RTOF Instrument Modes and Measurement Sequences Table of content 1. Change Record 2 2. RTOF Instrument Modes and Measurement Sequences 3 2.1 RTOF Instrument Parameter Settings 3 3. Explanations to the RTOF Parameters 4 4. RTOF Sub Parameter Definitions 5 5. Examples of RTOF Modes 6 6. Possible Standard RTOF Modes 9 7. Power Consumption in the different modes 19 8. Mode Transitions 19 8.1 From Standby to SS OR / AND OS mode and vice versa 19 8.2 From Ion mode to Gas mode and vice versa 20 8.3 From Standby to Ion source heater mode and vice versa 20 8.4 Transition into emergency mode 20 8.5 All other mode changes 20 9. Examples of RTOF measurement sequences 21 10. Tabels necessary to run RTOF autonomously (stored in the DPU) 22 11. Appendix A: Time of Flight 24 12. Appendix B: ETS and ETS_L Operations 25 13. Appendix C: ETS Sampling Modes 27 14. Appendix D: ETS Parameter Settings 30 {{{1 Change Record}}} {| TABLE !Date !!Version No. !!Responsible !!Description of Change ! |- | ||3.0 ||K. Altwegg ||First distributed issue |- |15/12/2000 ||3.1 ||K. Altwegg ||Appendix C, Windowing mode WCS, Parameters WCS, power consumption, transitions |- |09/01/01 ||3.2 ||K. Altwegg ||Add Instrument modes (1,1L,1I, 1G) |- |13/03/2001 ||3.3 ||K. Altwegg ||Add low and high sensitivity modes, 1,5,10 kHz modes |- |03/07/2001 ||4 ||K. Altwegg ||Add ETS parameter settings |- |24/01/2002 ||5 ||K. Altwegg ||Replace WCS by ETS-L |} {{{2 RTOF Instrument Modes and Measurement Sequences}}} {{2.1 RTOF Instrument Parameter Settings}} {| TABLE !Channel !!STOrage !! ! |- | ||ORThogonal || |- | ||BOTh || |- | ||OFF{cov} || |- |Function ||GAS || |- | ||ION || |- | ||GAs and Ion || |- |Task ||COMetary || |- | ||BACkground || |- | ||SHUt off{pos1,pos2} || |- | ||OPTimization{AMU} || |- | ||CALibration || |- |Ambient ||AMBient{U1,U2} || |- |Emission ||NONe || |- | ||SUBemission{fil} || |- | ||EMIssion{fil,I} || |- | ||HEAt{fil,sec} || |- |Electron Energy ||HIGh || |- | ||LOW || |- | ||VAR{U1,U2} || |- |Reflections ||SINgle || |- | ||TRIple || |- | ||BLAnk{t1,t2} || |- |Data acquisition ||ETS{d,freq,NOE,CAL, thr,MLM, SM, thr_L,MLM_L,SM_L} ||_L refers to ETS Light |- |Data Compression ||DAC{num} || |} {{{3 Explanations to the RTOF Parameters}}} Channel: This parameter determines which channel to be used. Normally the orthosource is used for ions, the storage source for gas. However, if for example the filaments in the storage source fail the orthosource can also be used to measure neutrals. The channel OFF means that both channels are inactive, the {cov} determines if the cover shall be closed (=1) or stay open (=0). Associated table: cover position; Voltages for ion sources Function: This parameter determines if the instrument measures gas, ions, ions and gas simultaneously Associated tables: Voltages for ion sources Task: COMetary means that the instrument measures the cometary (asteroidal) gas and/or ions. BACkground is measured by deflecting the ions away from the detector (adjust for example reflectron backplane?). This then gives the detector/data acquisition background. SHUt off closes partly the cover to shut off cometary particles. Mass spectra are measured in a fixed position of the cover if pos1=pos2, or in a series of positions between pos1 and pos2. E.g. cover position is 90 degrees, 80, 70, 60, etc up to 20 degrees. In this way the background from reflections on the spacecraft and/or RTOF can best be distinguished from cometary neutrals, OPTimization means that the voltages in RTOF are