ResourceName
Ulysses Cosmic Ray and Solar Particle Investigation (COSPIN) High Energy Telescope (HET) Full Resolution Proton Counts and Accumulation Times for Eight-Sectored Coincidence Counting Rates, SECT2 H45S, 128 s Data
ReleaseDate
2020-07-07 21:15:40Z
Description
A Directory containing Daily FTP downloadable Files containing Readout-by-Readout Listings of the Counts accumulated in each Spin Sector of the Eight-Sectored H45S Counting Rate. Aside from its Division of Counts into Spin Sectors, H45S is a Coincidence Counting Rate with Coincidence Logic Requirements satisfying the Logical inclusive OR of the H4 and H5 Spin-Averaged Counting Rates. Therefore the H45S Counting Rate responds primarily to Protons in the approximate Energy Range 34-92 MeV. The Naming Convention for the Daily Files is uly_het_full_rat_sect2_YYYDDD.txt, where YYY indicates the three digit Year since 1900 (e.g. YYY=090 for 1990, and YYY=102 for 2002) and DDD indicates the three digit Day of Year (January 1 = 1). In each File, following a detailed Description of the Format, the Data consist of a Readout by Readout Listing of Counts accumulated in the eight 45° Spin Sectors of the Sectored Counting Rate H45S during the Intervals between successive Readouts, organized into Columns as described below. The first four Columns give the Start Time of the Counting Rate Accumulation Period for Sector 7 of the Rate as Fractional Year (to 12 Decimal Places) and as Year since 1900, Day of Year, and Milliseconds of Day at the Start of the Accumulation, followed by one Column (labeled cov) giving the Duration of the total Accumulation Period for all eight Sectors in Milliseconds. Thus the Accumulation Period in each of the Sectors is the Value given in the "cov" Column divided by eight. The Accumulation in each of the successive Sectors 7,8,1,2,3,4,5, and 6 starts cov/8 Milliseconds after the Start of the Accumulation in the previous Sector. Columns 6-13 then give the Counts accumulated in each of the eight Sectors during the Accumulation Period. Each Line contains Data for one single Readout Accumulation of the eight Sectors of H45S. Since the Accumulation Period for each Readout is forced to include an Integral Number of Spacecraft Spins in order to produce equal Coverage in all Sectors, the Lengths of the Accumulation Periods vary in a Cyclic Manner as the Period of the Telemetry Cycle beats with the Spacecraft Spin Period. The H45S Counting Rate is fully read out every 128 s at the most common Science Telemetry Bit Rate (2048 bps). Thus, with a typical 5 rpm Spacecraft Spin Rate the Accumulation Intervals vary in a repeating Cycle of 132, 132, 120, 132, 132, 120, etc., seconds. At lower Bit Rates the Average Interval is equal to 128 times (2048/BR) seconds and the Cycle automatically adjusts to produce this Average Accumulation. The Spin Plane of the Ulysses Spacecraft, in which the Sectors are defined, is normal to the Spin Axis (Spacecraft +Z Axis), which is maintained within one to 2° of Earth pointing at all Times. Viewed from Earth the Spacecraft spins Counter Clockwise. The Start of Sector 1 is defined by the Spacecraft Generated Sun Pulse, which is issued when the Sun crosses the +X/+Z Quadrant of the X/Z Plane. The HET Telescope Axis is parallel to the +X Axis and normal to the Z Axis. No Noise Removal or Despiking has been done, so Caution must be used in interpreting isolated large Increases or Decreases in the Counting Rates.
Acknowledgement
Please acknowledge the COSPIN HET Lead Investigator and COSPIN PI, R. Bruce McKibben
Contacts
InformationURL
Name
The Ulysses Cosmic Ray and Solar Particle Investigation, COSPIN
URL
Description
Published Description of the COSPIN Instrumentation, J.A. Simpson et al., Astron. Astrophys. Suppl. Ser. 92, 365-399, 1992. See especially Section 4.3 for a detailed Description of the High Energy Telescopes, HET. An electronic Copy of this Paper is available at http://adsbit.harvard.edu/cgi-bin/nph-iarticle_query?1992A%26AS...92..365S&defaultprint=YES&filetype=.pdf.
