CDPP / CNES

Commit dca1ad38b28276b3ee518b6ca4e1ba74a9e6e106

Authored by Elena.Budnik
1 parent 3783d46a
Exists in master and in 12 other branches amdadev, aschulz, autocommit, bepi_master, bepi_update, branch_q, cleanup_registry, cleanup_registry_master, cleanup_registry_merged, juice_jdc, juno_jade, soar

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Showing 2 changed files with 26 additions and 26 deletions   Show diff stats
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Instrument/AMDA/Helios1/MAG.xml
  Diff comments   View file @dca1ad3
... ... @@ -7,24 +7,24 @@
7 7 <ResourceName>MAG</ResourceName>
8 8 <AlternateName>Helios Magnetometers : E2, E3</AlternateName>
9 9 <ReleaseDate>2018-10-20T21:10:13Z</ReleaseDate>
10   - <Description>E2 : The Förster probe experiment E2 is a three component-vector magnetometer. Its purpose is to
11   -continuously observe the interplanetary magnetic field in a frequency range up to 4 Hz. Thereby certain
12   -phenomena are to be analysed as a function of the distance from the sun e.g. the spiral structure and
  10 + <Description>E2 : The Förster probe experiment E2 is a three component-vector magnetometer. Its purpose is to
  11 +continuously observe the interplanetary magnetic field in a frequency range up to 4 Hz. Thereby certain
  12 +phenomena are to be analysed as a function of the distance from the sun e.g. the spiral structure and
13 13 discontinuities. The measurement ranges are ± 100 nT and ± 400 nT. The resolution is ± 0.2 nT and ±
14 14 0.8 nT respectively.
15 15  
16   -For accurate measurements of the zero offset of each sensor the component parallel to the spinaxis can
17   -be flipped by 90°. Depending on telemetry format and bitrate the digital data are fed into a time average
18   -computer or directly connected to telemetry. A shock identification-computer triggers the S/C core
  16 +For accurate measurements of the zero offset of each sensor the component parallel to the spinaxis can
  17 +be flipped by 90°. Depending on telemetry format and bitrate the digital data are fed into a time average
  18 +computer or directly connected to telemetry. A shock identification-computer triggers the S/C core
19 19 memory in case of discontinuities with variations of the ambient magnetic field magnitude.
20 20  
21   -The Förster probe experiment E2 is a three-axe vector magnetometer. It is used for the continuous
22   -observation of the interplanetary magnetic field in a frequency range from 0 to 4 Hz. This will be
23   -investigated phenomena such as the spiral structure and discontinuities as a function of the distance
24   -from the Sun. The measuring ranges are ± 100 nT and ± 400 nT with a resolution of ± 0.2 nT or ± 0.8 nT.
25   -The component that is parallel to the axis of the spin, to perform precise zero point provisions of each
26   -sensor is rotated 90 degrees. Depending on format and bit rate digital data pass through an average
27   -computer or directly to the telemetry. A shock wave identification computer triggers the S/C core memory
  21 +The Förster probe experiment E2 is a three-axe vector magnetometer. It is used for the continuous
  22 +observation of the interplanetary magnetic field in a frequency range from 0 to 4 Hz. This will be
  23 +investigated phenomena such as the spiral structure and discontinuities as a function of the distance
  24 +from the Sun. The measuring ranges are ± 100 nT and ± 400 nT with a resolution of ± 0.2 nT or ± 0.8 nT.
  25 +The component that is parallel to the axis of the spin, to perform precise zero point provisions of each
  26 +sensor is rotated 90 degrees. Depending on format and bit rate digital data pass through an average
  27 +computer or directly to the telemetry. A shock wave identification computer triggers the S/C core memory
28 28 in the presence of discontinuities with magnetic field variations.
29 29  
30 30 E3 : The Rome‐GSFC magnetic field experiment utilized a triaxial fluxgate (saturable inductor) 
... ...
Instrument/AMDA/Helios2/MAG.xml
  Diff comments   View file @dca1ad3
... ... @@ -7,24 +7,24 @@
7 7 <ResourceName>MAG</ResourceName>
8 8 <AlternateName>Helios Magnetometers : E2, E3</AlternateName>
9 9 <ReleaseDate>2018-10-20T21:10:13Z</ReleaseDate>
10   - <Description>E2 : The Förster probe experiment E2 is a three component-vector magnetometer. Its purpose is to
11   -continuously observe the interplanetary magnetic field in a frequency range up to 4 Hz. Thereby certain
12   -phenomena are to be analysed as a function of the distance from the sun e.g. the spiral structure and
  10 + <Description>E2 : The Förster probe experiment E2 is a three component-vector magnetometer. Its purpose is to
  11 +continuously observe the interplanetary magnetic field in a frequency range up to 4 Hz. Thereby certain
  12 +phenomena are to be analysed as a function of the distance from the sun e.g. the spiral structure and
13 13 discontinuities. The measurement ranges are ± 100 nT and ± 400 nT. The resolution is ± 0.2 nT and ±
14 14 0.8 nT respectively.
15 15  
16   -For accurate measurements of the zero offset of each sensor the component parallel to the spinaxis can
17   -be flipped by 90°. Depending on telemetry format and bitrate the digital data are fed into a time average
18   -computer or directly connected to telemetry. A shock identification-computer triggers the S/C core
  16 +For accurate measurements of the zero offset of each sensor the component parallel to the spinaxis can
  17 +be flipped by 90°. Depending on telemetry format and bitrate the digital data are fed into a time average
  18 +computer or directly connected to telemetry. A shock identification-computer triggers the S/C core
19 19 memory in case of discontinuities with variations of the ambient magnetic field magnitude.
20 20  
21   -The Förster probe experiment E2 is a three-axe vector magnetometer. It is used for the continuous
22   -observation of the interplanetary magnetic field in a frequency range from 0 to 4 Hz. This will be
23   -investigated phenomena such as the spiral structure and discontinuities as a function of the distance
24   -from the Sun. The measuring ranges are ± 100 nT and ± 400 nT with a resolution of ± 0.2 nT or ± 0.8 nT.
25   -The component that is parallel to the axis of the spin, to perform precise zero point provisions of each
26   -sensor is rotated 90 degrees. Depending on format and bit rate digital data pass through an average
27   -computer or directly to the telemetry. A shock wave identification computer triggers the S/C core memory
  21 +The Förster probe experiment E2 is a three-axe vector magnetometer. It is used for the continuous
  22 +observation of the interplanetary magnetic field in a frequency range from 0 to 4 Hz. This will be
  23 +investigated phenomena such as the spiral structure and discontinuities as a function of the distance
  24 +from the Sun. The measuring ranges are ± 100 nT and ± 400 nT with a resolution of ± 0.2 nT or ± 0.8 nT.
  25 +The component that is parallel to the axis of the spin, to perform precise zero point provisions of each
  26 +sensor is rotated 90 degrees. Depending on format and bit rate digital data pass through an average
  27 +computer or directly to the telemetry. A shock wave identification computer triggers the S/C core memory
28 28 in the presence of discontinuities with magnetic field variations.
29 29  
30 30 E3 : The Rome‐GSFC magnetic field experiment utilized a triaxial fluxgate (saturable inductor) 
... ...