being optimized (S/W to be developed at a later stage, possibly not before the end of 2002). The parameter GCU determines if the GCU is used for this purpose (AMU=0) or if a cometary mass is being used (AMU=mass number) CALibration will be used to recalibrate RTOF (without optimization) with the GCU. Associated tables: Voltages for reflectron; cover position;optimization;calibration Ambient: This parameter is only active for the function ION. It determines the absolute potential of the external attraction grid. U1 and U2 determine the potential of the grid. If U1=U2 the voltage is fixed. If U1 is not U2 then the voltage is scanned at a fixed number of steps (limits included). Internal voltages are adjusted automatically to the different potentials according to a table. Associated tables: ion source voltages dependency on attraction potential Emission: This parameter sets the emission current and the active filament. Filament no. 1 and 2 are in the storage source, filament no. 3 and 4 in the orthosource. The number of filament settings should be kept as low as possible. RTOF like DFMS 2, 20, 200 A. In the setting SUB the filament is kept just below the emission threshold. In the setting HEA, the ion source heater of the ion source with the filament f would be used for sec seconds. Parallel to this the filament f would be kept in subemission mode. Associated tables: FEC settings Electron Energy: The electron energy in the source can be adjusted continuously. However, to simplify calibration it is advisable to use only two values regularly: HIGh (ca. 70 eV), LOW (ca. 17 eV). In the VARiable setting the electron energy will be stepped (0.2 eV steps, tbc) from U1 to U2. It must be guaranteed that no dangerous combinations of emission and electron energies are executed (tbd). FEC settings Reflections: SINgle reflection is the mode with lower resolution but higher sensitivity. TRIple reflection uses the hardmirror and twice the reflectron to enhance the time of flight and with it the mass resolution. BLAnk mode uses a triple reflection with a blanking pulse in the hardmirror, t1 indicates the delay of the blank pulse with respect to the extraction pulse, t2 gives the duration of the pulse. Associated table : Voltages for ion sources, hard mirror and reflectron Data acquisition: ETS is connected to the storage source, ETS_Light to the ortho source. If both are active they have to work together, that is, ETS is triggered by ETS_L. The blank pulser can only be triggered by the ETS. A detailed description of the ETS modes is in appendix B to D. Associated table : calibration table for ETS; Data Compression: This gives the method for the DAta Compression. 0=no compression, which may lead to too much data being produced. The DPU would then stop the data taking. >0=data compression by integration. Num is the minimum number of spectra being integrated. The DPU would increase this value if the data flow is not compatible with the allowed data rate, it would lower it again if permissible, but never below num. <0= wavelet compression. {{{4 RTOF Sub Parameter Definitions}}} Channel: OFF{cov} cov=0 cover open cov=1 cover closed Task: SHUt off{pos1,pos2} pos1: start position of cover pos2: end position of cover steps of 10 degrees (TBC) OPTimization(AMU) AMU: mass number to be used for optimization; if AMU=0, GCU is used Ambient: AMBient{U1,U2} U1:start voltage of attraction grid potential U2:stop voltage of attraction grid potential Steps 2V, TBC Emission SUBemission{fil} fil: