- Antenna and Base Capacitances (see Receiver/Electrical Design section, for detailed information)
Quantity Value Unit Antenna Capacitance (Ca) ~ 40 pF Monopole Stray Capacitance (Cs,m) ~ 67 pF Dipole Stray Capacitance (Cs,d) 32±4 pF - Receiver Noise Level (see Receiver/Receiver Noise section, for detailed information)
Quantity Value Unit Receiver Noise on STEREO-A (V2noise) -161.8±0.8 dB Receiver Noise on STEREO-B (V2noise) -163.9±1.5 dB - Antenna Length (see Antenna Length section, for detailed information)
Quantity Value Unit Effective length for hX on STEREO-A
(using mode 11, 12 and 13)2.96±0.20 m Effective length for hY on STEREO-A
(using mode 12 and 21)3.69±0.22 m Effective length for hZ on STEREO-A
(using mode 11, 21 and 31)2.68±0.41 m Effective length for hXY on STEREO-A
(using mode 31)4.25±0.15 m Effective length for hYZ on STEREO-A
(using mode 13)4.32±0.27 m Effective length for hX on STEREO-B
(using mode 11, 12 and 13)3.15±0.13 m Effective length for hY on STEREO-B
(using mode 12 and 21)3.68±0.10 m Effective length for hZ on STEREO-B
(using mode 11, 21 and 31)2.34±0.25 m Effective length for hXY on STEREO-B
(using mode 31)4.30±0.12 m Effective length for hYZ on STEREO-B
(using mode 13)3.89±0.15 m - Antenna Direction (see Antenna Direction section, for detailed information)
Quantity Value Unit Effective antenna colatitude (θ) for hX 52.4±0.2 deg Effective antenna azimuth (φ) for hX 231.6±0.1 deg Effective antenna colatitude (θ) for hY 58.4±0.6 deg Effective antenna azimuth (φ) for hY 120.1±1.1 deg Effective antenna colatitude (θ) for hZ 142.0±0.5 deg Effective antenna azimuth (φ) for hZ 160.9±0.7 deg Effective antenna colatitude (θ) for hXY 90.3±0.2 deg Effective antenna azimuth (φ) for hXY 91.1±0.4 deg Effective antenna colatitude (θ) for hYZ 32.9±0.1 deg Effective antenna azimuth (φ) for hYZ 93.3±2.9 deg
STEREO/Waves antenna Quick Facts
Operational Set of Calibrated Parameters
We present here a simplified operational set of calibrated parameters considered as the most "up-to-date" for use with the STEREO/Waves data.
Credits
This web page has been compiled and is maintained by B. Cecconi1, Co-I of STEREO/Waves.
Special thanks to: C. Briand1, V. Krupar1,2, M. Maksimovic1, M. Panchenko3, A. Zaslavsky1.
1. LESIA, Observatoire de Paris, Meudon, France;
2. Faculty of Mathematics and Physics, Charles University, Prague, Czech Republic;
3. Space Research Institute, Austrian Academy of Sciences, Graz, Austria.
Special thanks to: C. Briand1, V. Krupar1,2, M. Maksimovic1, M. Panchenko3, A. Zaslavsky1.
1. LESIA, Observatoire de Paris, Meudon, France;
2. Faculty of Mathematics and Physics, Charles University, Prague, Czech Republic;
3. Space Research Institute, Austrian Academy of Sciences, Graz, Austria.
For any comments, inputs or suggestion, please contact B. Cecconi.
Last update:
January 22 2015 19:51:29.