national science foundation 1 andrew clegg u.s. national science foundation [email protected] third...
TRANSCRIPT
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Andrew CLEGGU.S. National Science Foundation
Third Summer School on Spectrum Management for Radio AstronomyTokyo, Japan – June 3, 2010
Digital TV and Its Impact onRadio Astronomy
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nAnalog Television Terrestrial
Broadcasting Standards
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Abbrev Name Main Geographic Use
PAL Phase Alternating Line Most of Europe, Australia, Parts of Asia (including India & China), Most of Africa, Eastern South America
NTSC National Television System Committee
North & Central America, Western South America, Japan, Philippines, Thailand, Taiwan, South Korea
SECAM Sequential Color with Memory
France, Russia & former Soviet republics, portions of Africa, Madagascar
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nAnalog TV Standards Worldwide
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nDigital Television Worldwide
• Worldwide, terrestrial TV broadcasts are switching from analog to digital modulation> Different countries have different schedules for
switching over (most by 2015)> Some satellite TV broadcasting has been digital for
more than 15 years
• Japan is deploying ISDB-T technology, replacing NTSC and analog HDTV MUSE standards> ISDB-T also being widely deployed in South America
• North America is deploying ATSC digital TV to replace NTSC analog standard> U.S. digital transition is completed for “full-service”
broadcasts; legacy NTSC remains for low-power stations
• Australia and Europe are deploying DVB-T
• China is rolling its own (DMB-T)4
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n Digital TV Terrestrial Broadcasting Standards
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Abbrev NameOver-the-Air Modulation Type
Main Geographic Use
DVB-T Digital Video Broadcasting – Terrestrial
Coded Orthogonal Frequency Division Multiplexing (COFDM) (QPSK, 16QAM, and 64QAM)
Europe, Russia, Australia, Parts of Asia
ISDB-T Integrated Services Digital Broadcasting - Terrestrial
Coded Orthogonal Frequency Division Multiplexing (COFDM) (DQPSK, QPSK, 16QAM, and 64QAM)
Japan, South America (ISDB-T International)
ATSC Advanced Television Systems Committee
8-level Vestigial Sideband (8VSB)
North America, South Korea
DMB-T/H Digital Multimedia Broadcast – Terrestrial/Handheld
Time Domain Synchronous Orthogonal Frequency Division Multiplexing (TDS-OFDM)
China only
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nDigital TV Standards Worldwide
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nDigital Transition Worldwide
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Completed, no analog / Completed for full-service stations / In transition /Planned / No transition planned / No Information
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n TV Spectra
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DVB-T (OFDM)
ISDB-T (Yellow) (OFDM)
DigitalAnalog
PAL / SECAM / NTSC Generic(All have video, chrominance, and audio
carriers. Some differences in total bandwidth and frequency offset between carriers.)
ATSC(8-VSB)
PAL
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Maximum Transmit Power (U.S.)
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Chan Freq (MHz)Maximum Analog
EIRP (kW)Maximum Digital
EIRP (kW)
2 – 6 54 – 72 & 76 – 88 164 74
7 – 13 174 – 216 518 262
14 – 51 470 – 698 8222 1640
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nDTV Unwanted Emissions Limits (U.S.)
(Assumes full-power 1640 kW EIRP)
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Fig. 1.14.5: Unwanted Emissions Limits for a Full-Power (1640 kW EIRP)Digital TV Signal
-110
-100
-90
-80
-70
-60
-50
-40
0 1 2 3 4 5 6 7 8 9 10
Frequency Offset from Channel Edge (MHz)
EIR
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[dB
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n Comparison of Analog (NTSC) and Digital (ATSC) TV Signal Spectra
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Direct comparison of digital (8-VSB modulation, left) and analog (AM-VSB, PM, and FM, right) TV signals, of the same station from the same tower at the same time. The analog signal has more power because of the large video carrier, but the digital signal fills in the spectrum completely.
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n Comparison of Digital (ATSC) and Analog (NTSC) Signals
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n Ratio of Power Spectral Density of Digital (ATSC) to Analog (NTSC)
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n Ratio of Power Spectral Density of Digital to Analog (detail)
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Detail of DTV/Analog TV
0
1
2
3
4
5
6
7
8
9
10
0.000 1.000 2.000 3.000 4.000 5.000 6.000
Frequency Offset from Bottom of Channel (MHz)
(DTV
PSD
)/(An
alog
TV
PSD)
For equivalent digital and analog TV signals, the digital
power spectral density exceeds the analog PSD over 94% of the bandwidth, and by
as much as 3 orders of magnitude.
