<=== observer ===>
"CLEINERT",\
"Leinert, Ch.",\
"",\
"Max-Planck-Institut f\"ur Astronomie",\
"K\"onigstuhl 17",\
"",\
"D-69117",\
"Heidelberg",\
"Germany",\
"49 6221 528264",\
"49 6221 528246",\
"leinert@mpia-hd.mpg.de"
<=== proposal ===>
"PROPERT4",1,1,\
{"interplanetary medium","dust properties","comet trails"},\
{"Gr\"un,E.", "Salama,A.", "Sykes, M.", "Staude,J.", "Lemke,D.",\
"Abraham,P.", "Abolins,J."}
<=== title ===>
Properties of solar system dust, Section 4
<=== abstract ===>
SCIENTIFIC ABSTRACT
This proposal makes use of the opportunity given by ISO to study the
properties fo the different dust populations in interplanetary space
with the same instrument and identical observational procedures. For
technical reasons, the properties of dust in comets and of asteroid
surfacess are studied in separate central programme proposals, while
this central programme proposal deals with
- dust in the general interplanetary medium,
- dust in the asteroidal bands,
- dust in cometary trails.
This procedure allows a thorough comparison of interplanetary dust with
the properties of dust released from its probable sources, comets and
asteroids, and thus contributes to the knowledge of the origin of
interplanetary dust.
OBSERVATION SUMMARY
The properties of dust in the interplanetary medium, in asteroidal bands
and in comet trails will be studied with ISOPHOT by the same type of
measurements: photometry with ISOPHOT-P and ISOPHOT-C, either with full or
with reduced spectral coverage, and spectrophotometry with ISOPHOT-S.
In addition, scans perpendicular to the chosen asteroidal bands and comet
trail will be performed to detect structure and to determine the
position of maximum brightness for subsequent full photometry and
spectrophotometry. For all measurements the largest aperture (180 arcsec)
will be used.
We aim at relative photometric accuracies of at least a few percent or
better, which is needed to separate bands or trails from the much brighter
background of zodiacal light. In spectrophotometry this accuracy will not
be achieved for a single pixel. Here we take the longest available integration
time and will improve the signal-to-noise ratio by binning.
The proposal consists of three parts:
1. Dust in the general interplanetary medium
2. Asteroidal bands
3. Cometary trails
Object lists and breakdown of observations by AOT's will be given in the
three separate parts of this proposal. The common observing plan for photometry,
spectrophotometry or scans will be given here. The choice of filters
reflects the coordination with the proposals on "comets", "zodiacal
light" and "extragalactic background light".
Distribution of the observing times:
Observations priority 1 priority 2 priority 3 sum
------------------------------------------------------------------
general medium 6478 s 15254 s 6478 s 28210 s
asteroidal band 0 s 54369 s 0 s 54369 s
cometary trail 24988 s 0 s 1859 s 26847 s
------------------------------------------------------------------
total 31466 s 69623 s 8337 s 109426 s
(8.7 h) (19.3 h) (2.3 h) (30.4 h)
29 % 64 % 8 %
=== Detailed observing plan ===
1. Full photometry
Filter t(on object) t(performance)
----------------------------------------------
P_3.6 256 s 562 s
P_4.85 64 s 180 s
P_7.3 32 s 114 s
P_10 32 s 110 s
P_12.8 32 s 106 s
P_11.5 32 s 98 s
P_16 32 s 104 s
P_25 32 s 198 s
P_60 32 s 200 s
P_100 32 s 202 s
C_135 32 s 86 s
C_160 32 s 76 s
C_200 32 s 82 s
Acquisition 180 s
-------------------------------------------------
Performance time 2298 s (0.64 h)
2. Reduced photometry
Filter t(on object) t(performance)
----------------------------------------------
P_7.3 32 s 114 s
P_10 32 s 110 s
P_12.8 32 s 106 s
P_11.5 32 s 98 s
P_16 32 s 104 s
P_25 32 s 198 s
P_60 32 s 200 s
P_100 32 s 202 s
C_160 32 s 76 s
C_200 32 s 82 s
Acquisition 180 s
-------------------------------------------------
Performance time 1470 s (0.41 h)
3. Short photometry for scans
Filter t(on object) t(performance)
--------------------------------------------------------------------
P_12.8 4 s per raster point depends on scan type and length
P_25 4 s per raster point depends on scan type and length
P_60 4 s per raster point depends on scan type and length
Acquisition 180 s per scan leg depends on number of legs
20 s per leg repetition depends on number of legs
---------------------------------------------------------------
Performance time depends on scan length
4. Spectrophotometry
Detector t(on object) t(performance)
----------------------------------------------------
SL 4096 s 4180 s
SS 4096 s 0 s (parallel operation)
Acquisition 0 s (already done)
----------------------------------------------------
Performance time 4180 s (1.2 h)
=== Special requirements ===
1. It is the nature of the objects studied here that they are moving with the
annual motion of the sun. This leads to the following consequences:
a. FIXED TIME OBSERVATIONS are needed in several cases, because
visibility and aspect conditions are only fulfilled around
certain dates (defined by a value of lambda(sun), but also
depending on launch date). These observations will be clearly
indicated in the object lists of the three parts of this proposal.