filament no., 1 and 2 in storage , 3 and 4 ortho EMIssion{fil,I} fil: as above I: Emission current in microamps HEAt{fil,sec} fil as above sec: time in seconds for heating Electron energy: VAR{U1,U2} U1: start energy U2: stop energy steps 0.2V, TBC Reflections BLAnk{t1,t2} t1: delay of blank pulse in microsecs t2:duration of pulse in microsecs Data acquisition: ETS{d,freq,thr,MLM, SM, NOE,CAL,thr_L,MLM_L,SM_L }. The appendix _L refers to ETS_L d: Ex. Del.: Extraction Delay, this values delays the start of the data acquisition Freq: Rep. Rate: Extraction frequency , 2,5,or 10kHz NOE: Number of Extractions, a fixed number between 1... 65535 if "on" is selected , if NOE<0 it gives the integration time in seconds. The parameter has to be set to "off" in the ETS and the integration is started and stopped by the DPU. Cal. Func.: Functions of the internal electrical calibrator 0=off, >0 =on (a few combinations of pulse width, pulse heigth TBD) Thr (THR_L).: Threshold level of the analog signal discriminator MLM (MLM_L): Mass Lines Mode: 31, 63, 255 (related to Freq) SM (SM_L): Sampl. Mode: Sampling Mode, STD, TDC_STD, DTS, TDC_DTS or HIRM, for SM_L only TDC modes Data compression: DAC{num} num=0: no compression num>0: compression by integration over num spectra num<0: wavelet compression {{{5 Examples of RTOF Modes}}} To facilitate the definition of measurement sequences it is necessary to use short hand designation for specific modes. The simplest solution is to just consecutively number the modes. This requires that an updated table of modes is available to designate sequences. The numbering should however follow a few simple rules: Thus the following last digits should be used for the following combination of channel, function: 0: Other combinations of source,task,freq 1: STO,GAS,ETS,10kHz 2: STO,ION,ETS, 10 kHz 3: ORT,GAS,ETS_L, 10 kHz 4: ORT,ION,ETS_L, 10 kHz 5: BOT,GAI, both ETS, 10 kHz 6: STO,GAS,ETS,5 kHz 7: ORT,ION,ETS_L, 5 kHz 8: STO,GAS,ETS,2 kHz 9: ORT,ION,ETS_L, 2 kHz The numbering should be arranged as follows: 0 to 49 Basic modes for switch on/off 50 to 99 Bake out and other technical modes 100 to 499 Basic optimization and calibration modes 500 to 999 Standard survey modes 1000 to 1999 Modes specialized for scientific questions 2000 to 9999 Custom modes A wide mass range, storage source only mode would be defined by the following parameter set: A normal gas and ion mode for RTOF could be commanded by: M205: mode(BOT,GAI,COM,AMB{5,5},EMI{1,med},HIG,TRI,ETS{10,10,0, 31,STD,0,-100,1,31,STD}, DAC{-1}) In this mode the instrument would measure cometary gas and ions, using both channels and both data acquisition systems. The filament 1 has a medium emission (20 microA) and an electron energy of 70 eV. The hard mirror is active, triple reflection. Delay time for both ETS and ETS_L is 10 s, the measurement mode for both ETS is standard, which is with ADC for the ETS. The threshold level is 0 for ETS and 1 for ETS_L. Data compression is by wavelet compression. Integration time is 100 s/spectra. The extraction frequency is 10 kHz. A lower power mode is given by: M201: mode(STO,GAS,COM,AMB{0,0},EMI{1,med},HIG,SIN,ETS{10,10, 0,31,TDC,0,-100,0,0,0}, DAC{-1}) The background is then measured by the two following sequences: M101: mode(STO,GAS,BAC,AMB{0,0},EMI{1,med},HIG,SIN,ETS{10,10, 0,31,TDC,0,-100,0,0,0}, DAC{10}) M111: mode(STO,GAS,SHU{10,80},AMB{0,0},EMI{1,med},HIG,SIN,ETS{10,10, 0,31,TDC,0,-100,0,0,0}, DAC{10}) ETS is put in the TDC mode (ADC inactive). M101 