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nHow to Identify TV Signal
Technology Bandwidth Most dominant spectral characteristic Secondary spectral characteristic Other spectral characteristic(s)
NTSC (analog; System M) 6 MHz
Strong video carrier peaked at 1.25 MHz above bottom channel edge. When tuned in AM mode on an appropriate receiver, sounds like a buzzing sound that changes with changes in the TV picture.
FM audio carrier 5.75 MHz above bottom edge of channel (250 kHz below top edge). Audio can be clearly monitored in wideband FM mode with appropriate radio receiver.
Chrominance carrier (phase and amplitude modulated) 4.829545 MHz above bottom of channel.
PAL (analog; Southern Africa; System I) 8 MHz
Strong video carrier peaked at 1.25 MHz above bottom channel edge. When tuned in AM mode on an appropriate receiver, sounds like a buzzing sound that changes with changes in the TV picture.
FM audio carrier 7.2496 MHz above bottom edge of channel (250 kHz below top edge). Audio can be clearly monitored in wideband FM mode with appropriate radio receiver.
Chrominance carrier 5.68361875 MHz above bottom-edge of channel.
PAL (analog; Australia; System B) 7 MHz
Strong video carrier peaked at 1.25 MHz above bottom channel edge. When tuned in AM mode on an appropriate receiver, sounds like a buzzing sound that changes with changes in the TV picture.
FM audio carrier 6.75 MHz above bottom edge of channel (250 kHz below top edge). Audio can be clearly monitored in wideband FM mode with appropriate radio receiver.
Chrominance carrier 5.68361875 MHz above bottom-edge of channel.
ATSC (digital) 6 MHz
Flat spectrum except very narrow pilot tone carrier approximately 309.4 kHz above bottom edge of channel. Pilot tone can be heard in CW mode of an appropriate radio receiver, otherwise rest of signal just sounds like gaussian noise.
ISDB-T, DVB-T (digital) 6, 7, & 8 MHzFlat spectrum, OFDM. No significant spectral features. Identified by frequency and bandwidth.
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Digital and Analog TV in Mitaka
Japanese NTSC TV broadcast on channel 3 (102 – 108 MHz).
Video carrier (103.25 MHz)
Color carrier(106.78 MHz)
Audio carrier(107.75 MHz)
Japanese ISDB-T broadcasts on channels 25, 26, & 27 (542 – 560 MHz)
Channel 26(548 – 554 MHz)
Channel 25(542 – 548 MHz) Channel 27
(554 – 560 MHz)
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n Observational Comparison ofDigital and Analog TV Interference
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nTelevision Interference Caused by Anomalous
Propagation at the Murchison Widefield Array Site
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Digital TV signal in Australian channel 7 (181 – 188 MHz), and narrowband interference from analog (PAL) luminance, chrominance, and audio carriers of channels 6 (174 – 181 MHz),
8 (188 – 195 MHz), and (partially) 9 (195-202 MHz). The digital TV signal is believed to be arising from a distance of 290 km during a period of anomalous propagation. Data obtained in March 2010.
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nTV Broadcasts and Rec. 769
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Digital TV and Redshifted HI
Fig. 1.14.2: U.S. Television Channels After Feb 17, 2009 Digital TV TransitionV
HF
UH
F
MHzz(HI)
5425.3
2
6022.7
3
6620.5
4
7218.7
7617.7
5
8216.3
6
8815.1
~
1747.2
7
1806.9
8
1866.6
9
1926.4
10
1986.2
11
2046.0
12
2105.8
13
2165.6
MHzz(HI)
4702.02
14
4761.98
15
4821.95
16
4881.91
17
4941.88
18
5001.84
19
5061.81
20
5121.77
21
5181.74
22
5241.71
23
5301.68
24
5361.65
25
5421.62
26
5481.59
27
5541.56
MHzz(HI)
5541.56
28
5601.54
29
5661.51
30
5721.48
31
5781.46
32
5841.43
33
5901.41
34
5961.38
35
6021.36
36
6081.34
6141.31
38
6201.29
39
6261.27
40
6321.25
41
6381.23
MHzz(HI)
6381.23
42
6441.21
43
6501.19
44
6561.17
45
6621.15
46
6681.13
47
6741.11
48
6801.09
49
6861.07
50
6921.05
51
6981.03
52
7041.02
53
7101.00
54
7160.98
55
7220.97
MHzz(HI)
7220.97
56
7280.95
57
7340.94
58
7400.92
59
7460.90
60
7520.89
61
7580.87
62
7640.86
63
7700.84
64
7760.83
65
7820.82
66
7880.80
67
7940.79
68
8000.78
69
8060.76
Allocated to radio astronomy. Not used for TV.
