evn vlbi [email protected] tow may 2017 · n17c1 jive 6cm nme 512 0.69 l+r 6cm nme + ftp-ft. cl17c1...
TRANSCRIPT
EVN e-VLBI TOW May [email protected]
EVN e-VLBI TOW May [email protected]
EVN e-VLBI TOW May [email protected]
Intarwebs
EVN e-VLBI TOW May [email protected]
Intarwebs
EVN e-VLBI TOW May [email protected]
Harro Verkouter
EVN e-VLBI TOW May [email protected]
Real-time VLBI!
• anything/anyone **** up?
• anything/anyone not keeping up?
you lose science data!
you lose science data!
EVN e-VLBI TOW May [email protected]
EVN e-VLBI TOW May [email protected]
Why on earth e-VLBI?
EVN e-VLBI TOW May [email protected]
EVN e-VLBI TOW May [email protected]
Why on earth e-VLBI?
1. Address time scaleget data to scientist faster
EVN e-VLBI TOW May [email protected]
Why on earth e-VLBI?
1. Address time scaleget data to scientist faster
2. Reliabilitydetect + fix errors before science run
EVN e-VLBI TOW May [email protected]
Sensitivity
EVN e-VLBI TOW May [email protected]
Sensitivity ∼ 1 ∕σT
EVN e-VLBI TOW May [email protected]
Tsys
√(∆ν ⋅ ∆t)σT =
σT noise∆ν bandwidth
∆t integration time
Sensitivity ∼ 1 ∕σT
EVN e-VLBI TOW May [email protected]
Tsys
√(∆ν ⋅ ∆t)σT =
σT noise∆ν bandwidth
∆t integration time
Sensitivity ∼ 1 ∕σT
EVN e-VLBI TOW May [email protected]
Tsys
√(∆ν ⋅ ∆t)σT =
σT noise∆ν bandwidth
∆t integration time
Sensitivity ∼ 1 ∕σT
∆ν☝︎ ⇒σT☟
EVN e-VLBI TOW May [email protected]
Sensitivity ∼ 1 ∕σT
Recorded data rate ∆ Sensitivity (wrt 1Gbps)1 Gbps + 0%2 Gbps + 41.4213562...%4 Gbps + 100%
EVN e-VLBI TOW May [email protected]
Sensitivity ∼ 1 ∕σT
`whole’ EVN equipped with• DBBC2• FiLa10G
⇒ 4Gbps capable
EVN e-VLBI TOW May [email protected]
F17L1 JIVE 18cm FTP-FT 512 0.23 L+R 18cm FTP Fringe TestEP103A Paragi FRB121102 1024 5.99 L+R 18cmCL17L1 Gunn 18cm FS CAL ---- 0.00 L+R 18cm Amplitude Calibration EM127A Maan B0525+21 1024 3.26 L+R 21cmEM127B Maan B2045-16 1024 2.53 L+R 21cmEK036C Kirsten Crab Nebula 1024 0.92 L+R 18cm 3rd epoch N17L1 JIVE 18cm NME 512 0.69 L+R 18cm NME + FTP-FTGV022A Varenius Arp 220 2048 11.06 L+R 18cm +VLBA+Y27EP102 Paragi J0959+1259 1024 4.61 L+R 18cm +eMERLINN17C1 JIVE 6cm NME 512 0.69 L+R 6cm NME + FTP-FTCL17C1 Gunn 6cm FS CAL ---- 0.00 L+R 6cm Amplitude CalibrationEP103B Paragi FRB121102 2048 11.06 L+R -EL056 Landoni SDSS 0040-0915 2048 5.53 L+R -N17P1 JIVE 90cm NME 256 0.35 