  COVER INFORMATION 

 Station:    HART_S2   (Code Hh ) 
 Experiment: VSOP observation of  J2218-03  at 5  GHz
 Exp. Code:  w009d3  


Schedule Version:       1.00                                              
Processed by SCHED version: Release of 28 April 2000                      

PI:       Roger P. Linfield                                               

Address:  Mail Stop 238-600                                               
          Jet Propulsion Laboratory                                       
          Pasadena, CA   91109  USA                                       
                                                                          

Phone:    1-818-354-2806                                                  
EMAIL:    rpl@ipac.caltech.edu                                            
Fax:      1-818-393-4965                                                  
Phone during observation:                                                 

Observing mode: VSOP, 5  GHz continuum, 128-2-2                           

Notes:    Fringe finder : J2148+06                                        
                                                                          
                                                                          
                                                                          

Schedule for HART_S2   (Code Hh )                                   Page   2
               VSOP observation of  J2218-03  at 5  GHz
  UP:  D => Below limits;  H => Below horizon mask.  blank => Up.
  Early: Seconds between end of slew and start.   Dwell: On source seconds. 
  Tapes: Drive, Index, Start footage / Direction, Head Group, End footage.
  TPStart:  Tape motion start time.
----------------------------------------------------------------------------------------
Start UT  Source               Start / Stop                 Early    Tapes      TPStart
Stop UT                  LST      EL    AZ   HA  UP   ParA  Dwell  (see above)
----------------------------------------------------------------------------------------

 --- Sun  26 Nov 2000   Day 331 ---

 Next scan frequencies:  4800.00  4816.00
 Next BBC frequencies:    160.00   176.00
 Next scan bandwidths:     16.00    16.00

10 30 00  J2218-03     16 43 24   7.1  90.6 -5.6    -115.7     0   1  1     52  10 30 00
10 59 00  ---          17 12 28  13.6  87.4 -5.1    -115.8  1740   F  1    661

11 00 50  J2148+06     17 14 19  16.0  73.8 -4.6    -119.5   107   1  1    700  11 00 50
11 06 00  ---          17 19 29  17.1  73.1 -4.5    -119.8   310   F  1    808

11 07 50  J2218-03     17 21 20  15.6  86.4 -5.0    -115.9   107   1  1    847  11 07 50
12 00 00  ---          18 13 38  27.3  80.1 -4.1    -117.4  3130   F  1   1942

12 00 00  J2218-03     18 13 38  27.3  80.1 -4.1    -117.4    -2   1  1   1942  12 00 00
13 00 00  ---          19 13 48  40.4  71.2 -3.1    -121.4  3598   F  1   3202

13 00 00  J2218-03     19 13 48  40.4  71.2 -3.1    -121.4    -2   1  1   3202  13 00 00
13 30 00  ---          19 43 53  46.7  65.6 -2.6    -124.8  1798   F  1   3832

13 30 00  J2218-03     19 43 53  46.7  65.6 -2.6    -124.8    -2   1  1   3832  13 30 00
14 00 00  ---          20 13 58  52.7  58.6 -2.1    -129.7  1798   F  1   4462


SETUP FILE INFORMATION:
   NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings.


 Setup file: /home/sched/short-term/progs/current/setups/vsop4800_s2.set
   Matches group hh6cm_a in /home/sched/short-term/progs/current/catalogs/freq.dat

   Setup group:    6         Station: HART_S2           Total bit rate:  128
   Format: S2                Bits per sample: 2         Sample rate: 32.000
   Number of channels:  2    Passes/head pos:   1       Speedup factor:   1.00

   Tape speeds: Low density -   6.300 ips,  High density -   4.20 ips
   Time per pass for   7600 ft, High density tapes is: 06:01:54

   1st LO=  4640.00  4640.00
   Net SB=        U        U
   Pol.  =     LCP      LCP 
   BBC   =        1        3
   BBC SB=        U        U
   IF    =       1N       1N

  The following frequency sets based on this setup were used.

   Frequency Set:   6  Setup file default.  No pcal detection.
   LO sum=   4800.00  4816.00
   BBC fr=    160.00   176.00
   Bandwd=    16.000   16.000

   Track assignments are: 
    track1=   0,  0
    barrel=roll_off 
 SOURCE LIST -- VSOP observation of  J2218-03  at 5  GHz
     Catalog positions marked with *. 
     Position of date is for stop time of first scan.
     Names used in schedule marked with *. 
     Short names used in VLA and SNAP files marked with +. 

   Source                         Source position (RA/Dec) 
                        (B1950)           (J2000)           (Date) 

   J2148+0657        21 45 36.078484   * 21 48 05.458682     21 48 06.887528 
   2145+067          06 43 40.90444    * 06 57 38.60404      06 57 55.47208 
 * J2148+06          /home/sched/short-term/progs/current/catalogs/sources.vlba
                     USNO - Ref Frame 1998-6, Eubanks June 1998

   J2218-0335        22 16 16.381739   * 22 18 52.037727     22 18 53.685729 
   2216-038         -03 50 40.62454    *-03 35 36.87963     -03 35 23.36483 
 * J2218-03          /home/sched/short-term/progs/current/catalogs/sources.vlba
                     USNO - Ref Frame 1998-6, Eubanks June 1998



  The solar corona can cause unstable phases for sources too close to the Sun.
  SCHED provides warnings at individual scans for distances less than 10 degrees.
  The distance from the Sun to each source in this schedule is:
    Source         Sun distance (deg) 
   J2148+06            87.4
   J2218-03            90.8

  Barry Clark estimates from predictions by Ketan Desai of IPM scattering sizes 
  that the Sun will cause amplitude reductions on the  longest VLBA baselines 
  at a solar distance of 60deg F^(-0.6) where F is in GHz. 
  For common VLBI bands, this is: 
       327 MHz        117. deg 
       610 MHz         81. deg 
       1.6 GHz         45. deg 
       2.3 GHz         36. deg 
       5.0 GHz         23. deg 
       8.4 GHz         17. deg 
      15.0 GHz         12. deg 
      22.0 GHz          9. deg 
      43.0 GHz          6. deg 

