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author | Klaus Schmidinger <vdr@tvdr.de> | 2008-12-13 12:22:36 +0100 |
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committer | Klaus Schmidinger <vdr@tvdr.de> | 2008-12-13 12:22:36 +0100 |
commit | 3c7d1a16aca49c647320c0ee67759007fa06a845 (patch) | |
tree | e1e42d585ace0a9e94fdce643ae9bf265bc810c6 /vdr.5 | |
parent | 3abe4f2b91df3748acafce4bb90e7f296745f270 (diff) | |
download | vdr-3c7d1a16aca49c647320c0ee67759007fa06a845.tar.gz vdr-3c7d1a16aca49c647320c0ee67759007fa06a845.tar.bz2 |
Switched to the new S2API driver API; cDvbTuner::IsTunedTo()now also checks the symbol rate in case of DVB-S and DVB-C
Diffstat (limited to 'vdr.5')
-rw-r--r-- | vdr.5 | 16 |
1 files changed, 7 insertions, 9 deletions
@@ -8,7 +8,7 @@ .\" License as specified in the file COPYING that comes with the .\" vdr distribution. .\" -.\" $Id: vdr.5 2.4 2008/07/06 13:00:19 kls Exp $ +.\" $Id: vdr.5 2.5 2008/11/22 15:23:10 kls Exp $ .\" .TH vdr 5 "10 Feb 2008" "1.6" "Video Disk Recorder Files" .SH NAME @@ -83,22 +83,20 @@ meaning (and allowed values) are .TS tab (@); l l. -\fBA\fR@Alpha (0, 1, 2, 4) -\fBB\fR@Bandwidth (5, 6, 7, 8) -\fBC\fR@Code rate high priority (0, 12, 13, 14, 23, 25, 34, 35, 45, 56, 67, 78, 89, 910) -\fBD\fR@coDe rate low priority (0, 12, 13, 14, 23, 25, 34, 35, 45, 56, 67, 78, 89, 910) +\fBB\fR@Bandwidth (6, 7, 8) +\fBC\fR@Code rate high priority (0, 12, 23, 34, 35, 45, 56, 67, 78, 89, 910) +\fBD\fR@coDe rate low priority (0, 12, 23, 34, 35, 45, 56, 67, 78, 89, 910) \fBG\fR@Guard interval (4, 8, 16, 32) \fBH\fR@Horizontal polarization \fBI\fR@Inversion (0, 1) \fBL\fR@Left circular polarization -\fBM\fR@Modulation (0, 1, 2, 3, 4, 5, 6, 7, 8, 9, 10, 11, 16, 32, 64, 128, 256, 512, 998, 1024) +\fBM\fR@Modulation (2, 5, 6, 10, 11, 16, 32, 64, 128, 256, 998) \fBO\fR@rollOff (0, 20, 25, 35) -\fBP\fR@Priority (0, 1) \fBR\fR@Right circular polarization \fBS\fR@delivery System (0, 1) -\fBT\fR@Transmission mode (2, 4, 8) +\fBT\fR@Transmission mode (2, 8) \fBV\fR@Vertical polarization -\fBY\fR@hierarchY (0, 1) +\fBY\fR@hierarchY (0, 1, 2, 4) .TE The polarization parameters have no integer numbers following them. This is for |