L+R 90cm NME + FTP-FTCL17P1 Gunn 90cm FS CAL ---- 0.00 L+R 90cm Amplitude CalibrationGK049C Kirsten B1133+16 256 2.88 L+R +GBT+Y27 B1133+16GK049D Kirsten B1737+13 256 2.88 L+R +GBT+Y27 B1737+13F17K1 JIVE 1.3cm FTP-FT 1024 0.46 L+R 1.3cm FTP Fringe TestGG081C Gomez AGN Jets 1024 6.91 L+R 1.3cm EVN+RA OJ287EC057B Cutini S51803+78 128 0.35 L+R 2nd epochN17K1 JIVE 1.3cm NME 1024 0.69 L+R 1.3cm NME + FTP-FTGG081D Gomez AGN Jets 1024 0.46 L+R +RA 0823+033GG081E Gomez AGN Jets 1024 0.69 L+R +RA OJ287GG081F Gomez AGN Jets 1024 0.69 L+R +RA+VLBA (HnScNl) OJ287GG081G Gomez AGN Jets 1024 0.46 L+R VLBA ONLY+RA 0823+033 EB060A Bach Cygnus A 1024 4.61 L+R -GG081H Gomez AGN Jets 1024 0.69 L+R VLBA ONLY +RA OJ287CL17K1 Gunn 1.3cm FS CAL ---- 0.00 L+R 1.3cm Amplitude CalibrationGG081I Gomez AGN Jets 1024 0.69 L+R +RA OJ287GG081J Gomez AGN Jets 1024 0.69 L+R +RA+VLBA (HnScNl) OJ287F17Q1 JIVE 0.7cm FTP-FT 1024 0.46 L+R 0.7cm FTP Fringe TestGK050 Koyama Mrk 501 1024 6.91 L+R 0.7cm +VLBAEP101A Pilhstrom Q-band Calibrators 1024 0.46 L+R 0.7cm field 1EP101B Pilhstrom Q-band Calibrators 1024 0.92 L+R 0.7cm field 2EP101C Pilhstrom Q-band Calibrators 1024 0.46 L+R 0.7cm field 1EP101D Pilhstrom Q-band Calibrators 1024 0.92 L+R 0.7cm field 2GG081L Gomez AGN Jets 1024 0.69 L+R 1.3cm VLBA ONLY +RA OJ287GA032D Agudo NRAO 150 1024 5.33 L+R 0.7cm +VLBAEP101E Pilhstrom Q-band Calibrators 1024 0.46 L+R 0.7cm field 1EP101F Pilhstrom Q-band Calibrators 1024 0.92 L+R 0.7cm field 2N17Q1 JIVE 0.7cm NME 1024 1.38 L+R 0.7cm NME + FTP-FTCL17Q1 Gunn 0.7cm FS CAL ---- 0.00 L+R 0.7cm Amplitude CalibrationEP101G Pilhstrom Q-band Calibrators 1024 0.46 L+R 0.7cm field 1EP101H Pilhstrom Q-band Calibrators 1024 0.92 L+R 0.7cm field 2
EV
N S
ession I/2017
EVN e-VLBI TOW May [email protected]
F17L1 JIVE 18cm FTP-FT 512 0.23 L+R 18cm FTP Fringe TestEP103A Paragi FRB121102 1024 5.99 L+R 18cmCL17L1 Gunn 18cm FS CAL ---- 0.00 L+R 18cm Amplitude Calibration EM127A Maan B0525+21 1024 3.26 L+R 21cmEM127B Maan B2045-16 1024 2.53 L+R 21cmEK036C Kirsten Crab Nebula 1024 0.92 L+R 18cm 3rd epoch N17L1 JIVE 18cm NME 512 0.69 L+R 18cm NME + FTP-FTGV022A Varenius Arp 220 2048 11.06 L+R 18cm +VLBA+Y27EP102 Paragi J0959+1259 1024 4.61 L+R 18cm +eMERLINN17C1 JIVE 6cm NME 512 0.69 L+R 6cm NME + FTP-FTCL17C1 Gunn 6cm FS CAL ---- 0.00 L+R 6cm Amplitude CalibrationEP103B Paragi