HDPWS

MAVEN - MAG - 0.03 sec

ResourceID
spase://CNES/NumericalData/CDPP-AMDA/MAVEN/MAG/mav-mag-pds

Description
* Calibrated science vector magnetic-field data in Planetocentric coordinates (IAU Mars) vs. time (LID = urn:nasa:pds:maven.mag.calibrated:data.pc) * Calibrated science vector magnetic-field in Sun-State (MSO) coordinates vs. time (LID = urn:nasa:pds:maven.mag.calibrated:data.ss)

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Version:2.4.1

NumericalData

ResourceID
spase://CNES/NumericalData/CDPP-AMDA/MAVEN/MAG/mav-mag-pds
ResourceHeader
ResourceName
MAVEN - MAG - 0.03 sec
ReleaseDate
2024-08-19 14:49:09Z
Description
* Calibrated science vector magnetic-field data in Planetocentric coordinates (IAU Mars) vs. time (LID = urn:nasa:pds:maven.mag.calibrated:data.pc) * Calibrated science vector magnetic-field in Sun-State (MSO) coordinates vs. time (LID = urn:nasa:pds:maven.mag.calibrated:data.ss)
Acknowledgement
Principal Investigator : John E.P. Connerney, NASA GODDARD, Greenbelt
Contacts
Role Person StartDate StopDate Note
1. PrincipalInvestigator spase://SMWG/Person/John.E.P.Connerney
InformationURL
AccessInformation
RepositoryID
Availability
Online
AccessRights
Open
AccessURL
Name
CDPP/AMDA HAPI Server
URL
Style
HAPI
ProductKey
mav-mag-pds
Description
Web Service to this product using the HAPI interface.
Format
CSV
Acknowledgement
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.
AccessInformation
RepositoryID
Availability
Online
AccessRights
Open
AccessURL
Name
CDPP/AMDA Web application
URL
Description
Access to Data via CDPP/AMDA Web application.
Format
CSV
Format
VOTable
Format
CDF
Format
PNG
Acknowledgement
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.
ProviderName
PDS
ProviderResourceName
maven-mag-calibrated/pc[ss]/highres
InstrumentIDs
MeasurementType
MagneticField
TemporalDescription
TimeSpan
StartDate
2014-10-10 00:00:00Z
StopDate
2024-05-01 00:00:02Z
Cadence
PT0.031S
ObservedRegion
Mars
Caveats
MAG data products are provided in several useful coordinate systems and at the highest time resolution available. The MAG observations contain some known artifacts that you may encounter in your use of the data that you should be aware of. These are related to several different sources on the spacecraft that have been, and continue to be, under investigation. This message is dated April 10, 2015, and it represents our current (and evolving) understanding of the status of the spacecraft and its influence on MAG data. These include: * rapid magnetic field variations of ~6 nT in magnitude (in spacecraft payload coordinate axes y and z) associated with infrequent thruster firings (every few days) that are employed in trajectory correction maneuvers (TCM). These are relatively easy to identify. * variations (in spacecraft payload coordinate axes y and z) of ~1 nT in magnitude associated with solar array currents in circuits at the outer edge of the solar arrays, near the magnetometer sensor. MAG processing mitigates these signatures where spacecraft engineering telemetry is available at high time resolution. The necessary spacecraft engineering data was made available after Jan 9, 2015, following in-flight spacecraft testing to isolate the problem. Prior to this time, we use a coarse indication of solar array currents to correct the data, and this correction will be out of time step with the actual needed correction part of the time. Corrections applied are listed on each record along with the corrected data. These variations may appear as step functions, e.g., when the spacecraft enters eclipse, or slow variations as the spacecraft attitude with respect to the sun varies. They were identified in the quiet, weak field environment of cruise and when illumination on the solar arrays was more intense than experienced in cruise. * multiple sinewave variations usually of ~0.1 nT in magnitude, that track the frequency of operation of the four Reaction Wheel Assemblies (RWAs). The magnitude of these variations has been observed to increase substantially when the RWAs are operated at very low frequencies; at such times they may appear prominently in spectra of MAG observations. * the "static" or slowly-varying spacecraft field has been estimated using spacecraft roll maneuvers that are scheduled to occur approximately every 2 months. The MAVEN static sc field specification was NTE 2 nT. The MAG data processed for December 2014 use an estimate of the spacecraft field obtained from the day 353 2014 magroll maneuvers, the only set performed subsequent to deployment of the APP after insertion into Mars orbit. We have yet to verify if this sc field estimate remains relatively constant or if it varies over the interval between magroll maneuvers. Investigation of the time variability of this part of the sc field is expected shortly.
Parameter #1
Name
b_mso
ParameterKey
mavb_mso
UCD
phys.magField
Units
nT
Structure
Size
3
Element
Name
bx
Index
1
ParameterKey
mavb_mso(0)
Element
Name
by
Index
2
ParameterKey
mavb_mso(1)
Element
Name
bz
Index
3
ParameterKey
mavb_mso(2)
Field
FieldQuantity
Magnetic
Parameter #2
Name
b_iau_mars
ParameterKey
mavb_iau
UCD
phys.magField
Units
nT
Structure
Size
3
Element
Name
bx
Qualifier
Component
Index
1
ParameterKey
mavb_iau(0)
Element
Name
by
Qualifier
Component
Index
2
ParameterKey
mavb_iau(1)
Element
Name
bz
Qualifier
Component
Index
3
ParameterKey
mavb_iau(2)
Field
FieldQuantity
Magnetic
Parameter #3
Name
|b|
ParameterKey
mavb_tot
UCD
phys.magField
Units
nT
Field
FieldQuantity
Magnetic