| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 10705419 | Planetary and Space Science | 2005 | 15 Pages |
Abstract
In order to obtain correct results, the source-instrument-detector interaction is studied very accurately. The instrument variations during a pericentre pass impose a complex procedure for the LW channel calibration, but fortunately the procedure adopted seems to work well. Samples of the calibrated data are given (as single spectrum and as an average over a few spectra) to show the performance of the experiment and its scientific potentialities.
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Geophysics
Authors
M. Giuranna, V. Formisano, D. Biondi, A. Ekonomov, S. Fonti, D. Grassi, H. Hirsch, I. Khatuntsev, N. Ignatiev, M. Malgoska, A. Mattana, A. Maturilli, E. Mencarelli, F. Nespoli, R. Orfei, P. Orleanski, G. Piccioni, M. Rataj, L. Zasova,