FRB121102 2048 11.06 L+R -EL056 Landoni SDSS 0040-0915 2048 5.53 L+R -N17P1 JIVE 90cm NME 256 0.35 L+R 90cm NME + FTP-FTCL17P1 Gunn 90cm FS CAL ---- 0.00 L+R 90cm Amplitude CalibrationGK049C Kirsten B1133+16 256 2.88 L+R +GBT+Y27 B1133+16GK049D Kirsten B1737+13 256 2.88 L+R +GBT+Y27 B1737+13F17K1 JIVE 1.3cm FTP-FT 1024 0.46 L+R 1.3cm FTP Fringe TestGG081C Gomez AGN Jets 1024 6.91 L+R 1.3cm EVN+RA OJ287EC057B Cutini S51803+78 128 0.35 L+R 2nd epochN17K1 JIVE 1.3cm NME 1024 0.69 L+R 1.3cm NME + FTP-FTGG081D Gomez AGN Jets 1024 0.46 L+R +RA 0823+033GG081E Gomez AGN Jets 1024 0.69 L+R +RA OJ287GG081F Gomez AGN Jets 1024 0.69 L+R +RA+VLBA (HnScNl) OJ287GG081G Gomez AGN Jets 1024 0.46 L+R VLBA ONLY+RA 0823+033 EB060A Bach Cygnus A 1024 4.61 L+R -GG081H Gomez AGN Jets 1024 0.69 L+R VLBA ONLY +RA OJ287CL17K1 Gunn 1.3cm FS CAL ---- 0.00 L+R 1.3cm Amplitude CalibrationGG081I Gomez AGN Jets 1024 0.69 L+R +RA OJ287GG081J Gomez AGN Jets 1024 0.69 L+R +RA+VLBA (HnScNl) OJ287F17Q1 JIVE 0.7cm FTP-FT 1024 0.46 L+R 0.7cm FTP Fringe TestGK050 Koyama Mrk 501 1024 6.91 L+R 0.7cm +VLBAEP101A Pilhstrom Q-band Calibrators 1024 0.46 L+R 0.7cm field 1EP101B Pilhstrom Q-band Calibrators 1024 0.92 L+R 0.7cm field 2EP101C Pilhstrom Q-band Calibrators 1024 0.46 L+R 0.7cm field 1EP101D Pilhstrom Q-band Calibrators 1024 0.92 L+R 0.7cm field 2GG081L Gomez AGN Jets 1024 0.69 L+R 1.3cm VLBA ONLY +RA OJ287GA032D Agudo NRAO 150 1024 5.33 L+R 0.7cm +VLBAEP101E Pilhstrom Q-band Calibrators 1024 0.46 L+R 0.7cm field 1EP101F Pilhstrom Q-band Calibrators 1024 0.92 L+R 0.7cm field 2N17Q1 JIVE 0.7cm NME 1024 1.38 L+R 0.7cm NME + FTP-FTCL17Q1 Gunn 0.7cm FS CAL ---- 0.00 L+R 0.7cm Amplitude CalibrationEP101G Pilhstrom Q-band Calibrators 1024 0.46 L+R 0.7cm field 1EP101H Pilhstrom Q-band Calibrators 1024 0.92 L+R 0.7cm field 2
EV
N S
ession I/2017
EVN e-VLBI TOW May [email protected]
F17L1 JIVE 18cm FTP-FT 512 0.23 L+R 18cm FTP Fringe TestEP103A Paragi FRB121102 1024 5.99 L+R 18cmCL17L1 Gunn 18cm FS CAL ---- 0.00 L+R 18cm Amplitude Calibration EM127A Maan B0525+21 1024 3.26 L+R 21cmEM127B Maan B2045-16 1024 2.53 L+R 21cmEK036C Kirsten Crab Nebula 1024 0.92 L+R 18cm 3rd epoch N17L1 JIVE 18cm NME 512 0.69 L+R 18cm NME + FTP-FTGV022A Varenius Arp 220 2048 11.06 L+R 18cm +VLBA+Y27EP102 Paragi J0959+1259 1024 4.61 L+R 18cm +eMERLINN17C1 JIVE 6cm NME 