Commit 233f1880830d529046e306d67c5817e4e3f037b4

Authored by Elena.Budnik
1 parent ad7a238e

LAP descr

Showing 1 changed file with 21 additions and 1 deletions   Show diff stats
Instrument/AMDA/Rosetta/LAP.xml
... ... @@ -7,7 +7,27 @@
7 7 <ResourceName>LAP</ResourceName>
8 8 <AlternateName>Langmuir Probe</AlternateName>
9 9 <ReleaseDate>2009-05-20T21:10:13Z</ReleaseDate>
10   - <Description></Description>
  10 + <Description> The ESA Rosetta mission to comet 67P/Churyumov-Gerasimenko carried a small but
  11 + comprehensive set of plasma instruments known as the Rosetta Plasma Consortium (RPC),
  12 + monitoring the cometary plasma from arrival in August 2014 to end of mission in September
  13 + 2016. Among the RPC instruments was the Langmuir probe instrument LAP, with chief
  14 + mission to measure:
  15 + * Plasma density, ne
  16 + * Spacecraft potential, Vsc
  17 + * Electron temperature, Te
  18 + * Electric field, E
  19 + * Ion flow speed, ui
  20 + * Photoemission current, Iph
  21 + * Wave activity
  22 +
  23 + The LAP sensors are two spherical probes, 5 cm in diameter, known as LAP1 and LAP2, one
  24 +on each of the two booms protruding a few meters from the s/c body. The primary
  25 +parameters actually measured by the instrument is the current flowing to (or the voltage of)
  26 +the probes when some bias voltage (or bias current) is applied to it, which are the data
  27 +transmitted to ground. From these data the parameters above have been derived, for some
  28 +products also with use of data from RPC-MIP. Do not expect all parameters to be available at
  29 +any given time.
  30 + </Description>
11 31 <Contact>
12 32 <PersonID>spase://CDPP/Person/Anders.Eriksson</PersonID>
13 33 <Role>PrincipalInvestigator</Role>
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