Subject: Time Tagging HRC Rates in NIL Mode
M. Juda
May 12 , 1999
1 Introduction
In a previous memo (HRC Time
Tagging - February 28, 1996), I described
how to time-tag HRC telemetry in both ``observing'' and
``next-in-line'' (NIL) mode. That memo contains errors in its
explanation of the time-tagging of the rate data when in both
modes. This memo is an update that provides a correction to the
time-tagging algorithm.
2 Observing Mode Rate Data
There are two samples of each of the rate data items (total, valid,
and shield events) in every science frame. The previous memo
incorrectly stated the the two samples corresponded to the two halves
of the science frame. The two samples actually correspond to two
consecutive, 1 second intervals, starting at the begining of the
previous science frame. The last 0.05 seconds of the science frame are
not included in the rate data.
If rij is the j-th rate sample (j = 0 or 1) from the i-th
science frame (i = 0-15) within a major frame, TMF is
the time of the start of the major frame, and tMF is the
duration of a major frame (32.8 seconds), then the time tag of the
sample is given by:
Trij = TMF + i |
tMF
16
|
+(j-2)×1.000 sec - 0.050 sec. |
|
3 NIL Mode Rate Data
There are two samples of each of the rate data items in every major
frame of HRC NIL mode data. Unlike the observing mode case, the
accumulation intervals for the two samples are not equal and do not
both occur in the previous major frame.
The start of the accumulation interval of the first sample of each
pair occurs 2.000 seconds after the start of science frame 14 (of
0-15) in the previous major frame. The end of the accumulation
interval is 1.000 seconds after the start science frame 15. Thus this
interval starts 2.100 seconds before the major frame the rate is
telemetered in and lasts for 1.050 seconds. The start of the
accumulation interval of the second sample of each pair is at the
start of the major frame and lasts for 1.000 seconds.
Given the description above, the time-tags that should be applied to
the two samples are:
and
where Tr1 and Tr2 are the time-tags for the first and
second samples respectively and TMF is the start time of the
major frame in which the samples are telemetered.
Dr. Michael Juda
Harvard-Smithsonian Center for Astrophysics
60 Garden Street, Mail Stop 70
Cambridge, MA 02138, USA
Ph.: (617) 495-7062
Fax: (617) 495-7356
E-mail: mjuda@cfa.harvard.edu
File translated from TEX by TTH, version 2.01.
On 12 May 1999, 14:38.