InformationURL
Name
User Notes for the COSPIN/HET Data Files
URL
Description
The User Notes File at the Ulysses Final Archive (UFA) describes the Format of the ASCII Data Files for the COSPIN High Energy Telescope, HET
InformationURL
Name
COSPIN HET Full Resolution ReadMe Document, Word Format
URL
Description
Top Level Descriptions of Formats and Contents of the six File Types that make up the COSPIN HET Full Resolution Data Set. Detailed Descriptions of the Formats and Contents are found in Header Lines at the Start of each downloaded Data File. The Data covered by this SPASE Description are described in the ReadMe under the Heading sect2. (*** Note ***: During the Build-up of this Data Set, a few Errors and Omissions have been found in the Header Lines for some of the File Types. These Errors and Omissions are listed in this ReadMe File. Upon Completion of the Data Set, all Errors and Omissions discovered will be corrected in all of the Header Lines of all of the File Types at which time this Note will be removed).
Association
AssociationID
AssociationType
Other
Association
AssociationID
AssociationType
Other
Association
AssociationID
AssociationType
Other
PriorIDs
spase://VEPO/NumericalData/Ulysses/COSPIN/HET/FullResolution/Rates/Sect2
spase://VSPO/NumericalData/Ulysses/COSPIN/HET/Rates/Sect2/PT128S
Name
Counts per sector for COSPIN/HET Eight-Sectored Counting Rate H45S
Description
Counts accumulated in each of the 8 sectors of counting rate H45S during the accumulation period starting at the time given in columns 1-4 and with a duration as given in column 5. Each sector contains counts incident from a specific 45° sector of the spin plane. The start of sector 1 (0°) is coincident with the spacecraft-generated Sun-pulse, and the start of each subsequent sector is shifted by 45° with respect to the preceding sector. For example, H45S1 covers the azimuthal range 0° to 45°, H45S2 covers the azimuthal range 45° to 90°, etc. In each sector, counts are registered only when the Axis of the Telescope view cone is within that sector. The H45S normally responds primarily to protons in the energy interval from about 34-92 MeV.
Caveats
Because the orbit of the spacecraft about the Sun lies in a plane inclined 80° to the heliographic equator, and because the spacecraft spin Axis (and thus the Axis of the high gain antenna) be pointed at Earth within 2° at all times, determination of the direction in space corresponding to the start of sector 1 can be complex. Depending upon conditions, H45S may also respond to heavier nuclei, primarily Helium in the energy range from about 34-92 MeV/n, and to electrons in the energy range from about 5-10 MeV. When significant electron contamination is present, the H7 spin-averaged rate and/or the H7S sectored rate should also be elevated and closely tracking the H45S rate.
Cadence
PT128S
Structure
Size
8
Element
Name
H45S1
Index
1
ParameterKey
Column_6
ValidMin
0
ValidMax
1000000
FillValue
-1
Element
Name
H45S2
Index
2
ParameterKey
Column_7
ValidMin
0
ValidMax
1000000
FillValue
-1
Element
Name
H45S3
Index
3
ParameterKey
Column_8
ValidMin
0
ValidMax
1000000
FillValue
-1
Element
Name
H45S4
Index
4
ParameterKey
Column_9
ValidMin
0
ValidMax
1000000
FillValue
-1
Element
Name
H45S5
Index
5
ParameterKey
Column_10
ValidMin
0
ValidMax
1000000
FillValue
-1
Element
Name
H45S6
Index
6
ParameterKey
Column_11
ValidMin
0
ValidMax
1000000
FillValue
-1
Element
Name
H45S7
Index
7
ParameterKey
Column_12
ValidMin
0
ValidMax
1000000
FillValue
-1
Element
Name
H45S8
Index
8
ParameterKey
Column_13
ValidMin
0
ValidMax
1000000
FillValue
-1
Particle
ParticleType
Proton
ParticleQuantity
Counts
EnergyRange