measures the electronic background (the pulser voltage is misadjusted)). The integration is 10 spectra, that is 2000 sec. M111 then measures the gas density while the cover is being closed in steps of 10 degrees (TBC) from 10 degrees to 80 degrees. This gives a measure for the background molecules coming from inside the ion source or being reflected from the spacecraft or from RTOF itself. Maximum number of mass lines per extraction is 31 (should be sufficient if we need the low power mode); the extraction frequency is 10 kHz. {{{6 Possible Standard RTOF Modes}}} The RTOF Instrument Modes are detailed in a separated document named RTOF_MODE_DESC.ASC {{{7 Power Consumption in the different modes}}} The power consumption of RTOF is composed of six main components, namely of the standby power (low voltage converters and main controller), of the analyzer part, of the filament, of the data acquisition system(s) used, of the ion source heater and of the cover motor. It does vary neither with triple or single reflection nor with using one or two channels. The following table shows the four contributions: {| TABLE ! !!Power (W) ! |- |Standby mode (LVPS, MC) ||11.2 |- |Analyzer Part ||1.5 |- |Filament ||2.8 |- |ETS low power or ETS_L / ETS normal/ Both ||4 / 7 / 11 |- |Ion source heater* ||12 |- |Cover motor ||2 |} *Not run in parallel to analyzer part, filament or cover motor The power used by RTOF in each mode can therefore be calculated. A normal measurement mode (one channel only) in power savings mode needs 19.5 W; with ETS in normal operation 22.5 W, with ETS and ETS_L 26.5 W, the ion source heater needs 23.2 W. {{{8 Mode Transitions}}} All mode transitions are controlled by the DPU. {{8.1 From Standby to SS OR / AND OS mode and vice versa}} To go from standby mode to either the SS (Storage Source) or OS (Ortho Source) mode needs the activation of the high voltage power supply. This is done in a predefined sequence by the DPU (set voltages to zero, activate high voltage enable, set voltages in a predefined sequence to their respective values). The SS and the OS mode can be run in parallel. To go back to standby mode is done in the same way (set voltages to zero, disable high voltages). {{8.2 From Ion mode to Gas mode and vice versa}} For all the gas modes (including Gas calibration, optimization and background measurement with the cover) the filament is needed. For this mode normally the Storage Source is used. The ion modes can either be done with the filament in subemission mode or with the filament off. For this mode the Ortho source is optimised. If both channels are active, normal operation in the OS is without filament, in the SS with filament in emission mode. However, if for scientific reasons or because one of the channels is degraded, gas and ions are measured with the same channel the following restrictions apply: To switch between gas and ion mode and vice versa is done by adjusting the filament current from emission to subemission and vice versa in order not to stress the filament. This is also controlled by the DPU. {{8.3 From Standby to Ion source heater mode and vice versa}} The ion source heater mode is activated by the DPU from the standby mode only. No transitions are foreseen from any active mode into this mode. {{8.4 Transition into emergency mode}} From all modes, a transition into the emergency mode is possible. From the emergency mode the only transition allowed is into standby mode (TBC). {{8.5 All other mode changes}} All mode transitions