b. COORDINATES in alpha, delta can be provided for
these moving objects, but only after more is known about
lauch date and visibilities. Therefore they will not be given now
but after the required information is available.
c. Observations have to be performed at low background positions
and at correct angles with respect to the sun. Even for
non-fixed-time-observations strong constraints result,
and we give PREFERRED TIME WINDOWS for the observations.
d. For the observations of the comet trail we need the
predicted position of the comet and the orientation of its trail
for the date or dates of observation.
2. In contrast to most other observing programmes, the measurements of this
proposal require absolute measurements. This needs both calibration and
a knowledge of the dark current of the detectors for the integration
times used. We assume, that - as part of the general calibration effort -
DARK CURRENT MEASUREMENTS of sufficient quality will be
available for the proposed measurements.
<=== scientific_justification ===>
Team top 40% middle 30% remaining 30% total performance time
---------------------------------------------------------------------
PHOT 25160 s 51435 s 3612 s 80213 s
SOT 6300 s 4725 s 4725 s 15750 s
---------------------------------------------------------------------
Sum 31460 s 56160 s 8337 s 95963 s
(8.7 h) (15.6 h) (2.3 h) (26.66 h)
33 % 59 % 9 %
=== Part 3: Cometary trails ===
The comet best suited for these observations is comet Kopff, which
was selected for its brightness and favourable position in the sky.
These are linked fixed time observations.
They consist of scans across the cometary trail and of pointed
observations. The scans serves to determine the position of
maximum brightness. This position (default value is the
predicted position for the date of observation) is used in the following
pointed observations for full photometry and spectrophotometry.
This constitutes the link.
Both the scans and the pointed observations have to be performed in
one orbit each, and only a few orbits apart. Therefore they are declared as
fixed-time observations, however with a time window about ten of days given
for their execution.
=== Object list ===
The list is given both for an autumn launch (30.11.95) and a spring
launch (31.5.96).
object (autumn) object (spring) Observations Priority
-----------------------------------------------------------------
KOPFFSCAN+2.0 KOPFFSCAN+2.0 short photometry 1
KOPFFSCAN-2.0 KOPFFSCAN-2.0 short photometry 1
KOPFFSCAN+5.0 KOPFFSCAN+5.0 short photometry 1
KOPFFSCAN+0.25 KOPFFSCAN+0.25 short photometry 1
KOPFFLATE+2.0 KOPFFLATE+2.0 short photometry 3
KOPFF+2.0,MAX KOPFF+2.0,MAX full photometry 1
KOPFF+0.25,MAX KOPFF+0.25,MAX full photometry 1
spectrophotometry 1
KOPFFBACK+2.0,+0.5 KOPFFBACK+2.0,+0.5 full photometry 1
spectrophotometry 1
KOPFFBACK+2.0,-0.5 KOPFFBACK+2.0,-0.5 full photometry 1
-----------------------------------------------------------------
SCAN:
filter scan performance time
-----------------------------------------------------------
initial acquisition: 180 s
P_12.8 start beta = MAX - 18' 485 s * P05
step 1.5' * concatenated
end beta = MAX + 18'
P_25 same but reverse 596 s (20 s acquisition)
P_60 same as P_12.8 598 s (20 s acquisition)
-----------------------------------------------------------
total 1859 s
POSITIONS:
KOPFFSCAN "a" is a strip of length 36' approximately perpendicular to
the comet trail and "a" deg behind the coma position. Negative values of "a"
mean a position ahead of the comet coma.
KOPFLATE similarly describes the same type of strips but
to be measured later in the visibility interval of the comet in order to look
for temporal changes.
KOPF "a",MAX refers to a position in the maximum of the comet trail, "a" deg
behind the coma.