512 0.69 L+R 6cm NME + FTP-FTCL17C1 Gunn 6cm FS CAL ---- 0.00 L+R 6cm Amplitude CalibrationEP103B Paragi FRB121102 2048 11.06 L+R -EL056 Landoni SDSS 0040-0915 2048 5.53 L+R -N17P1 JIVE 90cm NME 256 0.35 L+R 90cm NME + FTP-FTCL17P1 Gunn 90cm FS CAL ---- 0.00 L+R 90cm Amplitude CalibrationGK049C Kirsten B1133+16 256 2.88 L+R +GBT+Y27 B1133+16GK049D Kirsten B1737+13 256 2.88 L+R +GBT+Y27 B1737+13F17K1 JIVE 1.3cm FTP-FT 1024 0.46 L+R 1.3cm FTP Fringe TestGG081C Gomez AGN Jets 1024 6.91 L+R 1.3cm EVN+RA OJ287EC057B Cutini S51803+78 128 0.35 L+R 2nd epochN17K1 JIVE 1.3cm NME 1024 0.69 L+R 1.3cm NME + FTP-FTGG081D Gomez AGN Jets 1024 0.46 L+R +RA 0823+033GG081E Gomez AGN Jets 1024 0.69 L+R +RA OJ287GG081F Gomez AGN Jets 1024 0.69 L+R +RA+VLBA (HnScNl) OJ287GG081G Gomez AGN Jets 1024 0.46 L+R VLBA ONLY+RA 0823+033 EB060A Bach Cygnus A 1024 4.61 L+R -GG081H Gomez AGN Jets 1024 0.69 L+R VLBA ONLY +RA OJ287CL17K1 Gunn 1.3cm FS CAL ---- 0.00 L+R 1.3cm Amplitude CalibrationGG081I Gomez AGN Jets 1024 0.69 L+R +RA OJ287GG081J Gomez AGN Jets 1024 0.69 L+R +RA+VLBA (HnScNl) OJ287F17Q1 JIVE 0.7cm FTP-FT 1024 0.46 L+R 0.7cm FTP Fringe TestGK050 Koyama Mrk 501 1024 6.91 L+R 0.7cm +VLBAEP101A Pilhstrom Q-band Calibrators 1024 0.46 L+R 0.7cm field 1EP101B Pilhstrom Q-band Calibrators 1024 0.92 L+R 0.7cm field 2EP101C Pilhstrom Q-band Calibrators 1024 0.46 L+R 0.7cm field 1EP101D Pilhstrom Q-band Calibrators 1024 0.92 L+R 0.7cm field 2GG081L Gomez AGN Jets 1024 0.69 L+R 1.3cm VLBA ONLY +RA OJ287GA032D Agudo NRAO 150 1024 5.33 L+R 0.7cm +VLBAEP101E Pilhstrom Q-band Calibrators 1024 0.46 L+R 0.7cm field 1EP101F Pilhstrom Q-band Calibrators 1024 0.92 L+R 0.7cm field 2N17Q1 JIVE 0.7cm NME 1024 1.38 L+R 0.7cm NME + FTP-FTCL17Q1 Gunn 0.7cm FS CAL ---- 0.00 L+R 0.7cm Amplitude CalibrationEP101G Pilhstrom Q-band Calibrators 1024 0.46 L+R 0.7cm field 1EP101H Pilhstrom Q-band Calibrators 1024 0.92 L+R 0.7cm field 2
EV
N S
ession I/2017
EVN e-VLBI TOW May [email protected]
EVN Sensitivity
> 1Gbps observations sparsesolely
due to recording media shortage!
EVN e-VLBI TOW May [email protected]
Why on earth e-VLBI?
1. Address time scaleget data to scientist faster
2. Reliabilitydetect + fix errors before science run
3. Sensitivity/capacitynot limited by recording media any more
EVN e-VLBI TOW May [email protected]
Why on earth e-VLBI?
