 GPS signals
4.5 Modeling GPS observables
4.5.1 Observation equations
4.5.2 Observation differences
4.5.3 Linear combinations
4.6 The International GNSS Service (IGS)
4.7 Bernese GPS Software (BSW)
5 Data processing
5.1 Generation of the A1UB-CHAMP01S gravity field model
5.1.1 Data Screening
5.1.2 Gravity field recovery
5.1.3 The AIUB-CHAMP01S gravity field model
5.2 Generation of the AIUB-CHAMP02S gravity field model
5.2.1 GNSS model changes
5.2.2 GPS orbit reprocessing
5.2.3 GPS satellite clock reprocessing
5.2.4 CHAMP orbit determination
5.2.5 AIUB-CHAMP02S gravity field recovery
5.2.6 The AIUB-CHAMP02S gravity field model
5.3 Generation of the AIUB-CHAMP03S gravity field model
5.3.1 Estimation of high-rate GPS satellite clock corrections
5.3.2 CHAMP orbit determination
5.3.3 Data screening and gravity field recovery
5.3.4 The AIUB-CHAMP03S gravity field model
6 Studies and experiments
6.1 Studies related to A1UB-C11AMP01S
6.1.1 Orbit modeling with arc-specific parameters
6.1.2 Modeling of non-gravitational perturbations with dynamic force models
6.1.3 Accelerometer data
6.1.4 Simulation study
6.1.5 Observation weights .
6.1.6 Influence of the a priori gravity field model
6.1.7 Screening the kinematic positions
6.1.8 Quality variations in monthly gravity field solutions
6.1.9 Summary and discussion of the IUB-CHAMPOlS-related studies
6.2 Experiments related to AIUB-CI1AMP02S
6.2.1 The impact of GNSS model changes
6.2.2 Inconsistency in the low degree harmonics
6.2.3 Simulation study
6.2.4 Latitude dependency of the observation scenario
6.2.5 Summary and conclusion of the AIUB-CHAMP02S-related studies
6.3 Experiments related to AIUB-CHAMP03S ..
6.3.1 Influence of empirical PCV-models on gravity field recovery using CHAMP GPS data ..
6.3.2 Elevation-dependent weighting
6.3.3 Observation sampling
6.3.4 Inter-epoch correlations of kinematic positions
6.3.5 Position differences vs. positions
6.3.6 Impact of observations of eclipsing GPS satellites on CHAMP gravity field recovery ...
6.3.7 Temporal variations of the Earth's gravity field
6.3.8 Recovery of the low degree harmonics
6.3.9 Summary of the experiments related to AIUB-CHAMP03S
7 Gravity field validation
7.1 Validation methods
7.1.1 Formal errors
7.1.2 Comparison with other gravity field models
7.1.3 Comparison with ground data
7.1.4 Altimetry data
7.1.5 Orbit determination
7.2 Validation of AIUB-CHAMP01S
7.2.1 Internal validation .
7.2.2 External validation
7.3 Validation of AIUB-CHAMP02S
7.3.1 Internal validation
7.3.2 External validation
7.4 Validation of AIUB-CHAMP03S
7.4.1 Internal validation
7.4.2 External validation
8 Summary and conclusionsNuméro de notice : 10370 Affiliation des auteurs : non IGN Thématique : POSITIONNEMENT Nature : Rapport de recherche En ligne : https://www.sgc.ethz.ch/sgc-volumes/sgk-81.pdf Format de la ressource électronique : URL Permalink : https://documentation.ensg.eu/index.php?lvl=notice_display&id=62409 Réservation
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Code-barres Cote Support Localisation Section Disponibilité 10370-01 30.40 Livre Centre de documentation Géodésie Disponible Journées 2010, systèmes de référence spatio-temporels, Paris, 20-22 septembre 2010 / Nicole Capitaine (2010)
Titre : Journées 2010, systèmes de référence spatio-temporels, Paris, 20-22 septembre 2010 : New challenges for reference systems and numerical standards in astronomy Titre original : Nouveaux défis pour les systèmes de référence et les constantes astronomiques Type de document : Actes de congrès Auteurs : Nicole Capitaine, Éditeur scientifique Editeur : Paris, Meudon et Nançay : Observatoire de Paris Année de publication : 2010 Conférence : JSRST 2010, Journées systèmes de référence spatio-temporels, New challenges for reference systems and numerical standards in astronomy 20/09/2010 22/09/2010 Paris France OA proceedings Importance : 300 p. Format : 21 x 30 cm ISBN/ISSN/EAN : 978-2-901057-64-2 Note générale : Bibliographie Langues : Anglais (eng) Descripteur : [Vedettes matières IGN] Systèmes de référence et réseaux
[Termes IGN] catalogue d'étoiles
[Termes IGN] éphémérides astronomiques
