DIM_sets
Description
The files are the records of DIM (Declination and Inclination Magnetometer) during re-occupation of two repeat stations near the Adriatic see in 2010. In the HUN_RS directory the files are also DIM records from the Hungarian RS network measurement campaign in 2010. The calculated offset values of the equipped DI fluxgate device is a function of the geomagnetic gradient measured in the horizontal plane. See the referred paper for the details. The description of the data: The name of the file: AB (absolute measurement), date (yy,mm,dd) The extension: sim belongs to Sinsko Polje station morning sets, sie the same station evening sets. krm belongs to KRBavsko Polje station morning sets, kre is the same station evening sets. The extensions in HUN_RS directory have no additional meanings. Header: Name_of_the_station extension Instrument Date Name_of_the_Observer1 Name_of_the_Observer2 Data: The direction of azimuth mark (xxx° yy.yy') delta F (nT) MIRA1 (xxx° yy.yy') MIRA2 (xxx° yy.yy') East Up (xxx° yy.yy') Time (UTC) (hh mm) West Up (xxx° yy.yy') Time (UTC) (hh mm) East Down (xxx° yy.yy') Time (UTC) (hh mm) West Down (xxx° yy.yy') Time (UTC) (hh mm) Nord Up (xxx° yy.yy') Time (UTC) (hh mm) Total field (nT) South Down (xxx° yy.yy') Time (UTC) (hh mm) Total field (nT) Nord Down (xxx° yy.yy') Time (UTC) (hh mm) Total field (nT) South Up (xxx° yy.yy') Time (UTC) (hh mm) Total field (nT) MIRA1 (xxx° yy.yy') MIRA2 (xxx° yy.yy') etc...
Files
Steps to reproduce
The geomagnetic records are generally not reproducible because the results of every magnetic readings are the superposition of the influences of different fluctuating phenomena. In this situation the accuracy of the measurement (i.e., absolute measurements) the only way to reach the expected quality of the observation. Different solutions were developed to use the proper geomagnetic conditions for the computation of the spatial difference between the repeat station and the reference geomagnetic observatory. Use the recommendation of IAGA (International Association of Geomagnetism and Aeronomy) for the successful observation!