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MAVEN Solar Energetic Particle, SEP, Instrument

ResourceID
spase://SMWG/Instrument/MAVEN/SEP

Description

The Solar Energetic Particle, SEP, Instrument will characterize the Relationship between Solar Energetic Particle Events and Martian Atmospheric Escape. The SEP measures the Energy and Angular Distribution of Energetic Protons and Electrons in the Energy Range absorbed by the Upper Atmosphere. The main Instrument comprises two orthogonal dual double-ended Solid State Telescopes with passive Ion-implanted Silicon Detectors, giving it four Look Directions.

The SEP can measure Proton Energies from 25 keV to 6 MeV and Electrons from 25 keV to 1 MeV. It can measure Particle Fluxes from 20/(cm² s sr) to 107/(cm² s sr). It has three Measurement Frequencies depending on Orbital Distance from the Surface: once every 2 s below 300 km, 8 s from 300 km to 800 km, and 32 s beyond 800 km.

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Details

Version:2.3.2

Instrument

ResourceID
spase://SMWG/Instrument/MAVEN/SEP
ResourceHeader
ResourceName
MAVEN Solar Energetic Particle, SEP, Instrument
AlternateName
MAVEN SEP Instrument
ReleaseDate
2021-05-30 12:34:56.789
RevisionHistory
RevisionEvent
ReleaseDate
2021-05-30 12:34:56.789
Note
Updated to SPASE Version 2.3.2 if needed, Applied quality conntrol for DOI usage, LFB
Description

The Solar Energetic Particle, SEP, Instrument will characterize the Relationship between Solar Energetic Particle Events and Martian Atmospheric Escape. The SEP measures the Energy and Angular Distribution of Energetic Protons and Electrons in the Energy Range absorbed by the Upper Atmosphere. The main Instrument comprises two orthogonal dual double-ended Solid State Telescopes with passive Ion-implanted Silicon Detectors, giving it four Look Directions.

The SEP can measure Proton Energies from 25 keV to 6 MeV and Electrons from 25 keV to 1 MeV. It can measure Particle Fluxes from 20/(cm² s sr) to 107/(cm² s sr). It has three Measurement Frequencies depending on Orbital Distance from the Surface: once every 2 s below 300 km, 8 s from 300 km to 800 km, and 32 s beyond 800 km.

Acknowledgement
National Aeronautics and Space Administration, NASA, Space Sciences Laboratory, University of California, Berkeley
Funding
Agency
National Aeronautics and Space Administration, Mars Scout Program
Project
MAVEN Solar Energetic Particle Investigation
AwardNumber
UNKNOWN
Contacts
RolePersonStartDateStopDateNote
1.PrincipalInvestigatorspase://SMWG/Person/Davin.Larson
2.MetadataContactspase://SMWG/Person/Lee.Frost.Bargatze
InformationURL
Name
The Mars Atmosphere and Volatile Evolution, MAVEN, Solar Energetic Particle Instrument Home Page, LASP, UC Boulder
URL
Description

The Mars Atmosphere and Volatile Evolution, MAVEN, Solar Energetic Particle Instrument Home Page, Laboratory of Atmospheric and Space Physics, LASP, University of Colorado, Boulder

InformationURL
Name
MAVEN Solar Energetic Particle, SEP, Instrument paper, Published by Space Sci. Rev., Date: 2015-03-29
URL
Description

Author List: Larson, D. E., Lillis, R. J., Lee, C. O., Dunn, P. A., Hatch, K., Robinson, M., Glaser, D., Chen, J., Curtis, D. W., Tiu, C., Lin, R. P., Luhmann, J. G., & Jakosky, B. M.

InformationURL
Name
NSSDC Master Catalog Listing, MAVEN Solar Energetic Particle, SEP, Instrument
URL
Description

NSSDC Master Catalog Listing for the MAVEN Solar Energetic Particle, SEP, Instrument, NSSDCA/COSPAR ID: 2013-063A-05

InstrumentType
SolidStateDetector
InvestigationName
MAVEN Solar Energetic Particle Investigation
OperatingSpan
StartDate
2013-11-18 18:28:00
Note
MAVEN Launch Date and Time until data are available
ObservatoryID