Details
| Originalsprache | Englisch |
|---|---|
| Seiten (von - bis) | S1-S9 |
| Fachzeitschrift | Classical and quantum gravity |
| Jahrgang | 20 |
| Ausgabenummer | 10 |
| Publikationsstatus | Veröffentlicht - 21 Mai 2003 |
| Veranstaltung | 4th International LISA Symposium - Penn State University, Pennsylvania, USA / Vereinigte Staaten Dauer: 19 Juli 2002 → 24 Juli 2002 |
Abstract
The existence of gravitational waves is the most prominent of Einstein's predictions that has not yet been directly verified. The space project LISA shares its goal and principle of operation with the ground-based interferometers currently under construction: the detection and measurement of gravitational waves by laser interferometry. Only in space, detection of signals below, say, 1 Hz is possible. LISA, a joint project of ESA and NASA, is a mission that will measure these low-frequency waves. LISA consists of three spacecraft in heliocentric orbits, forming a triangle with 5 million km sides. Launch for LISA is scheduled for 2011, following a technology demonstrator LTP in 2006.
ASJC Scopus Sachgebiete
- Physik und Astronomie (insg.)
- Physik und Astronomie (sonstige)
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in: Classical and quantum gravity, Jahrgang 20, Nr. 10, 21.05.2003, S. S1-S9.
Publikation: Beitrag in Fachzeitschrift › Konferenzaufsatz in Fachzeitschrift › Forschung › Peer-Review
}
TY - JOUR
T1 - LISA technology
T2 - 4th International LISA Symposium
AU - Danzmann, Karsten
AU - R̈diger, Albrecht
PY - 2003/5/21
Y1 - 2003/5/21
N2 - The existence of gravitational waves is the most prominent of Einstein's predictions that has not yet been directly verified. The space project LISA shares its goal and principle of operation with the ground-based interferometers currently under construction: the detection and measurement of gravitational waves by laser interferometry. Only in space, detection of signals below, say, 1 Hz is possible. LISA, a joint project of ESA and NASA, is a mission that will measure these low-frequency waves. LISA consists of three spacecraft in heliocentric orbits, forming a triangle with 5 million km sides. Launch for LISA is scheduled for 2011, following a technology demonstrator LTP in 2006.
AB - The existence of gravitational waves is the most prominent of Einstein's predictions that has not yet been directly verified. The space project LISA shares its goal and principle of operation with the ground-based interferometers currently under construction: the detection and measurement of gravitational waves by laser interferometry. Only in space, detection of signals below, say, 1 Hz is possible. LISA, a joint project of ESA and NASA, is a mission that will measure these low-frequency waves. LISA consists of three spacecraft in heliocentric orbits, forming a triangle with 5 million km sides. Launch for LISA is scheduled for 2011, following a technology demonstrator LTP in 2006.
UR - http://www.scopus.com/inward/record.url?scp=0242266061&partnerID=8YFLogxK
U2 - 10.1088/0264-9381/20/10/301
DO - 10.1088/0264-9381/20/10/301
M3 - Conference article
AN - SCOPUS:0242266061
VL - 20
SP - S1-S9
JO - Classical and quantum gravity
JF - Classical and quantum gravity
SN - 0264-9381
IS - 10
Y2 - 19 July 2002 through 24 July 2002
ER -