2.4.1
spase://CNES/NumericalData/CDPP-AMDA/PSP/epiHi/psp-let2-1min
LET2 1min
Low Energy Telescope 2, 1 min rate
2024-09-23T15:19:38Z
LET1 and LET2 are similar in design to the HET, cylinders containing a central stack of detector disks and positionally
sensitive detectors at the ends. LET1 has 1000-micron thick detector disks in the central stack, except for the end disks
which are 500 microns. At the front of the cylinder, separate from the central stack, is a 12 micron thick disk and then a
25 micron disk. The back of the detector has the same arrangement. The front of the detector also has a thin window
(~3 micron silicon equivalent). The 12, 25, and 500 micron thick disks are all separated into five active elements in the
same way as the HET for positional determination. LET2 is similar to LET1 but does not have the end 12, 25, and 500 micron disks.
The Low-Energy Telescopes can measure protons and heavy ions from approximately
1 MeV to greater than 20 MeV/n and electrons from about 0.5 MeV to 2 MeV.
LET2 telescope, unlike LET1 and HET, is single sided, with its only side called C, oriented at +135° from the sunward direction.
Please acknowledge the National Aeronautics and Space Administration, NASA
spase://SMWG/Person/David.J.McComas
PrincipalInvestigator
spase://SMWG/Person/Eric.R.Christian
DeputyPI
PSP/ISoIS Energetic Particle Data - User Guide
https://spdf.sci.gsfc.nasa.gov/pub/data/psp/isois/ISOIS_Data_Glossary.pdf
Parker Solar Probe Mission Instrument web page, JPL
http://parkersolarprobe.jhuapl.edu/Spacecraft/index.php#Instruments
psp-isois-let2
PartOf
LET2
spase://SMWG/Repository/CDPP/AMDA
Online
Open
CDPP/AMDA HAPI Server
https://amda.irap.omp.eu/service/hapi
psp-let2-1min
Web Service to this product using the HAPI interface.
CSV
Thank you for acknowledging the use of AMDA in publications with wording like "Data analysis was performed with the AMDA science analysis system provided by the Centre de Données de la Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and Université Paul Sabatier, Toulouse". See the Rules of the road at https://amda.cdpp.eu/help/policy.html . Please acknowledge the Data Providers.
spase://SMWG/Repository/CDPP/AMDA
Online
Open
CDPP/AMDA Web application
https://amda.cdpp.eu
Access to Data via CDPP/AMDA Web application.
CSV
VOTable
CDF
PNG
Thank you for acknowledging the use of AMDA in publications with wording like "Data analysis was performed with the AMDA science analysis system provided by the Centre de Données de la Physique des Plasmas (CDPP) supported by CNRS, CNES, Observatoire de Paris and Université Paul Sabatier, Toulouse". See the Rules of the road at https://amda.cdpp.eu/help/policy.html . Please acknowledge the Data Providers.
SPDF
spase://CNES/Instrument/CDPP-AMDA/PSP/epiHi
EnergeticParticles
2018-09-28T00:00:26Z
2024-06-16T23:59:39Z
PT60S
Heliosphere.Inner
Sun.Corona
h+ flux side C
psp_let2_1min_Hf
Proton flux side C
1/cm²/sr/s/(MeV/nuc)
Spectrogram
EnergyFlux
h+ uncertainty
psp_let2_1min_Hfu
Proton flux side C uncertainty
1/cm²/sr/s/(MeV/nuc)
Spectrogram
EnergyFlux
he flux side C
psp_let2_1min_Hef
Helium flux side C
1/cm²/sr/s/(MeV/nuc)
Spectrogram
EnergyFlux
he uncertainty
psp_let2_1min_Hefu
Helium flux side C uncertainty
1/cm²/sr/s/(MeV/nuc)
Spectrogram
EnergyFlux