Used for land mobile instead of TV in some major cities.Reallocated to mobile and f ixed use.
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n Worldwide Lower VHF Channel Plans
21Figure from Wikipedia, based on data from “World Analogue Television Standards and Waveforms” (http://www.pembers.freeserve.co.uk/World-TV-Standards/Transmission-Systems.html)
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n Worldwide Upper VHF Channel Plans
22Figure from Wikipedia, based on data from “World Analogue Television Standards and Waveforms” (http://www.pembers.freeserve.co.uk/World-TV-Standards/Transmission-Systems.html)
See color key onprevious slide
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n Comparison of Analog and DTV Channel Allotments
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• Allotments specify which channels are available for use in each city or market area> Allotments are based on market size, co- and adjacent-
channel interference criteria, geography, frequency, and other considerations
• Given the lucrative nature of a TV license, virtually all allotted channels are spoken for
• There are significant differences between the DTV allotments after the transition and the analog allotments prior to the transition
• A comparison of the allotment tables provides a quick snapshot of the imminent changes in the spectrum landscape.
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Number of Analog TV Allotments Per Channel Prior to DTV Transition
58
61
64
5658
6161
565757
58
68
3030
27272726
28
3230
3334
26
31
27
22
25
22
1817
25
2122
24
0
20
17
22
141616
1918
19
1615
21
1818
1312
16
10
1312
13
79
1012
79
6
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6
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2 4 6 8 10 12 14 16 18 20 22 24 26 28 30 32 34 36 38 40 42 44 46 48 50 52 54 56 58 60 62 64 66 68
TV Channel
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Σ = 1756
Analog TV AllotmentsBefore DTV Transition
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Digital TV AllotmentsAfter DTV Transition
Number of Digital TV Allotments Per Channel After DTV Transition
7 7
2
13
8
68
6361
68
5757
76
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40
3436
37
48
3940
414141
31
4140
38
35
32
36
41
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29
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3331
3031
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27
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0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 00
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2 4 6 8 10 12 14 16 18 20 22 24 26 28 30 32 34 36 38 40 42 44 46 48 50 52 54 56 58 60 62 64 66 68
TV Channel
Nu
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igit
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V S
tati
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All
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Σ = 1811
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Difference between Digital and Analog TV Allotments
Change in TV Allotments Per Channel After DTV Transition
-200%
-150%
-100%
-50%
0%
50%
100%
150%
200%
2 4 6 8 10 12 14 16 18 20 22 24 26 28 30 32 34 36 38 40 42 44 46 48 50 52 54 56 58 60 62 64 66 68
% C
han
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( ND
TV -
NA
nal
og)/N
An
alo
g
Lower VHF, Chs 2 - 6 (54 - 72 & 76 - 88 MHz)
Upper VHF, Chs 7 - 13(174 - 216 MHz)
UHF Chs 14 - 51 (470 ~ 698 MHz)
No longer used, Chs 52 - 69 (698 - 806 MHz)
Ch 37 (608 - 614 MHz)(not used for TV)
ΔN = +55
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n Summary• The world is switching to digital terrestrial TV
broadcasting
• Digital TV produces more apparent interference than analog TV
• Both digital TV and (in some countries) the refarming of TV broadcast spectrum will make observations using TV band frequencies more challenging
• TV interference is most disruptive to the search for highly redshifted HI, such as the search for the Epoch of Reionization (EOR)
• TV interference in general, and digital TV interference in particular, have been shown to impact radio observatories hundreds of km from the transmitting source
• Radio astronomers can generally not expect any regulatory protections when using TV spectrum for observing
• Future instruments such as the SKA must take TV interference into account 27