Version:2.4.1
NumericalData
ResourceID
spase://CNES/NumericalData/CDPP-AMDA/MGS/Proxy/mgs-proxy-drap
ResourceHeader
ResourceName
MGS - Proxy - imf draping direction
ReleaseDate
2012-03-06 20:46:16Z
Description
Draping direction is calculated on an orbit-by-obit basis using MGS data from time periods when the spacecraft was above 50-60 N planetary latitude on the Martian dayside. We use this small latitude range in an attempt to minimize the contaminating effects of crustal magnetic fields, which are weakest in this latitude band. Draping direction is reported as the median azimuth angle from each orbit, with 0o pointing locally Eastward from the spacecraft, and 90o pointing locally Northward.
We have tried several other methods of determining draping direction - all have strengths and weaknesses. In the future we may include the results of some of these other methods on this page
Contacts
InformationURL
Name
MGS Proxy webpage
URL
AccessInformation
RepositoryID
Availability
Online
AccessRights
Open
AccessURL
Name
CDPP/AMDA HAPI Server
URL
Style
HAPI
ProductKey
mgs-proxy-drap
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
David Brain
InstrumentIDs
MeasurementType
MagneticField
TemporalDescription
TimeSpan
StartDate
1999-04-02 15:50:49Z
StopDate
2006-10-27 14:20:34Z
CadenceMin
PT1H
CadenceMax
PT2H
ObservedRegion
Mars
Caveats
* IMF direction can change on any timescale, from seconds to minutes to hours to days. Therefore, determination of the direction of the ambient magnetic field between 50-60 N latitude on the dayside maynot provide a reliable indication of the IMF direction over an entire MGS 2-hour orbital period. Please use appropriate caution when using the information on this page.
* We do not believe that IMF draping direction is accurate to more than ~90o, due to contributions of ionospheric current-generated magnetic fields to the ambient field measured at 400 km altitudes by MGS. Further, anti-solar "weathervaning" of the ambient magnetic field is observed more prominently for one set of IMF directions (dawnward upstream IMF).
* Keep in mind that Mars "rocks" back and forth with respect to the Sun over the course of a single year, and therefore the azimuth angle (which is defined relative to the planetary rotation axis) rocks back and forth by as much as 25o as well.
* I use only publicly available MGS data, since those data have been fully calibrated. Therefore, the timeseries will usually be several months "behind" the current date. You can always email me to see whether the page is as up-to-date as possible.
Parameter #1
Name
draping_azimuth_ang
ParameterKey
mgs_drap_ang
Units
deg
Field
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