1. Address time scaleget data to scientist faster
2. Reliabilitydetect + fix errors before science run
3. Sensitivity/capacitynot limited by recording media any more
4. FUN!!playing with novel technologies!
EVN e-VLBI TOW May [email protected]
CORIntarwebs
EVN e-VLBI TOW May [email protected]
Intarwebs
EVN e-VLBI TOW May [email protected]
EVN e-VLBI TOW May [email protected]
Intarwebs
EVN e-VLBI TOW May [email protected]
EVN e-VLBI TOW May [email protected]
EVN e-VLBI TOW May [email protected]
Intarwebs
EVN e-VLBI TOW May [email protected]
Intarwebs
EVN e-VLBI TOW May [email protected]
Intarwebs
EVN e-VLBI TOW May [email protected]
Thus: e-VLBI necessities1. get your `telescope’ connected
• fix “last mile problem”• 2017: sometimes still prohibitively expensive!
• may need sucking up to Research Network Provider• some charge commercial rates:
• ~ few 1000 currency units / time unit / bandwidth• 2017: sometimes still prohibitively expensive!
• sometimes even political issues i.s.o. money
2. switch to Mark5 recorder or newer
Any of these fail, you can forget it
EVN e-VLBI TOW May [email protected]
CORIntarwebs
EVN e-VLBI TOW May [email protected]
Simplified network diagram!
EVN e-VLBI TOW May [email protected]
Simplified network diagram!
EVN e-VLBI TOW May [email protected]
EVN e-VLBI TOW May [email protected]
Intarwebs
EVN e-VLBI TOW May [email protected]
Intarwebs
EVN e-VLBI TOW May [email protected]
control s/w
Mark5 system
mem
Anatomy of Mark5
PCI bus
I/O board
StreamstorCard
bank a bank b
EVN e-VLBI TOW May [email protected]
control s/w
Mark5 system
PCI bus
I/O board
StreamstorCard
bank a bank b
disk
in
net
file
record = on / off
EVN e-VLBI TOW May [email protected]
control s/w
Mark5 system
mem
in2net = on / off
PCI bus
I/O board
StreamstorCard
bank a bank b
disk
in
net
file
EVN e-VLBI TOW May [email protected]
• TCP• TCP BIC• TCP Reno• ...
Started off with TCP
Long fat pipes: large BW x delay producte.g. RTT Netherlands - Australia ~ 270ms⇒ unfavourable for TCP
EVN e-VLBI TOW May [email protected]
EVN e-VLBI TOW May [email protected]
EVN e-VLBI TOW May [email protected]
“let’s try udp”
we were in for a few surprises ...
• connections were dedicated light paths• did not have to be very polite to other users• we can tolerate loss of ~ few % easily
• our data is pure noise!
EVN e-VLBI TOW May [email protected]
Current:
for( pkt=0; pkt<npkt; pkt++) {write(socket, data, 1500);
}
The n00b does UDP ...
EVN e-VLBI TOW May [email protected]
Current:
• packets don’t even leave the Mark5! • udp has no rate control/feedback (handled by O/S for tcp)
• kernel: no obligation to actually deliver the packet(s) ...• sender overwrites own send buffer ...• have to invent ingestion rate control
The n00b does UDP ...
EVN e-VLBI TOW May [email protected]
δt
Use Linux nanosleep() system call:
for( pkt=0; pkt<npkt; pkt++) {write(socket, data, 1500);nanosleep( delta_t );
}
For 1Gbps/MTU1500 delta_t(δt) is ~12 microseconds.Linux not real-time O/S:
threads only scheduled every 10ms (100Hz)!
n00b reads manpage
EVN e-VLBI TOW May [email protected]
δt (~10ms)!
