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• LFI design, qualification, and performance
  Every RCA consists of two radiometers, each feeding two diode detectors (see Fig. 2 above), for a total of 44 detectors. The 11 RCAs are P_{\rm out}^{\rm diode} = a\, G_{\rm tot}\,k\,\beta \left[ T_{\rm sky} + T_{\rm noise} - r\left(
  50 KB (7,826 words) - 22:29, 4 February 2015
• The LFI DPC
  ...|Gain Modulation Factor]] • [[TOI_processing LFI#Diode Combination|Diode Combination]] • [[TOI_processing LFI#Planet Flagging|Planet Flagging]] • [[TOI_proc
  8 KB (1,072 words) - 20:27, 4 February 2015
• Timelines
  ...rumental effect is removed by applying well know templates directly to the diode signal. ; Demodulation: each LFI diode switches at 4096 Hz between the sky and the 4K reference load. The data acq
  28 KB (4,415 words) - 18:43, 21 August 2015
• The satellite
  ...operating temperatures, 20 K for LFI and 0.1 K for HFI, achieved through a combination of passive radiative cooling and three active coolers. The scientific requ diode detector (D3). The main entrance window is covered
  14 KB (2,170 words) - 09:29, 21 May 2014
• TOI processing LFI
  ...he signals from one diode are combined with signals from the complementary diode in the same radiometer. Finally, photometric calibration is applied for eac ...d the white noise in the difference timestream. The i index represents the diode and can be 0 or 1.
  34 KB (5,468 words) - 15:34, 4 February 2015
• The satellite WiP
  ...operating temperatures, 20 K for LFI and 0.1 K for HFI, achieved through a combination of passive radiative cooling and three active coolers. The scientific requ diode detector (D3). The main entrance window is covered
  14 KB (2,136 words) - 09:37, 3 February 2015