not shown in the diagram (e.g. triple reflection to single reflection, electronic noise to cometary gas measurement, optimization to calibration, etc.) can be done without involving any intermediate modes. There are no mode transitions, which are forbidden, except the ones shown above. {{{9 Examples of RTOF measurement sequences}}} Standard Survey sequence, low power mode: Step no. Mode Description Time 10 M50 10 minutes bake of storage source 600 s 20 M1 Storage source switch on, 50 s A waiting time to stabilize ion source may be required 30 M161 Storage source, Gas, Electr. Background,ETS low power 100 s 40 M221 Storage source, Gas, Background, ETS , low power 1000 s 50 n*M261 Storage source, Gas, Survey, ETS,low power n*100 s 60 M161 Storage source, Gas, Electr. Background,ETS, low power 100 s 70 go to 50 Standard Survey Sequence, full power mode Step no. Mode Description Time 10 M50 10 minutes bake of storage source 600 s 20 M5 Storage source and ortho source switch on 50 s A waiting time to stabilize ion source may be required 30 M155 Both sources,Gas and ions, Electr. Background,ETS and ETS_L 50 s 40 M245 Both sources, Gas and ions, S/C charging, ETS and ETS_L 1000 s 50 M2156 Both sources, Gas and ions, Background,ETS and ETS_L 1000 s 60 n*M205 Both sources, Gas and Ions, Survey, ETS and ETS_L n*100 s 70 M155 Both sources, Gas and ions, Electr. Background,ETS and ETS_L 50 s 80 go to 60 {{{10 Tabels necessary to run RTOF autonomously (stored in the DPU)}}} Table 1: Standard voltage values for mass spectrum at 20 DegC {| TABLE !Storage source parameters !!Ortho source parameters !!Reflectron, single reflection !!Reflectron, triple reflection !!Hard Mirror ! |- |Lens 1: L10 ||Lens 1 ||Lens ||Lens ||Lens |- |Lens 2 ||Lens 2 ||U1 ||U1 ||U1 |- |Backplane ||Backplane ||U2 ||U2 ||Backplane |- |etc. ||etc. ||Backplane ||Backplane ||etc. |- | || ||etc ||etc || |} Table 2: Functions of temperatures for all voltages : {| TABLE !Storage source parameters !!Ortho source parameters !!Reflectron, single reflection !!Reflectron, triple reflection !!Hard Mirror ! |- |Lens 1:L1(T)=L10*f(T) || || || || |- |etc. || || || || |} Table 3: Relationship between mass no. and delay time for single and triple reflections: m=f(t) Table 4: Relationship between attraction grid potential and source voltages for ortho source and storage source See Appendix C Table 6.: Cover position table Table 7a....: Tables for Optimisation Table 8: Settings for FEC: High, med, low emission, subemission Table 9: Calibration mode tables for ETS_L and ETS (internal pulser) {{{11 Appendix A: Time of Flight}}} Below some typical TOF's s) for inexperienced people like myself: Mass TOF single delta to next mass TOF triple delta to next mass 1 3.3 1.3 6 2.5 4 6.5 0.9 12 1.3 28 17 0.3 31 0.56 40 21 0.26 37 0.47 130 37 0.14 68 0.26 300 56 0.09 103 0.17 {{{12 Appendix B: ETS and ETS_L Operations}}} The ETS has the following parameters ETS{d,thr,fifo,freq,int,ADC,dts,cal} Thereby the parameters have the following meaning: d delay (units TBD) thr threshold (0...7) fifo number of mass lines allowed (16 ADC samples per mass line) freq Extraction pulser frequency Int Integration time ADC =1: ADC is on; =0 ADC is off (2.5W power savings); not for ETS_L Dts: delayed time sampling, 0=off, 1=on; <0 =high resolution mode cal Calibration (0=off, 1...n different combinations of settings of pulse height,etc., TBD) The time to take one ETS spectrum is divided into the following sections: d is the delay time before ETS starts looking for peaks. Electronic noise can also trigger the ETS signal acquisition, which looks the same to the ETS electronics. At the moment the extraction pulser disturbance extends to approx. 