KOPFBACK "a","b" are background fields positioned "a" deg back along the comet
trail and then offset by "b" deg in beta. Since the comet is at about
beta = -4 deg during the visibility period, positive "b" means closer
to the ecliptic.
VISIBILITIES:
Visibilities both for an autumn launch and for a spring launch
are suitable during end of September and October 1996, possibly extending into
November.
PERFORMANCE TIME:
Priority 1 24988 s (6.9 h)
Priority 2 -
Priority 3 1859 s (0.5 h)
--------------------------------------
Sum 26847 s (7.5 h)
<=== autumn_launch_targets ===>
1, "PHT05", 1.0, "N", "KOPFFSCAN+2.0 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 665, 2
2, "PHT05", 1.0, "N", "KOPFFSCAN+2.0 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 596, 3
3, "PHT05", 1.0, "N", "KOPFFSCAN+2.0 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 598, 0
4, "PHT05", 1.0, "N", "KOPFFSCAN-2.0 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 665, 5
5, "PHT05", 1.0, "N", "KOPFFSCAN-2.0 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 596, 6
6, "PHT05", 1.0, "N", "KOPFFSCAN-2.0 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 598, 0
7, "PHT05", 1.0, "N", "KOPFFSCAN+5.0 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 665, 8
8, "PHT05", 1.0, "N", "KOPFFSCAN+5.0 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 596, 9
9, "PHT05", 1.0, "N", "KOPFFSCAN+5.0 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 598, 0
10, "PHT05", 3.0, "N", "KOPFFSCAN+0.25 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 665, 11
11, "PHT05", 3.0, "N", "KOPFFSCAN+0.25 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 596, 12
12, "PHT05", 3.0, "N", "KOPFFSCAN+0.25 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 598, 0
13, "PHT05", 3.0, "N", "KOPFFLATE+2.0 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 665, 14
14, "PHT05", 3.0, "N", "KOPFFLATE+2.0 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 596, 15
15, "PHT05", 3.0, "N", "KOPFFLATE+2.0 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 598, 0
16, "PHT05", 1.0, "N", "KOPFF+2.0,MAX ", 0.00000, 0.00000, 2000, 0.000, 0.000, 742, 17
17, "PHT05", 1.0, "N", "KOPFF+2.0,MAX ", 0.00000, 0.00000, 2000, 0.000, 0.000, 180, 18
18, "PHT05", 1.0, "N", "KOPFF+2.0,MAX ", 0.00000, 0.00000, 2000, 0.000, 0.000, 114, 19
19, "PHT05", 1.0, "N", "KOPFF+2.0,MAX ", 0.00000, 0.00000, 2000, 0.000, 0.000, 110, 20
20, "PHT05", 1.0, "N", "KOPFF+2.0,MAX ", 0.00000, 0.00000, 2000, 0.000, 0.000, 106, 21
21, "PHT05", 1.0, "N", "KOPFF+2.0,MAX ", 0.00000, 0.00000, 2000, 0.000, 0.000, 98, 22
22, "PHT05", 1.0, "N", "KOPFF+2.0,MAX ", 0.00000, 0.00000, 2000, 0.000, 0.000, 104, 23
23, "PHT05", 1.0, "N", "KOPFF+2.0,MAX ", 0.00000, 0.00000, 2000, 0.000, 0.000, 198, 24
24, "PHT05", 1.0, "N", "KOPFF+2.0,MAX ", 0.00000, 0.00000, 2000, 0.000, 0.000, 200, 25
25, "PHT05", 1.0, "N", "KOPFF+2.0,MAX ", 0.00000, 0.00000, 2000, 0.000, 0.000, 202, 26
26, "PHT25", 1.0, "N", "KOPFF+2.0,MAX ", 0.00000, 0.00000, 2000, 0.000, 0.000, 86, 27
27, "PHT25", 1.0, "N", "KOPFF+2.0,MAX ", 0.00000, 0.00000, 2000, 0.000, 0.000, 76, 28
28, "PHT25", 1.0, "N", "KOPFF+2.0,MAX ", 0.00000, 0.00000, 2000, 0.000, 0.000, 82, 0
29, "PHT05", 1.0, "N", "KOPFF+0.25,MAX ", 0.00000, 0.00000, 2000, 0.000, 0.000, 742, 30
30, "PHT05", 1.0, "N", "KOPFF+0.25,MAX ", 0.00000, 0.00000, 2000, 0.000, 0.000, 180, 31
31, "PHT05", 1.0, "N", "KOPFF+0.25,MAX ", 0.00000, 0.00000, 2000, 0.000, 0.000, 114, 32
