The European Science Foundation is an association of its 67 member
research councils and academies in 23 countries. The ESF brings
European scientists together to work on topics of common concern, to
co-ordinate the use of expensive facilities, and to discover and
define new endeavors that will benefit from a co-operative approach
On behalf of European radio astronomers, the ESF
Committee on Radio Astronomy Frequencies, CRAF, coordinates activities
to keep the frequency bands used by radio astronomers free from interference.
The scientific work sponsored by ESF includes basic research in
the natural sciences, the medical and biosciences, the humanities and
the social sciences.
The ESF links scholarship and research
supported by its members and adds value by cooperation across national
frontiers. Through its function as coordinator, and also by holding
workshops and conferences and by enabling researchers to visit and
study in laboratories throughout Europe, the ESF works for the
advancement of European science.
Paris, 27-28 January 2000
Subject: This liaison statement is in response to the liaison letter ETSI/TC-SES sent to CEPT SE PT28 (June 24, 1999).
SE28 discussed the protection of the Radio Astronomy Service in the band 1660-1670 MHz from harmful interference from AESs operating the band 1626.5-1660.5 MHz. An analysis was carried out by Inmarsat and accepted by CRAF. This statistical approach is based on the density of aircraft within a certain simulation area considered to be sufficiently large to encompass all potential interfering aircraft, the number of aircraft equipped with Satcom, the utilisation rate of AESs, and the probability of 2 simultaneous calls from the same terminal. This approach shows that with a reduction of the unwanted emission level, the radio astronomy protection criteria will be met.
SE28 therefore recommends to change the power output levels stated in the DEN/SES-00023 v.1.1.5, Section 9, table 13 as follows:
| Frequency band | 1660-1670 MHz | |
| Narrow band spurious | -49.5 dBW | for a reference bandwidth of 20 kHz |
| Wide band spurious | -39.5 dBW | for a reference bandwidth of 1 MHz |
These new levels being applicable to Harmonics, Spurious and Noisy density levels produced by an AES operating in the 1626.5-1660.5 MHz band.
It has been pointed out that such complete statistical analysis had not been performed for the assessment of the unwanted emission level from AES falling into the band 1610.6-1613.8 MHz and that, consequently, the value of -80 dBW/MHz which had been previously proposed to TC SES for this band might be unduly constraining. In absence of planned further SE28 meeting, the two parties which were involved in this earlier study, CRAF and Iridium, have been invited to carry out a full statistical analysis and to agree on some proposal to be submitted directly to the resolution meeting on DEN/SES-00023.
The drafting group distinguished the following aspects:
i. Uplink MSS in the band 1614-1626.5 MHz versus uplink MES in the band
1626.5-1660.5 MHz:
SE28 noted that the issue was not discussed by WP8D as indicated in footnote 1 to
document ITU-R 8/128-E. SE28 considers that, as far as possible, the AES unwanted
emission power below 1626.5 MHz should be made close to the one agreed in SG8 for
non AES terminals. The AES density, which is expected to be lower than the density
of handset stations, will guarantee that their interference will not significantly add
up on the aggregate interference level from land mobile earth stations.
ii. Two AESs on the same aircraft:
SE28 considers that this is an issue for ICAO.