[Termes IGN] norme
[Termes IGN] pulsar
[Termes IGN] rotation de la TerreNote de contenu : SESSION 1: THE ASTRONOMICAL CONSTANTS, SI UNITS AND FUTURE DEVELOPMENTS IN NUMERICAL STANDARDS
Luzum B., Capitaine N., Fienga A., Folkner W. et al.: Numerical standards of fundamental astronomy working group update
Petit G.: The new edition of the iers conventions: conventional reference systems and constants
Jacobson R. A. , Folkner W. M. , Taylor A. H. , Konopliv A. S. , Williams J. G. , Brozovic M. : Planetary system gms in the JPL planetary ephemerides
Hohenkerk C.Y.: SOFA - A status report, review and look to the future
Capitaine N., Guinot B., Klioner S.: Proposal for the re-definition of the astronomical unit of length through a fixed relation to the SI metre
Vondr?ak J., Capitaine N., Wallace P.: Some new thoughts about long-term precession formula
Débarbat S., Passeron I., Launay F.: From old weights and measures to the SI as a numerical standard for the world
Kudryavtsev S.M.: An inertial effect in satellite motion not described by the current IERS conventions
SESSION 2: SOLAR SYSTEM EPHEMERIDES AND THEIR COMPARISON
Kaplan G. H.: Introductory remarks for session 2
Fienga A., Manche H., Kuchynka P., Laskar J., Gastineau M.: Planetary and lunar ephemerides INPOP10A
Folkner W.M.: Uncertainties in the JPL planetary ephemeris
Pitjeva E.V., Bratseva O.A., Panfilov V.E.: EPM ? Ephemerides of Planets and the Moon of IAA RAS: their model, accuracy, availability
Laskar J., Fienga A., Gastineau M., Manche H: INPOP, a million year ephemeris
Kudryavtsev S.M.: Development of long-term numerical ephemerides of telluric planets to analytical series
Krasinsky G.A., Prokhorenko S.O., Yagudina E.I.: New version of EPM-ERA Lunar theory
Manche H., Fienga A., Laskar J., Bouquillon S., Francou G., Gastineau M.: LLR residuals of INPOP10A and constraints on Post-Newtonian parameters
Dehant V., Oberst J., Nadalini, R.: Geodesy instrument package on the Moon for improving our knowledge of the Moon and the realization of reference frames
Pashkevich V.V., Eroshkin G.I.: Application of the spectral analysis methods for the investigation of the Moon rotation
Hilton J.L., Hohenkerk C.Y.: A comparison of the high accuracy planetary ephemerides DE421, EPM2008, and INPOP08
Barache C., Bouquillon S., Carlucci T., Deleflie F. et al.: Web interface for lunar laser ranging observations
Cottereau L.: A dynamical study of Phoebe's rotation
Francou G., Simon J.-L.: New analytical planetary theories VSOP2010
Giorgini J.: Summary and status of the Horizons ephemeris system
Marco F.J., Martinez M.J., Lopez J.A.: Propagation in time of errors for the mutual inclination of satellites
Weratschnig J.M. , Taylor D.B., Bell S.A., Hilton J.L., A.T. Sinclair: Computation of the quantities describing Lunar librations in the Astronomical Almanac
SESSION 3: PROGRESS IN ASTROMETRIC CATALOGS IN OPTICAL AND RADIO WAVELENGTHS
Zacharias N., Gaume R.: UCAC and URAT: optical astrometric catalog observing programs
Souchay J.: The large quasar astrometric catalogue (LQAC) and the densification of the ICRF through the LQRF (Large Quasar Reference Frame)
Bucciarelli B., Andrei A.H., Smart R.L., Lattanzi M.G., Schirosi U., Penna J.L., Dapr?a M., de Moura Estev˜ Ao T.G., D'? Avila V.A., Camargo J.I.B., Crosta M.T., Goldman B., Jones H.R.A., Nicastro L., Da Silva Neto D.N., Teixeira R.: Absolute parallaxes and proper motions from the PARSEC program
Bourda G., Collioud A., Charlot P., Porcas R., Garrington S.: Towards a VLBI catalog of optically-bright extragalactic radio sources for the alignment of the radio frame with the future GAIA frame
Damljanovic G.: Comparison of the proper motions in declination of four catalogues via 807 hipparcos stars
Fedorov P.N., Akhmetov V.S., Yatskiv Ya.S.: THE XPM catalogue as a realisation of the extragalactic reference system in optical and near infrared WAVELENGHS
Maigurova N., Martynov M., Pinigin G.: Optical positions of ICRF sources using UCAC3 reference stars
Andrei A.H., Gontier A.-M., Barache C., da Silva Neto D.N. et al.: GAIA initial quasar catalogue - updates: morphology and variability