Use Linux nanosleep() system call:
for( pkt=0; pkt<npkt; pkt++) {write(socket, data, 1500);nanosleep( delta_t );
}
n00b reads manpage
EVN e-VLBI TOW May [email protected]
δt
Use (pseudo) calibrated busy-loop:
int N = delta_t * counts_per_microsecond;
for( pkt=0; pkt<npkt; pkt++) {write(socket, data, 1500);for(int dummy=0; dummy<N; dummy++);
}
n00b thinks he smart
EVN e-VLBI TOW May [email protected]
δt (random)
Use (pseudo) calibrated busy-loop:
int N = delta_t * counts_per_microsecond;
for( pkt=0; pkt<npkt; pkt++) {write(socket, data, 1500);for(int dummy=0; dummy<N; dummy++);
}
n00b thinks he smart
EVN e-VLBI TOW May [email protected]
δt (random)
Use (pseudo) calibrated busy-loop:
int N = delta_t * counts_per_microsecond;
for( pkt=0; pkt<npkt; pkt++) {write(socket, data, 1500);for(int dummy=0; dummy<N; dummy++);
}
n00b thinks he smart
EVN e-VLBI TOW May [email protected]
δt
Use wallclock time; busy wait until time for next packet:
for( pkt=0; pkt<npkt; pkt++) {// remember time of sendingtime_sent = gettimeofday();// send packetwrite(socket, data, 1500);// wait for wallclock time to pass ...time_next = time_sent + delta_t;while( gettimeofday() < time_next ) {}
}
n00b don’t give up
EVN e-VLBI TOW May [email protected]
δt
Use wallclock time; busy wait until time for next packet:
for( pkt=0; pkt<npkt; pkt++) {// remember time of sendingtime_sent = gettimeofday();// send packetwrite(socket, data, 1500);// wait for wallclock time to pass ...time_next = time_sent + delta_t;while( gettimeofday() < time_next ) {}
}
n00b don’t give up
EVN e-VLBI TOW May [email protected]
δt
Use wallclock time; busy wait until time for next packet:
for( pkt=0; pkt<npkt; pkt++) {// remember time of sendingtime_sent = gettimeofday();// send packetwrite(socket, data, 1500);// wait for wallclock time to pass ...time_next = time_sent + delta_t;while( gettimeofday() < time_next ) {}
}
n00b now know how!
EVN e-VLBI TOW May [email protected]
EVN e-VLBI TOW May [email protected]
0 1 2 3 4 5 6 97 8
So far only sender side!
UDP = no guarantees:packet losspacket reordering
Sender sends in sequence:
4 1 3 5 6 7 9 138 12Receiver gets this:
EVN e-VLBI TOW May [email protected]
0 1 2 3 4 5 6 97 8
Put back in order
4 1 3 5 6 7 9 138 12
Sender sends in sequence:
Receiver gets this:
receiver must do this in real-time
FF
EVN e-VLBI TOW May [email protected]
Put back in order• 3 generations of algorithm, up to 2048Mbps
• initializes buffer by overwriting (memcpy)• lots of statistics:
• reordering amount (RFC4737-ish)• loss statistics etc.
• 4th generation good up to 8192Mbps test• do not initialize• flag positions with data• only overwrite locations w/o data
• memory touched exactly once• still all statistics
EVN e-VLBI TOW May [email protected]
Intarwebs
EVN e-VLBI TOW May [email protected]
CORIntarwebs
EVN e-VLBI TOW May [email protected]
CORIntarwebs
EVN e-VLBI TOW May [email protected]
bsNeed Nsta ⋅ x Gbps
EVN e-VLBI TOW May [email protected]
bs1 x 40Gbps Haystack
EVN e-VLBI TOW May [email protected]
bs3 x 10Gbps JIVE
EVN e-VLBI TOW May [email protected]
bs Again: “last mile problem”In 2017:still not solved ∀correlators
EVN e-VLBI TOW May [email protected]
bsCOR
EVN e-VLBI TOW May [email protected]
bs
Custom chip: correlateextremely synchronous ...• no buffering• no handling of network jitter
EVN e-VLBI TOW May [email protected]
bs
FPGA: delay, cornerturnextremely synchronous ...• lost sync if too few valid time stamps found
• e.g. due to packet loss ...• correlation breaks badly!
