Details
| Originalsprache | Englisch |
|---|---|
| Fachzeitschrift | Journal of Physics: Conference Series |
| Jahrgang | 154 |
| Publikationsstatus | Veröffentlicht - 2009 |
| Extern publiziert | Ja |
| Veranstaltung | 7TH INTERNATIONAL LISA SYMPOSIUM - Barcelona, Spanien Dauer: 16 Juni 2008 → 20 Juni 2008 |
Abstract
Two key components of LISA's inter-spacecraft clock tone transfer chain are electro-optic modulators (EOMs) and high-frequency (HF) cable assemblies. At modulation frequencies of 2GHz, we characterized the excess phase noise of these components in the LISA frequency range (0.1 mHz to 1 Hz). The upper phase noise limit was found to be almost an order of magnitude better than required. In addition, phase dependencies on temperature were determined. The measured coefficients are within a few milliradians per Kelvin and thereby negligible due to the specified on-board temperature stability.
ASJC Scopus Sachgebiete
- Physik und Astronomie (insg.)
- Allgemeine Physik und Astronomie
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in: Journal of Physics: Conference Series, Jahrgang 154, 2009.
Publikation: Beitrag in Fachzeitschrift › Konferenzaufsatz in Fachzeitschrift › Forschung › Peer-Review
}
TY - JOUR
T1 - Phase noise contribution of EOMs and HF cables
AU - Barke, Simon
AU - Tröbs, Michael
AU - Sheard, Benjamin
AU - Heinzel, Gerhard
AU - Danzmann, Karsten
PY - 2009
Y1 - 2009
N2 - Two key components of LISA's inter-spacecraft clock tone transfer chain are electro-optic modulators (EOMs) and high-frequency (HF) cable assemblies. At modulation frequencies of 2GHz, we characterized the excess phase noise of these components in the LISA frequency range (0.1 mHz to 1 Hz). The upper phase noise limit was found to be almost an order of magnitude better than required. In addition, phase dependencies on temperature were determined. The measured coefficients are within a few milliradians per Kelvin and thereby negligible due to the specified on-board temperature stability.
AB - Two key components of LISA's inter-spacecraft clock tone transfer chain are electro-optic modulators (EOMs) and high-frequency (HF) cable assemblies. At modulation frequencies of 2GHz, we characterized the excess phase noise of these components in the LISA frequency range (0.1 mHz to 1 Hz). The upper phase noise limit was found to be almost an order of magnitude better than required. In addition, phase dependencies on temperature were determined. The measured coefficients are within a few milliradians per Kelvin and thereby negligible due to the specified on-board temperature stability.
UR - http://www.scopus.com/inward/record.url?scp=66149156561&partnerID=8YFLogxK
U2 - 10.1088/1742-6596/154/1/012006
DO - 10.1088/1742-6596/154/1/012006
M3 - Conference article
AN - SCOPUS:66149156561
VL - 154
JO - Journal of Physics: Conference Series
JF - Journal of Physics: Conference Series
SN - 1742-6588
T2 - 7TH INTERNATIONAL LISA SYMPOSIUM
Y2 - 16 June 2008 through 20 June 2008
ER -