32, "PHT05", 1.0, "N", "KOPFF+0.25,MAX ", 0.00000, 0.00000, 2000, 0.000, 0.000, 110, 35
33, "PHT05", 1.0, "N", "KOPFF+0.25,MAX ", 0.00000, 0.00000, 2000, 0.000, 0.000, 106, 34
34, "PHT05", 1.0, "N", "KOPFF+0.25,MAX ", 0.00000, 0.00000, 2000, 0.000, 0.000, 98, 36
35, "PHT05", 1.0, "N", "KOPFF+0.25,MAX ", 0.00000, 0.00000, 2000, 0.000, 0.000, 104, 33
36, "PHT05", 1.0, "N", "KOPFF+0.25,MAX ", 0.00000, 0.00000, 2000, 0.000, 0.000, 198, 37
37, "PHT05", 1.0, "N", "KOPFF+0.25,MAX ", 0.00000, 0.00000, 2000, 0.000, 0.000, 200, 38
38, "PHT05", 1.0, "N", "KOPFF+0.25,MAX ", 0.00000, 0.00000, 2000, 0.000, 0.000, 202, 41
39, "PHT25", 1.0, "N", "KOPFF+0.25,MAX ", 0.00000, 0.00000, 2000, 0.000, 0.000, 86, 40
40, "PHT25", 1.0, "N", "KOPFF+0.25,MAX ", 0.00000, 0.00000, 2000, 0.000, 0.000, 76, 42
41, "PHT25", 1.0, "N", "KOPFF+0.25,MAX ", 0.00000, 0.00000, 2000, 0.000, 0.000, 82, 39
42, "PHT40", 1.0, "N", "KOPFF+0.25,MAX ", 0.00000, 0.00000, 2000, 0.000, 0.000, 4180, 0
43, "PHT05", 1.0, "N", "KOPFFBACK+2.0,+0.5 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 742, 44
44, "PHT05", 1.0, "N", "KOPFFBACK+2.0,+0.5 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 180, 45
45, "PHT05", 1.0, "N", "KOPFFBACK+2.0,+0.5 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 114, 46
46, "PHT05", 1.0, "N", "KOPFFBACK+2.0,+0.5 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 110, 49
47, "PHT05", 1.0, "N", "KOPFFBACK+2.0,+0.5 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 106, 48
48, "PHT05", 1.0, "N", "KOPFFBACK+2.0,+0.5 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 98, 50
49, "PHT05", 1.0, "N", "KOPFFBACK+2.0,+0.5 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 104, 47
50, "PHT05", 1.0, "N", "KOPFFBACK+2.0,+0.5 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 198, 51
51, "PHT05", 1.0, "N", "KOPFFBACK+2.0,+0.5 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 200, 52
52, "PHT05", 1.0, "N", "KOPFFBACK+2.0,+0.5 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 202, 55
53, "PHT25", 1.0, "N", "KOPFFBACK+2.0,+0.5 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 86, 54
54, "PHT25", 1.0, "N", "KOPFFBACK+2.0,+0.5 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 76, 56
55, "PHT25", 1.0, "N", "KOPFFBACK+2.0,+0.5 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 82, 53
56, "PHT40", 1.0, "N", "KOPFFBACK+2.0,+0.5 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 4180, 0
57, "PHT05", 1.0, "N", "KOPFFBACK+2.0,-0.5 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 742, 58
58, "PHT05", 1.0, "N", "KOPFFBACK+2.0,-0.5 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 180, 59
59, "PHT05", 1.0, "N", "KOPFFBACK+2.0,-0.5 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 114, 60
60, "PHT05", 1.0, "N", "KOPFFBACK+2.0,-0.5 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 110, 61
61, "PHT05", 1.0, "N", "KOPFFBACK+2.0,-0.5 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 106, 62
62, "PHT05", 1.0, "N", "KOPFFBACK+2.0,-0.5 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 98, 63
63, "PHT05", 1.0, "N", "KOPFFBACK+2.0,-0.5 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 104, 64
64, "PHT05", 1.0, "N", "KOPFFBACK+2.0,-0.5 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 198, 65
65, "PHT05", 1.0, "N", "KOPFFBACK+2.0,-0.5 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 200, 66
66, "PHT05", 1.0, "N", "KOPFFBACK+2.0,-0.5 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 202, 67