10 us after pulser firing, which then gives the minimal useful time for d. However, protons will arrive at approx. 3 us in single reflection mode and arrive at approx. 6 us in triple reflection mode. s is the time while ETS looks for mass peaks. d+s therefore gives the flight time of the heaviest mass in the mass range. Acc is the time needed to calculate the spectrum. This is given by number of detected mass lines x 1.3 s. T is the time period for 1 spectrum and is 1/f with f being the frequency of the extraction pulser. While d and s are fixed, acc depends on the number of detected mass lines. The ETS is able to record up to 256 signals (e.g. mass lines) per spectrum. In order to keep f constant which is essential to be able to analyze the data at least for the storage source it was decided to add one more parameter for ETS which is fifo. This is the maximum number of mass lines allowed for a given frequency. This then fixes the time acc. Fifo can have the following values: 31 which corresponds to acc = 40.3 s 63 which corresponds to acc = 80.6 s 255 which corresponds to acc = 322.4 s The max. value of s is 217 s; this time is given by the size of the data memory in ETS. This corresponds to 128 kWords (48 bits/word; 30 for the ADC, 18 for the counter) of data. From this the following table can be deduced: {| TABLE !1/Freq s) !!dmin s) !!s s) !!Fifomax !!acc s) ! |- |100 ||10 ||50 ||31 ||40 |- |200 ||10 ||110 ||63 ||80 |- |500 ||10 ||170 ||255 ||320 |- |1000 ||10 ||217 ||255 ||320 |- |200 ||10 ||70 (high resolution) ||63 ||80 |} I suggest the following combinations of fifo and freq to be used: {| TABLE !Purpose !!d s) !!freq (kHz) !!fifo !!Max. mass (amu) ! |- |Normal survey, triple reflection ||10 ||2 ||255 ||>300 |- |Low intensity mode, single refl. ||10 ||5 ||63 ||>300 |- |Light masses only, high sensitivity ||10 ||10 ||31 ||>300 (single refl.) 100 (triple refl.) |- |Very large mass range ||Variable (<217 s), i.e. first spectrum 10, second spectrum 100 ||2 ||255 ||>1000 |- |High resolution, triple reflection ||Variable, i.e. first spectrum 10, second spectrum 60 ||5 ||63 ||>300 |} {{{13 Appendix C: ETS Sampling Modes}}} {| TABLE !Mode !!Commands * !!Extraction Period !!Prog. Parameters !!Resolution !!DPU Readout !!Event dead time [ns] ! |} {| TABLE !No !!Name !!DTS !!HIRM !! !!Delay [ s] ! !TOF [ s] !!Spectrum [ s] !!# of mass lines !!TDC !!ADC !! !! ! |- |0 ||STANDARD ||off ||off ||TOF + ACC ||0...217.0615 ||0...217.0615 |* |' 255 ' 63 ' 31 ||1.65 ||1.65 ||Delay: HK as info ||133 |- |1 ||DTS ||on ||off ||TOF + ACC ||0...217.0615 ||0...217.0615 |* |' 255 ' 63 ' 31 ||1.65 ||1.65 ||Delay: HK as info ||0 |- |2 ||HIRM ||off ||on ||DEL + S + ACC ||0...217.0615 |* |0...54.272 ||' 255 ' 63 ' 31 ||0.55 ||0.55 ||Delay: required ||133 |- |3 ||HI_DTS ||on ||on ||TOF + ACC ||0...217.0615 ||0...217.0615 |* |' 255 ' 63 ' 31 ||0.55 ||0.55 ||Delay: HK as info ||0 |} {{{14 Appendix D: ETS Parameter Settings}}} NEW Parameter Definitions: ETS{d,freq,thr,MLM, SM, NOE,CAL } The modified parameters are listed in red! lowest frequency 1.84kHz. File ETS_PAR_M#.txt Explanation of Parameters: d: Ex. Del.: Extraction Delay, this values delays the start of the data acquisition Freq: Rep. Rate: Extraction frequency Thr.: Threshold level of the analog signal discriminator MLM: Mass Lines Mode: 31, 63, 255 or adaptive 1 to 512 SM: Sampl. Mode: Sampling Mode, STD, TDC_STD, DTS, TDC_DTS or HIRM NOE: Number of Extractions, a fix number between 1... 