Author: SM0TGU

Enligt nedanstående är transpondern igång denna vecka:

On December 21, 2015 at 1038 UT, the EO-79 transponder was turned on for a
prolonged period.

The FUNcube transponder subsystem on QB50p1 (EO-79) had been provided by AMSAT-
UK and AMSAT-NL and is a similar subsystem as on FUNcube-1, but without the
telemetry downlink circuitry.

The current software running on EO-79 does experience occasional reboots. When
these reboots happen, the transponder is automatically turned off and will have
to be turned back on by a command station. The FUNcube team has selected a few
command stations to do so, but be advised the transponder may be off.

TLEs:
AMSAT keps name: EO-79
Celestrak keps Name: QB50P1
Celestrak file: cubesat.txt
NORAD #    40025
COSPAR designator    2014-033-R

Frequencies:
*Uplink:* 435.035-435.065 MHz LSB [See note below]
*Downlink:* 145.935-145.965 MHz USB

EO-79 has been set to only beacon the normal AX.25 beacon every 30 seconds
instead of 10 seconds. The beacon frequency is 145.815 MHz and consists of AX.25
frames on BPSK. More details about the downlink can be found on the ISIS Ham
Radio page at http://isispace.nl/HAM/qb50p.html

We kindly request you to share your experiences with the AMSAT Bulletin Board so
everyone can benefit from operating tips and tricks, as well as being up-to-date
on the status.

We would also welcome any observation related to the transponder behaviour when
the AX.25 beacon comes on.

Just like FUNcube-1, the crystal oscillator circuits exhibit drift with
temperature. This means manual tuning will probably work best.

Mike Seguin N1JEZ notes:  I found my downlink after setting my uplink +12 kHz
from published spec

SatPC32 tracking software Doppler SQF information used by Peter VK4NBL:
EO-79,145950,435063,USB,LSB,REV,0,0
EO-79,145814.8,435070,CW,TELEMETRY,0,0

Lastly, the commanding team will not be available over Christmas, so the current
activations are planned from today until Thursday 24th and from Monday 28th
until Thursday 31st

[ANS thanks Wouter, PA3WEG, and AMSAT-UK for the above information]

På årets WRC (World Radiocommunication Conference) har en agenda för nästa WRC (år 2019) föreslagit att satelliter som ej främst är för amatörradiobruk inte bör (ska?) använda amatörradiobandet. Info från ANS nedan:

The World Radiocommunication Conference (WRC) held in Geneva during November
2015 has recommended an agenda for the next WRC, to be held in 2019, to the
Council of the International Telecommunication Union (ITU). One of the agenda
items is of particular interest to the small-satellite community.

Agenda item 1.7 for WRC-19 reads: “to study the spectrum needs for telemetry,
tracking and command in the space operation service for non-GSO satellites with
short duration missions, to assess the suitability of existing allocations to
the space operation service and, if necessary, to consider new allocations, in
accordance with Resolution COM6/19 (WRC-15).”

Resolution COM6/19, which eventually will be given a new number, specifies the
frequency ranges that may be considered for possible new allocations. They are
150.05-174 MHz and 400.15-420 MHz.

One of the factors that the conference considered in deciding on these
particular frequency ranges was “that some non-amateur satellites have used
frequencies for telemetry, tracking and command in the frequency bands 144-146
MHz and 435-438 MHz which are allocated to the amateur-satellite service, and
that such use is not in accordance with Nos. 1.56 and 1.57.” Those two
provisions of the ITU Radio Regulations define the amateur and amateur-
satellite services respectively.

The International Amateur Radio Union welcomed the exclusion from
consideration of all existing frequency allocations to the amateur and amateur-
satellite services. IARU President Tim Ellam, VE6SH, observed: “This is an
excellent result for the amateur services and clearly shows that non-amateur
satellite constructors need to consider spectrum other than the very limited
and congested segments that are available for amateur satellites at 144 MHz and
435 MHz.”

[ANS thanks IARU, ARRL, & AMSAT-UK for the above information]