Solar storm detecting by integrated magnetometer based on anisotropic magnetoresistivity
Identifikátory výsledku
Kód výsledku v IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F49777513%3A23220%2F17%3A43950741" target="_blank" >RIV/49777513:23220/17:43950741 - isvavai.cz</a>
Výsledek na webu
<a href="http://ieeexplore.ieee.org/document/8249414/" target="_blank" >http://ieeexplore.ieee.org/document/8249414/</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1109/TELFOR.2017.8249414" target="_blank" >10.1109/TELFOR.2017.8249414</a>
Alternativní jazyky
Jazyk výsledku
angličtina
Název v původním jazyce
Solar storm detecting by integrated magnetometer based on anisotropic magnetoresistivity
Popis výsledku v původním jazyce
This paper deals with the geomagnetic field measurement by integrated sensor based on principle of anisotropic magnetoresistivity (AMR). The geomagnetic field measurements require very precise instrumentation which is mostly spacious. On the other hand, the chosen magnetometer - HMC5883L - is very tiny but suffers from lower resolution and high noise floor. The objective is to examine possibility of geomagnetism investigation made by an integrated widespread magnetometer, to evaluate its precision and to detect some outer space events by geomagnetism observations. There was proposed and constructed measuring device including AMR chip. The measuring device including the AMR chip was proposed and produced. A long-term measurement was recorded in collaboration with the geomagnetic observatory Budkov, Czech Republic (Institute of Geophysics of the CAS, v. v. i.; INTERMAGNET). The post-processing was designed in order to suppress sensor noise and temp-drift. The post-processing used was standardized by INTERMAGNET especially for geomagnetic observatories. Finally, with the constructed device there were detected the day-night variations of the Earth magnetic field and a solar storm of 4th grade of k-index.
Název v anglickém jazyce
Solar storm detecting by integrated magnetometer based on anisotropic magnetoresistivity
Popis výsledku anglicky
This paper deals with the geomagnetic field measurement by integrated sensor based on principle of anisotropic magnetoresistivity (AMR). The geomagnetic field measurements require very precise instrumentation which is mostly spacious. On the other hand, the chosen magnetometer - HMC5883L - is very tiny but suffers from lower resolution and high noise floor. The objective is to examine possibility of geomagnetism investigation made by an integrated widespread magnetometer, to evaluate its precision and to detect some outer space events by geomagnetism observations. There was proposed and constructed measuring device including AMR chip. The measuring device including the AMR chip was proposed and produced. A long-term measurement was recorded in collaboration with the geomagnetic observatory Budkov, Czech Republic (Institute of Geophysics of the CAS, v. v. i.; INTERMAGNET). The post-processing was designed in order to suppress sensor noise and temp-drift. The post-processing used was standardized by INTERMAGNET especially for geomagnetic observatories. Finally, with the constructed device there were detected the day-night variations of the Earth magnetic field and a solar storm of 4th grade of k-index.
Klasifikace
Druh
D - Stať ve sborníku
CEP obor
—
OECD FORD obor
20201 - Electrical and electronic engineering
Návaznosti výsledku
Projekt
—
Návaznosti
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Ostatní
Rok uplatnění
2017
Kód důvěrnosti údajů
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Údaje specifické pro druh výsledku
Název statě ve sborníku
2017 25th Telecommunications Forum (TELFOR) : Proceedings of Papers
ISBN
978-1-5386-3073-0
ISSN
—
e-ISSN
neuvedeno
Počet stran výsledku
4
Strana od-do
585-588
Název nakladatele
IEEE
Místo vydání
Piscataway
Místo konání akce
Belgrade, Serbia
Datum konání akce
21. 11. 2017
Typ akce podle státní příslušnosti
WRD - Celosvětová akce
Kód UT WoS článku
—