65535 if "on" is selected Cal. Func.: Functions of the internal electrical calibrator 0=off, >0 =on (a few combinations of pulse width, pulse heigth TBD) Other parameters for the ETS which will be deduced from the instrument mode parameters Sync.: Synchronization: internal(=0) or external (=1) trigger See also ETS Documentation for detailed information! Other parameters for the ETS, to be set by the DPU independent of instrument mode? RAM: Memory function: NONE, CLR or TEST before data acquisition Mem. Range: Memory readout address range TOF: Time Of Flight of extracted ions, after this time accumulation is initiated (derived from freq, d and MLM) Table : List of ETS Parameter settings for RTOF Operation {| TABLE !Mode !!File # !!Parameter ETS{ d,freq,thr,MLM, SM, NOE,CAL } !!Rep. Rate [kHz] !!MLM !!TOF [us] !!Ex. Del [us] !!Sampl. Mode !!Trig. to Source N/A !!Sig. Input N/A !!Thr. [mV] !!Sync. !!Cal. Func. !!Cal. Width [ns] !!Cal Height [mV] !!NOE !!RAM !!Mem. Range [us] ! |} O P T I M I Z A T I ON A N D C A L I B R A T I O N M O D E S {| TABLE !101 111 121 131 141 151 161 171 181 191 201 211 !! 1 !!10,10,0,31,STD,off,0 !! 10 !! 31 !! 60.0225 !! 9.9915 !! STD !! !! !! 18 !! Int !! off !! 0 !! 0 !! off !! CLR !!0 ... 64.9968 ! |} S T A N D A R D M O D E S {| TABLE !506 516 526 !! 0 !!10,5,0,63,STD,off,0 !! !! 63 !! 118.694 !! 9.9915 !! STD !! GAS !! GAS !! 18 !! Int !! off !! 0 !! 0 !! off !! CLR !!0 ... 120.001 ! |- |501 511 521 531 541 551 || 2 ||10,10,0,31,STD,off,0 || 10 || 31 || 118.694 || 9.9915 || STD || ION || ION || 18 || Int || off || 0 || 0 || off || CLR ||0 ... 120.001 |- |504 505 514 524 534 535 544 554 815 || 2 ||10,10,0,31,STD,off,0 || 10 || 31 || 118.694 || 9.9915 || STD || ION || ION || 18 || Int || off || 0 || 0 || off || CLR ||0 ... 120.001 |- |509 519 529 819 || 3 ||10,2,0, 255,STD,off,0 || 2 || 255 || 172.754 || 9.9915 || STD || GAS || GAS || 18 || Int || off || 0 || 0 || off || CLR ||0 ... 174.999 |- |591 601 611 ||4 ||10,5,0, 63,DTS,off,0 || 5 || 63 || 118.694 || 9.9915 || ADC DTS || GAS || GAS || 18 || Int || off || 0 || 0 || off || CLR ||0 ... 120.001 |- |861 ||5 ||10,5,0, 63,TDC_STD,off,0 || 5 || 63 || 118.694 || 9.9915 ||TDC_ STD || GAS || GAS || 18 || Int || off || 0 || 0 || off || CLR ||0 ... 120.001 |- |864 865 ||6 ||10,5,0, 63,TDC_STD,off,0 || 5 || 63 || 118.694 || 9.9915 ||TDC_ STD || ION || ION || 18 || Int || off || 0 || 0 || off || CLR ||0 ... 120.001 |- |871 ||7 ||10,2,0, 255,TDC_STD,off,0 || 2 || 255 || 172.754 || 9.9915 || STD || GAS || GAS || 18 || Int || off || 0 || 0 || off || CLR ||0 ... 174.999 |- |874 ||8 ||10,2,0, 255,TDC_STD,off,0 || 2 || 255 || 172.754 || 9.9915 || STD || ION || ION || 18 || Int || off || 0 || 0 || || || |- |196 506 516 526 536 546 556 596 606 616 ||9 ||10,5,0, 63,STD,off,0 ||5 || || || ||STD ||ION ||ION || ||Ext || || || || || || |- |802 ||10 ||100,5,0, 63,STD,off,0 ||5 ||63 || || ||STD ||GAS ||GAS || ||Ext || || || || || || |- |801 ||11 ||10 ,5,0, 63,HIRM,off,0 ||5 ||63 || || ||HIRM ||GAS ||GAS || ||Ext || || || || || || |- |804 ||12 ||10,5,0, 63,HIRM,off,0 ||5 ||63 || || ||HIRM ||ION ||ION || ||Ext || || || || || || |- |211 ||13 ||10,10,0, 31,STD,1,N ||10 || || || ||STD ||GAS ||GAS || ||Int ||On ||TBD ||TBD ||1 || || |- |214 ||14 ||10,10,0, 31,STD,1,N ||10 || || || ||STD ||ION ||ION || ||Int ||On ||TBD ||TBD || 1 || CLR ||0 ... 174.999 |}