• also no buffering
EVN e-VLBI TOW May [email protected]
bs
CPU: delay, cornerturn, correlate extremely asynchronous!• no guaranteed throughput, may not keep up• need ~ few 100 compute nodes for 16 Gbps
• CPUs inefficient for 2-bit data
EVN e-VLBI TOW May [email protected]
bs
CPU: delay, cornerturn, correlate • per packet overhead is a concern• takes to handle bad/missing data
• node waiting for data that will never arrive• look valid but is invalid: hard to detect!
EVN e-VLBI TOW May [email protected]
bs
CPU: delay, cornerturn, correlate • JIVE’s SFXC software correlator works!• Cluster internal network (architecture and
throughput) is important• Investe in enough compute nodes
EVN e-VLBI TOW May [email protected]
Correlator Control GUI
EVN e-VLBI TOW May [email protected]
Who does what in e-VLBIField System Correlator control
time sync formatter (which channels)
frequency setup start/stop transfer
antenna (re)configure network
recorder (re)configure destination
...
Correlator must have direct access to sender!
EVN e-VLBI TOW May [email protected]
JIVEThe NetYour station
ccs.jive.eu
fs.yourstation.tld
TCP/IP controlFirewall issues
EVN e-VLBI TOW May [email protected]
Real-time VLBI!
• anything/anyone **** up?
• anything/anyone not keeping up?
you lose science data!
you lose science data!
EVN e-VLBI TOW May [email protected]
http://services.jive.nl/sfxc/fringe.html
Real-time fringeplot on the web
EVN e-VLBI TOW May [email protected]
EVN e-VLBI TOW May [email protected]
EVN e-VLBI TOW May [email protected]
EVN e-VLBI TOW May [email protected]
EVN e-VLBI TOW May [email protected]
EVN e-VLBI TOW May [email protected]
EVN e-VLBI TOW May [email protected]
EVN e-VLBI TOW May [email protected]
Daunting?Yes.
Real-time VLBI requires:a lot of knowledgeabout a lot of subjectsby a lot of peoplesupported by a lot of tools
EVN e-VLBI TOW May [email protected]
Real-time VLBI in EVN
Organized as monthly 24hr sessionsFuture e-VLBI Observing Sessions (real-time correlation)
-------------------------------------------------------2016 Dec 06 - Dec 07 (start at 13 UTC) 18/21 cm, 6 cm, 5 cm or 1.3 cm2017 Jan 17 - Jan 18 (start at 13 UTC) 18/21 cm, 6 cm, 5 cm or 1.3 cm2017 Feb 14 - Feb 15 (start at 13 UTC) 18/21 cm, 6 cm, 5 cm or 1.3 cm2017 Mar 23 - Mar 24 (start at 13 UTC) 18/21 cm, 6 cm, 5 cm or 1.3 cm2017 Apr 11 - Apr 12 (start at 13 UTC) 18/21 cm, 6 cm, 5 cm or 1.3 cm2017 May 09 - May 10 (start at 13 UTC) 18/21 cm, 6 cm, 5 cm or 1.3 cm2017 Jun 20 - Jun 21 (start at 13 UTC) 18/21 cm, 6 cm, 5 cm or 1.3 cm
http://www.evlbi.org/evlbi/e-vlbi_status.html
ToO ~ scheduled on few days notice
EVN e-VLBI TOW May [email protected]
EVN e-VLBI TOW May [email protected]
EVN e-VLBI TOW May [email protected]
4hr of test/setup
1. clocksearch2. possible station changes
new network h/wnetwork setup, IPv4uses diff. equip from scheduled
3. AOB
EVN e-VLBI TOW May [email protected]
EVN e-VLBI TOW May [email protected]
EVN e-VLBI TOW May [email protected]
Danke schön!