Details
| Originalsprache | Englisch |
|---|---|
| Seiten | 426-427 |
| Seitenumfang | 2 |
| Publikationsstatus | Veröffentlicht - 2002 |
| Veranstaltung | Conference on Lasers and Electro-Optics (CLEO 2002) - Long Beach, CA, USA / Vereinigte Staaten Dauer: 19 Mai 2002 → 24 Mai 2002 |
Konferenz
| Konferenz | Conference on Lasers and Electro-Optics (CLEO 2002) |
|---|---|
| Kurztitel | CLEO 2002 |
| Land/Gebiet | USA / Vereinigte Staaten |
| Ort | Long Beach, CA |
| Zeitraum | 19 Mai 2002 → 24 Mai 2002 |
Abstract
Highly stable laser towards spaceborne gravitational wave detection was presented. The low frequency noise of the lasers was dominated by thermal fluctuations of the cavities. The frequency stability required for laser interferometer space antenna (LISA) was demonstrated. Results showed that sub-KHz power spectral densities at millihertz frequencies were observed.
ASJC Scopus Sachgebiete
- Werkstoffwissenschaften (insg.)
- Elektronische, optische und magnetische Materialien
- Physik und Astronomie (insg.)
- Atom- und Molekularphysik sowie Optik
- Physik und Astronomie (insg.)
- Physik der kondensierten Materie
- Ingenieurwesen (insg.)
- Elektrotechnik und Elektronik
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- BibTex
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2002. 426-427 Beitrag in Conference on Lasers and Electro-Optics (CLEO 2002), Long Beach, CA, USA / Vereinigte Staaten.
Publikation: Konferenzbeitrag › Paper › Forschung › Peer-Review
}
TY - CONF
T1 - Highly Stable Laser Towards Spaceborne Gravitational Wave Detection
AU - Tröbs, M.
AU - Hunnekuhl, M.
AU - Burdack, P.
AU - Hinze, U.
AU - Fallnich, C.
AU - Bode, M.
AU - Freitag, I.
AU - Skorupka, S.
AU - Heinzel, G.
AU - Danzmann, K.
PY - 2002
Y1 - 2002
N2 - Highly stable laser towards spaceborne gravitational wave detection was presented. The low frequency noise of the lasers was dominated by thermal fluctuations of the cavities. The frequency stability required for laser interferometer space antenna (LISA) was demonstrated. Results showed that sub-KHz power spectral densities at millihertz frequencies were observed.
AB - Highly stable laser towards spaceborne gravitational wave detection was presented. The low frequency noise of the lasers was dominated by thermal fluctuations of the cavities. The frequency stability required for laser interferometer space antenna (LISA) was demonstrated. Results showed that sub-KHz power spectral densities at millihertz frequencies were observed.
UR - http://www.scopus.com/inward/record.url?scp=0036459478&partnerID=8YFLogxK
M3 - Paper
AN - SCOPUS:0036459478
SP - 426
EP - 427
T2 - Conference on Lasers and Electro-Optics (CLEO 2002)
Y2 - 19 May 2002 through 24 May 2002
ER -