CDPP / CNES

Commit 1a085c3f48ec74380dcdc0f437a06abb1fdbe584

Authored by Benjamin Renard
1 parent a25755ce
Exists in juice_jdc and in 4 other branches amdadev, autocommit, cleanup_registry_master, cleanup_registry_merged

monor fix

Showing 1 changed file with 14 additions and 12 deletions   Show diff stats
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Instrument/CDPP-AMDA/JASON3/AMBRE.xml
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... ... @@ -7,19 +7,21 @@
7 7 <ResourceName>AMBRE</ResourceName>
8 8 <AlternateName>Active Monitor Box of Electrostatic Risks</AlternateName>
9 9 <ReleaseDate>2020-09-30T21:10:13Z</ReleaseDate>
10   - <Description>The AMBRE experiment onboard the ocean topography mapper JASON-3 aims at measuring
11   - the spacecraft potential as well as auroral particle precipitation using two top-hat analyzers
12   - for electrons and ions in the 20 eV–28 keV energy range. The JASON-3 spacecraft has a nearly
13   - circular orbit at an altitude of 1,336 km with an inclination of 66°, at times probing the equatorward
  10 + <Description>The AMBRE experiment onboard the ocean topography mapper JASON-3 aims at measuring
  11 + the spacecraft potential as well as auroral particle precipitation using two top-hat analyzers
  12 + for electrons and ions in the 20 eV–28 keV energy range. The JASON-3 spacecraft has a nearly
  13 + circular orbit at an altitude of 1,336 km with an inclination of 66°, at times probing the equatorward
14 14 part of the auroral oval in a nearly tangential manner upon leaving the outer radiation belt.
15   - AMBRE consists of two coupled top-hat analyzers, one for ions and the other for electrons in the 20 eV–28 keV
16   - energy range. The field of view of both spectrometers is 180° × 6° centered on the zenith. The 180° plane
17   - of view is divided into four anodes, the two central ones (sectors 2 and 3) looking at precipitating
18   - particles while the two side ones (sectors 1 and 4) record nearly trapped particles (note that the angular
19   - resolution of each anode is only ~35°). The geometries of both electron and ion analyzers are identical,
20   - except that the electron analyzer has an entrance grid with a transparency of 10% (Sauvaud & Payan, 2017).
21   - The AMBRE spectrometers provide particle spectra with 128, 32, or 16 energy steps with a time resolution
22   - that varies from 0.5 to 2 s. The geometrical factor of a single anode is 1.7 · 10−3 cm2.ster.eV/eV for ions
  15 +
  16 + AMBRE consists of two coupled top-hat analyzers, one for ions and the other for electrons in the 20 eV–28 keV
  17 + energy range. The field of view of both spectrometers is 180° × 6° centered on the zenith. The 180° plane
  18 + of view is divided into four anodes, the two central ones (sectors 2 and 3) looking at precipitating
  19 + particles while the two side ones (sectors 1 and 4) record nearly trapped particles (note that the angular
  20 + resolution of each anode is only ~35°). The geometries of both electron and ion analyzers are identical,
  21 + except that the electron analyzer has an entrance grid with a transparency of 10% (Sauvaud and Payan, 2017).
  22 +
  23 + The AMBRE spectrometers provide particle spectra with 128, 32, or 16 energy steps with a time resolution
  24 + that varies from 0.5 to 2 s. The geometrical factor of a single anode is 1.7 · 10−3 cm2.ster.eV/eV for ions
23 25 and 1.5 · 10−4 cm2.ster.eV/eV for electrons.
24 26 </Description>
25 27 <Acknowledgement/>
... ...