Yatskiv Ya.S., Bolotin S.L., Lytvyn S.O.: MAO C 08A combined catalogue of radio source positions created in the course of preparation for the ICRF2
SESSION 4: RECENT DEVELOPMENTS IN THEORY AND OBSERVATION OF EARTH ROTATION AND RELATED REFERENCE SYSTEMS
Brzezi?nski A.: Diurnal excitation of Earth rotation estimated from recent geophysical models
Gross R.S, Dickman S.R.: Observing and modeling long-period tidal variations in polar motion
Altamimi Z., Collilieux X.: Examination of some ITRF2008 results
Böhm S., Schuh H.: Response of the Earth system to zonal tidal forcing examined by VLBI based dUT1 variations
Chapanov Ya., Vondr?ak J., Ron C.: Centennial cycles of the solar activity and Earth rotation
Escapa A., Getino J., Miguel D., Ferr?andiz J. M.: Influence of the inner core geopotential variations on the rotation of the Earth
Brumberg V. A., Ivanova T. V.: On solution of the three?axial Earth's rotation problem
Boucher C.: A refined definition of the International Terrestrial Reference System
Coulot D., Bernard E., Collilieux X.: Influence of station referencing on the quality of EOP time series
Nastula J., Pasnicka M., Kolaczek B.: Comparison of the hydrological excitation functions HAM of polar motion for the period 1980.0-2007.0
KosekW., Popi?nskiW., Niedzielski T.: Wavelet based comparison of high frequency oscillations in the geodetic and fluid excitation functions of polar motion
Malkin Z.M.: Comparison of CPO and FCN empirical models
Nilsson T., B?ohm J., Schuh H.: Impacts of the 2010 Chile earthquake on Earth rotation
Schindelegger M., B?ohm J., Schuh H., Salstein D.A.: High-resolution atmospheric angular momentum. Functions from different ecmwf data classes
Stamatakos N., Luzum B. , Stetzler B., Shumate N., Carter M. S.: Recent improvements in IERS rapid service/prediction center products
Zotov L.V.: Analysis of Chandler wobble excitation, reconstructed from observations of the polar motion of the Earth
Aleshkina E.Yu.: on correlation between variations in Earth rotation and frequency of earthquakes
Abarca del Rio R. , Gambis D.: Revisiting a possible relationship between solar activity and Earth rotation variability
Bizouard C., Lambert S., Remus F., Seoane L., Gambis D.: The source of the variable Chandler wobble
Chapanov Ya. , Gambis D.: Variations of the Earth principal moments of inertia due to glacial cycles for the last 800KA
Hefty J., Gerhatova L., Burgan J.: Combination of GPS and GLONASS IN PPP algorithms and its effect on site coordinates determination
Kudryashova M., Lambert S., Dehant V., Bruyninx C., Defraigne P.: Determination of nutation offsets by combining VLBI/GPS-produced normal equations
Lambert S. B., Gontier A.-M., Barache C.: Operational and research activity at OPAR
Gontier A.-M., Lambert S. B.: Physical characteristics of the ICRF2 sources
Malkin Z.M. , Miller N.O.: Amplitude and phase variations of the chandler wobble from 164-yr polar motion series
Marýceta D., ý Segan S.: Method for prediction of _T based on long-periodic terms in the Earth's rate of rotation
Marco F.J., Martinez M.J.: Applications of simultaneous ground-based and satellite observations
Martinez M.J., Marco F.J.: _T and tidal acceleration values from three European medieval eclipses
Morcov G.: About the configuration of the geoid undulations and their kinematics
Niedzielski T., Kosek W.: Nonlinear sea level variations in the equatorial Pacific due to ENSO
Richard J.Y., Gambis D., Bizouard C.: Earth rotation parameters determined over CONT08 from the combination of space geodetic techniques
Ron C., Vondr?ak J., ý Stefka V.: Comparison of the various atmospheric and oceanic angular momentum series
ý Stefka V.: The recent improvement in non-rigorous combination method of space geodetic techniques
Tian W., Brzezinski A., Soffel M.H., Gebauer A., Schreiber K.U., Kl?ugel T.: The interpretation of high frequency signals in the g-ring laser gyroscope
Yao K., Capitaine, N.: Modelling of the Earth orientation and high precision astrometric observation techniques
SESSION 5: PULSARS TIMING, RELATIVITY AND TIME TRANSFER