67, "PHT25", 1.0, "N", "KOPFFBACK+2.0,-0.5 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 86, 68
68, "PHT25", 1.0, "N", "KOPFFBACK+2.0,-0.5 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 76, 69
69, "PHT25", 1.0, "N", "KOPFFBACK+2.0,-0.5 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 82, 0
<=== spring_launch_targets ===>
1, "PHT05", 1.0, "N", "KOPFFSCAN+2.0 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 665, 2
2, "PHT05", 1.0, "N", "KOPFFSCAN+2.0 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 596, 3
3, "PHT05", 1.0, "N", "KOPFFSCAN+2.0 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 598, 0
4, "PHT05", 1.0, "N", "KOPFFSCAN-2.0 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 665, 5
5, "PHT05", 1.0, "N", "KOPFFSCAN-2.0 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 596, 6
6, "PHT05", 1.0, "N", "KOPFFSCAN-2.0 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 598, 0
7, "PHT05", 1.0, "N", "KOPFFSCAN+5.0 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 665, 8
8, "PHT05", 1.0, "N", "KOPFFSCAN+5.0 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 596, 9
9, "PHT05", 1.0, "N", "KOPFFSCAN+5.0 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 598, 0
10, "PHT05", 3.0, "N", "KOPFFSCAN+0.25 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 665, 11
11, "PHT05", 3.0, "N", "KOPFFSCAN+0.25 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 596, 12
12, "PHT05", 3.0, "N", "KOPFFSCAN+0.25 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 598, 0
13, "PHT05", 3.0, "N", "KOPFFLATE+2.0 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 665, 14
14, "PHT05", 3.0, "N", "KOPFFLATE+2.0 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 596, 15
15, "PHT05", 3.0, "N", "KOPFFLATE+2.0 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 598, 0
16, "PHT05", 1.0, "N", "KOPFF+2.0,MAX ", 0.00000, 0.00000, 2000, 0.000, 0.000, 742, 17
17, "PHT05", 1.0, "N", "KOPFF+2.0,MAX ", 0.00000, 0.00000, 2000, 0.000, 0.000, 180, 18
18, "PHT05", 1.0, "N", "KOPFF+2.0,MAX ", 0.00000, 0.00000, 2000, 0.000, 0.000, 114, 19
19, "PHT05", 1.0, "N", "KOPFF+2.0,MAX ", 0.00000, 0.00000, 2000, 0.000, 0.000, 110, 20
20, "PHT05", 1.0, "N", "KOPFF+2.0,MAX ", 0.00000, 0.00000, 2000, 0.000, 0.000, 106, 21
21, "PHT05", 1.0, "N", "KOPFF+2.0,MAX ", 0.00000, 0.00000, 2000, 0.000, 0.000, 98, 22
22, "PHT05", 1.0, "N", "KOPFF+2.0,MAX ", 0.00000, 0.00000, 2000, 0.000, 0.000, 104, 23
23, "PHT05", 1.0, "N", "KOPFF+2.0,MAX ", 0.00000, 0.00000, 2000, 0.000, 0.000, 198, 24
24, "PHT05", 1.0, "N", "KOPFF+2.0,MAX ", 0.00000, 0.00000, 2000, 0.000, 0.000, 200, 25
25, "PHT05", 1.0, "N", "KOPFF+2.0,MAX ", 0.00000, 0.00000, 2000, 0.000, 0.000, 202, 26
26, "PHT25", 1.0, "N", "KOPFF+2.0,MAX ", 0.00000, 0.00000, 2000, 0.000, 0.000, 86, 27
27, "PHT25", 1.0, "N", "KOPFF+2.0,MAX ", 0.00000, 0.00000, 2000, 0.000, 0.000, 76, 28
28, "PHT25", 1.0, "N", "KOPFF+2.0,MAX ", 0.00000, 0.00000, 2000, 0.000, 0.000, 82, 0
29, "PHT05", 1.0, "N", "KOPFF+0.25,MAX ", 0.00000, 0.00000, 2000, 0.000, 0.000, 742, 30
30, "PHT05", 1.0, "N", "KOPFF+0.25,MAX ", 0.00000, 0.00000, 2000, 0.000, 0.000, 180, 31
31, "PHT05", 1.0, "N", "KOPFF+0.25,MAX ", 0.00000, 0.00000, 2000, 0.000, 0.000, 114, 32
32, "PHT05", 1.0, "N", "KOPFF+0.25,MAX ", 0.00000, 0.00000, 2000, 0.000, 0.000, 110, 35
33, "PHT05", 1.0, "N", "KOPFF+0.25,MAX ", 0.00000, 0.00000, 2000, 0.000, 0.000, 106, 34
34, "PHT05", 1.0, "N", "KOPFF+0.25,MAX ", 0.00000, 0.00000, 2000, 0.000, 0.000, 98, 36
