English

Level 1 on-ground telemetry handling in Planck LFI

Instrumentation and Methods for Astrophysics 2010-01-27 v1 Cosmology and Nongalactic Astrophysics

Abstract

The Planck Low Frequency Instrument (LFI) will observe the Cosmic Microwave Background (CMB) by covering the frequency range 30-70 GHz in three bands. The primary instrument data source are the temperature samples acquired by the 22 radiometers mounted on the Planck focal plane. Such samples represent the scientific data of LFI. In addition, the LFI instrument generates the so called housekeeping data by sampling regularly the on-board sensors and registers. The housekeeping data provides information on the overall health status of the instrument and on the scientific data quality. The scientific and housekeeping data are collected on-board into telemetry packets compliant with the ESA Packet Telemetry standards. They represent the primary input to the first processing level of the LFI Data Processing Centre. In this work we show the software systems which build the LFI Level 1. A real-time assessment system, based on the ESA SCOS 2000 generic mission control system, has the main purpose of monitoring the housekeeping parameters of LFI and detect possible anomalies. A telemetry handler system processes the housekeeping and scientific telemetry of LFI, generating timelines for each acquisition chain and each housekeeping parameter. Such timelines represent the main input to the subsequent processing levels of the LFI DPC. A telemetry quick-look system allows the real-time visualization of the LFI scientific and housekeeping data, by also calculating quick statistical functions and fast Fourier transforms. The LFI Level 1 has been designed to support all the mission phases, from the instrument ground tests and calibration to the flight operations, and developed according to the ESA engineering standards.

Keywords

Cite

@article{arxiv.1001.4730,
  title  = {Level 1 on-ground telemetry handling in Planck LFI},
  author = {A. Zacchei and M. Frailis and M. Maris and N. Morisset and R. Rohlfs and M. Meharga and P. Binko and M. Turler and S. Galeotta and F. Gasparo and E. Franceschi and R. C. Butler and F. Cuttaia and O. D'Arcangelo and S. Fogliani and A. Gregorio and R. Leonardi and S. R. Lowe and D. Maino and G. Maggio and M. Malaspina and N. Mandolesi and P. Manzato and P. Meinhold and L. Mendes and A. Mennella and G. Morgante and F. Pasian and F. Perrotta and M. Sandri and L. Stringhetti and L. Terenzi and M. Tomasi and A. Zonca},
  journal= {arXiv preprint arXiv:1001.4730},
  year   = {2010}
}

Comments

This paper is part of the Prelaunch status LFI papers published on JINST: http://www.iop.org/EJ/journal/-page=extra.proc5/jinst

R2 v1 2026-06-21T14:39:43.115Z