Kopeikin S.M.: An extension of the IAU framework for reference systems
Hobbs G., Coles W., Manchester R., Chen D.: Developing a pulsar-based timescale
Rodin A.E.: Ensemble pulsar time scale
Cognard I., Desvignes G., Theureau G.: High precision pulsar timing: Nancay and the European pulsar timing array
Gusev A.: Chandler wobble and free core nutation of single pulsar
Soffel M.H., Klioner S.A., Gerlach E.: About the MacCullagh relations in relativity
Xie Y., Kopeikin S.: Post-Newtonian mechanics of the Earth-Moon system
Teyssandier P.: Post-post-Newtonian light propagation without integrating the geodesic equations
Mouret S.: Tests of fundamental physics with the GAIA mission
Lamine B., Courty J.-M., Reynaud S., Jaekel M.-T.: Testing gravity law in the solar system
Deng X.-M. , Huang T.-Y.: 2PN light propagation and measurement in the solar system
Dumin Yu.V.: Perturbation of a planetary orbit by the lambda-term (dark energy) in Einstein equations
Fienga A., Desvignes G., Cognard I., Theureau G.: Use of millisecond pulsars to test and link
planetary ephemeride reference frames to ICRF
Kanj A., Achkar J.: Development of the TWSTFT carrier-phase technique at LNE-SYRTE
Bertone S., Le Poncin-Lafitte C., Lainey, V.: Light time calculations for deep space navigationNuméro de notice : 14318 Affiliation des auteurs : non IGN Thématique : POSITIONNEMENT Nature : Actes DOI : sans En ligne : https://syrte.obspm.fr/jsr/journees2010/pdf/ Format de la ressource électronique : URL Permalink : https://documentation.ensg.eu/index.php?lvl=notice_display&id=34654 ContientRéservation
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Code-barres Cote Support Localisation Section Disponibilité 14318-01 CG2010 Livre Centre de documentation Congrès Disponible Mise en place d’une chaîne de calcul ultra rapide des orbites et des corrections d’horloges des satellites GLONASS / Oussama Ben Abdelaziz (2010)PermalinkPermalinkSciences of geodesy, vol 1. Advanced and future directions / Guochang Xu (2010)PermalinkGeocenter variations derived from GPS tracking of the GRACE satellites / Z. Kang in Journal of geodesy, vol 83 n° 10 (October 2009)PermalinkAnnuaire du Bureau des Longitudes, Guide de données astronomiques 2010, pour l'observation du ciel / Bureau des longitudes (2009)PermalinkL'astronomie au service de tous / J.E. Arlot (2009)PermalinkSystème solaire et planètes / Anny-Chantal Levasseur-Regourd (2009)PermalinkVariations in the accuracy of gravity recovery due to ground track variability: GRACE, CHAMP, and GOCE / J. Klokocnik in Journal of geodesy, vol 82 n° 12 (December 2008)PermalinkFormulation of distortion error for the line-of-sight (LOS) vector adjustment model and its role in restitution of SPOT imagery / Hyung-Sup Jung in ISPRS Journal of photogrammetry and remote sensing, vol 63 n° 6 (November - December 2008)PermalinkAnnuaire du Bureau des Longitudes, Guide de données astronomiques 2009, pour l'observation du ciel / Bureau des longitudes (2008)PermalinkGNSS, Global Navigation Satellite Systems / Bernhard Hofmann-Wellenhof (2008)PermalinkZur Entwicklung von Bahntheorien / Enrico Mai (2008)PermalinkBringing all GNSS into line: new assistance standards embrace Galileo, Glonass, QZSS [Japanese quasi-zenith satellite system], SBAS [space-based augmentation system] / L. Wirola in GPS world, vol 18 n° 9 (September 2007)PermalinkMap projections minimizing distance errors / J.R. Gott in Cartographica, vol 42 n° 3 (September 2007)PermalinkSentinel-3, the ocean and medium-resolution land mission for GMES operational services / M. Aguirre in ESA bulletin, n° 131 (August 2007)PermalinkTidal analysis experiments with sun-synchronous satellite altimeter data / R.D. Ray in Journal of geodesy, vol 81 n° 4 (April 2007)PermalinkAnnuaire du Bureau des Longitudes, guide de données astronomiques 2008, pour l'observation du ciel / Bureau des longitudes (2007)PermalinkPermalinkPseudo-stochastic orbit modeling of low earth satellites using the Global Positioning System / Adrian Jäggi (2007)PermalinkTrajectoires en consommation minimale pour le déploiement d'une formation de satellites / J.B. Thevenet (2007)Permalink