Determination of Nutation Coefficients from Lunar Laser Ranging

Publikation: Beitrag in Buch/Bericht/Sammelwerk/KonferenzbandAufsatz in KonferenzbandForschungPeer-Review

Autoren

Organisationseinheiten

Forschungs-netzwerk anzeigen

Details

OriginalspracheEnglisch
Titel des SammelwerksGeodesy for Planet Earth - Proceedings of the 2009 IAG Symposium
Seiten521-525
Seitenumfang5
PublikationsstatusVeröffentlicht - Dez. 2012
VeranstaltungIAG Symposium on Geodesy for Planet Earth, IAG 2009 - Chania, Crete, Argentinien
Dauer: 31 Aug. 20094 Sept. 2009

Publikationsreihe

NameInternational Association of Geodesy Symposia
Band136
ISSN (Print)0939-9585

Abstract

It was just July 20, 1969 when the first retro-reflector for Lunar Laser Ranging (LLR) was deployed on the Moon by the Apollo 11 crew. From this day on, LLR is carried out to measure the distance between Earth and Moon. The complete set of observations is analysed and various parameters of the Earth-Moon system are determined by least-squares adjustment. Because of the long time span of data, long-term lunisolar nutation coefficients of the 18.6-year period (and the precession rate) can be determined well. But also other periods (182.62-day, 9.3-year, 365.26-day) can be fitted. The nutation coefficients were determined from LLR based on the models for precession and nutation according to the IAU Resolution 2006 and compared to the MHB2000 model of Mathews et al. (2002). In this paper, the corresponding preliminary results are discussed.

ASJC Scopus Sachgebiete

Zitieren

Determination of Nutation Coefficients from Lunar Laser Ranging. / Biskupek, L.; Müller, J.; Hofmann, F.
Geodesy for Planet Earth - Proceedings of the 2009 IAG Symposium. 2012. S. 521-525 (International Association of Geodesy Symposia; Band 136).

Publikation: Beitrag in Buch/Bericht/Sammelwerk/KonferenzbandAufsatz in KonferenzbandForschungPeer-Review

Biskupek, L, Müller, J & Hofmann, F 2012, Determination of Nutation Coefficients from Lunar Laser Ranging. in Geodesy for Planet Earth - Proceedings of the 2009 IAG Symposium. International Association of Geodesy Symposia, Bd. 136, S. 521-525, IAG Symposium on Geodesy for Planet Earth, IAG 2009, Chania, Crete, Argentinien, 31 Aug. 2009. https://doi.org/10.1007/978-3-642-20338-1_63
Biskupek, L., Müller, J., & Hofmann, F. (2012). Determination of Nutation Coefficients from Lunar Laser Ranging. In Geodesy for Planet Earth - Proceedings of the 2009 IAG Symposium (S. 521-525). (International Association of Geodesy Symposia; Band 136). https://doi.org/10.1007/978-3-642-20338-1_63
Biskupek L, Müller J, Hofmann F. Determination of Nutation Coefficients from Lunar Laser Ranging. in Geodesy for Planet Earth - Proceedings of the 2009 IAG Symposium. 2012. S. 521-525. (International Association of Geodesy Symposia). doi: 10.1007/978-3-642-20338-1_63
Biskupek, L. ; Müller, J. ; Hofmann, F. / Determination of Nutation Coefficients from Lunar Laser Ranging. Geodesy for Planet Earth - Proceedings of the 2009 IAG Symposium. 2012. S. 521-525 (International Association of Geodesy Symposia).
Download
@inproceedings{20773cb47b7741f9bd235349eee8369d,
title = "Determination of Nutation Coefficients from Lunar Laser Ranging",
abstract = "It was just July 20, 1969 when the first retro-reflector for Lunar Laser Ranging (LLR) was deployed on the Moon by the Apollo 11 crew. From this day on, LLR is carried out to measure the distance between Earth and Moon. The complete set of observations is analysed and various parameters of the Earth-Moon system are determined by least-squares adjustment. Because of the long time span of data, long-term lunisolar nutation coefficients of the 18.6-year period (and the precession rate) can be determined well. But also other periods (182.62-day, 9.3-year, 365.26-day) can be fitted. The nutation coefficients were determined from LLR based on the models for precession and nutation according to the IAU Resolution 2006 and compared to the MHB2000 model of Mathews et al. (2002). In this paper, the corresponding preliminary results are discussed.",
author = "L. Biskupek and J. M{\"u}ller and F. Hofmann",
note = "Funding information: We would also like to thank the DFG, the German Research Foundation, which funded this study within the research unit FOR584 “Earth rotation and global dynamic processes”.; IAG Symposium on Geodesy for Planet Earth, IAG 2009 ; Conference date: 31-08-2009 Through 04-09-2009",
year = "2012",
month = dec,
doi = "10.1007/978-3-642-20338-1_63",
language = "English",
isbn = "9783642203374",
series = "International Association of Geodesy Symposia",
pages = "521--525",
booktitle = "Geodesy for Planet Earth - Proceedings of the 2009 IAG Symposium",

}

Download

TY - GEN

T1 - Determination of Nutation Coefficients from Lunar Laser Ranging

AU - Biskupek, L.

AU - Müller, J.

AU - Hofmann, F.

N1 - Funding information: We would also like to thank the DFG, the German Research Foundation, which funded this study within the research unit FOR584 “Earth rotation and global dynamic processes”.

PY - 2012/12

Y1 - 2012/12

N2 - It was just July 20, 1969 when the first retro-reflector for Lunar Laser Ranging (LLR) was deployed on the Moon by the Apollo 11 crew. From this day on, LLR is carried out to measure the distance between Earth and Moon. The complete set of observations is analysed and various parameters of the Earth-Moon system are determined by least-squares adjustment. Because of the long time span of data, long-term lunisolar nutation coefficients of the 18.6-year period (and the precession rate) can be determined well. But also other periods (182.62-day, 9.3-year, 365.26-day) can be fitted. The nutation coefficients were determined from LLR based on the models for precession and nutation according to the IAU Resolution 2006 and compared to the MHB2000 model of Mathews et al. (2002). In this paper, the corresponding preliminary results are discussed.

AB - It was just July 20, 1969 when the first retro-reflector for Lunar Laser Ranging (LLR) was deployed on the Moon by the Apollo 11 crew. From this day on, LLR is carried out to measure the distance between Earth and Moon. The complete set of observations is analysed and various parameters of the Earth-Moon system are determined by least-squares adjustment. Because of the long time span of data, long-term lunisolar nutation coefficients of the 18.6-year period (and the precession rate) can be determined well. But also other periods (182.62-day, 9.3-year, 365.26-day) can be fitted. The nutation coefficients were determined from LLR based on the models for precession and nutation according to the IAU Resolution 2006 and compared to the MHB2000 model of Mathews et al. (2002). In this paper, the corresponding preliminary results are discussed.

UR - http://www.scopus.com/inward/record.url?scp=84884340386&partnerID=8YFLogxK

U2 - 10.1007/978-3-642-20338-1_63

DO - 10.1007/978-3-642-20338-1_63

M3 - Conference contribution

AN - SCOPUS:84884340386

SN - 9783642203374

T3 - International Association of Geodesy Symposia

SP - 521

EP - 525

BT - Geodesy for Planet Earth - Proceedings of the 2009 IAG Symposium

T2 - IAG Symposium on Geodesy for Planet Earth, IAG 2009

Y2 - 31 August 2009 through 4 September 2009

ER -

Von denselben Autoren