35, "PHT05", 1.0, "N", "KOPFF+0.25,MAX ", 0.00000, 0.00000, 2000, 0.000, 0.000, 104, 33
36, "PHT05", 1.0, "N", "KOPFF+0.25,MAX ", 0.00000, 0.00000, 2000, 0.000, 0.000, 198, 37
37, "PHT05", 1.0, "N", "KOPFF+0.25,MAX ", 0.00000, 0.00000, 2000, 0.000, 0.000, 200, 38
38, "PHT05", 1.0, "N", "KOPFF+0.25,MAX ", 0.00000, 0.00000, 2000, 0.000, 0.000, 202, 41
39, "PHT25", 1.0, "N", "KOPFF+0.25,MAX ", 0.00000, 0.00000, 2000, 0.000, 0.000, 86, 40
40, "PHT25", 1.0, "N", "KOPFF+0.25,MAX ", 0.00000, 0.00000, 2000, 0.000, 0.000, 76, 42
41, "PHT25", 1.0, "N", "KOPFF+0.25,MAX ", 0.00000, 0.00000, 2000, 0.000, 0.000, 82, 39
42, "PHT40", 1.0, "N", "KOPFF+0.25,MAX ", 0.00000, 0.00000, 2000, 0.000, 0.000, 4180, 0
43, "PHT05", 1.0, "N", "KOPFFBACK+2.0,+0.5 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 742, 44
44, "PHT05", 1.0, "N", "KOPFFBACK+2.0,+0.5 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 180, 45
45, "PHT05", 1.0, "N", "KOPFFBACK+2.0,+0.5 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 114, 46
46, "PHT05", 1.0, "N", "KOPFFBACK+2.0,+0.5 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 110, 49
47, "PHT05", 1.0, "N", "KOPFFBACK+2.0,+0.5 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 106, 48
48, "PHT05", 1.0, "N", "KOPFFBACK+2.0,+0.5 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 98, 50
49, "PHT05", 1.0, "N", "KOPFFBACK+2.0,+0.5 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 104, 47
50, "PHT05", 1.0, "N", "KOPFFBACK+2.0,+0.5 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 198, 51
51, "PHT05", 1.0, "N", "KOPFFBACK+2.0,+0.5 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 200, 52
52, "PHT05", 1.0, "N", "KOPFFBACK+2.0,+0.5 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 202, 55
53, "PHT25", 1.0, "N", "KOPFFBACK+2.0,+0.5 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 86, 54
54, "PHT25", 1.0, "N", "KOPFFBACK+2.0,+0.5 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 76, 56
55, "PHT25", 1.0, "N", "KOPFFBACK+2.0,+0.5 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 82, 53
56, "PHT40", 1.0, "N", "KOPFFBACK+2.0,+0.5 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 4180, 0
57, "PHT05", 1.0, "N", "KOPFFBACK+2.0,-0.5 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 742, 58
58, "PHT05", 1.0, "N", "KOPFFBACK+2.0,-0.5 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 180, 59
59, "PHT05", 1.0, "N", "KOPFFBACK+2.0,-0.5 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 114, 60
60, "PHT05", 1.0, "N", "KOPFFBACK+2.0,-0.5 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 110, 61
61, "PHT05", 1.0, "N", "KOPFFBACK+2.0,-0.5 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 106, 62
62, "PHT05", 1.0, "N", "KOPFFBACK+2.0,-0.5 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 98, 63
63, "PHT05", 1.0, "N", "KOPFFBACK+2.0,-0.5 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 104, 64
64, "PHT05", 1.0, "N", "KOPFFBACK+2.0,-0.5 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 198, 65
65, "PHT05", 1.0, "N", "KOPFFBACK+2.0,-0.5 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 200, 66
66, "PHT05", 1.0, "N", "KOPFFBACK+2.0,-0.5 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 202, 67
67, "PHT25", 1.0, "N", "KOPFFBACK+2.0,-0.5 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 86, 68
68, "PHT25", 1.0, "N", "KOPFFBACK+2.0,-0.5 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 76, 69
69, "PHT25", 1.0, "N", "KOPFFBACK+2.0,-0.5 ", 0.00000, 0.00000, 2000, 0.000, 0.000, 82, 0