Recent results from Odessa Observatory

Slides:



Advertisements
Similar presentations
DMI Development and World-wide Sale of Precision Magnetic Instruments High-Precision Magnetometers Measurement of the vertical geomagnetic component (middle)
Advertisements

Geomagnetic Measurements Workshop: DIflux: Absolute Measurement of the Geomagnetic Field orientation in Space prepared for the XIVth IAGA WORKSHOP ON.
Plasmapause detection by means of a meridional magnetometer array Balázs HEILIG, GGIH, Tihany, Hungary Massimo VELLANTE, University Of L'Aquila, L'Aquila,
THE AURORAL EMISSIONS AND THE ELECTRON PRECIPITATION UNDER DIFFERENT GEOMAGNETIC CONDITIONS DURING RECURRENT SOLAR WIND STREAM Guineva V. 1, Despirak I.
Vr: A New Index to Represent the Regional Geomagnetic Activity Dongmei Yang, Yufei He, Chuanhua Chen, Yahong Yuan Changchun.
Abnormal Analysis of Averaged Midnight F before the Ms 5.1 Chuxiong Earthquake Rong Zhu 1, Dong-mei Yang 1, Yan Zhang 2, Jian-jun Wang 3, Yu-fei He 1 1.
Repeat station crustal biases and accuracy determined from regional field models M. Korte, E. Thébault* and M. Mandea, GeoForschungsZentrum Potsdam (*now.
WANG Jianjun 1, YANG Dongmei 2 , ZHANG Suqing 2 , ZHU Rong 2 1 Earthquake Administration of Gansu Province, China, 2 Institute of Geophysics,
Separating internal geomagnetic secular variation and long-term magnetospheric field variations Monika Korte Deutsches GeoForschungsZentrum GFZ.
Swedish Institute of Space Physics, Kiruna Variable Sun-Earth energy coupling: dependence on solar cycle strength M. Yamauchi
Marine Branch of Ukrainian Hydrometeorological Institute Marine Branch of Ukrainian Hydrometeorological Institute Soviet Street, , Sevastopol,
OBSERVATIONS OF SEASONAL PLUMB LINE VARIATIONS OBTAINED WITH HELP OF THE LONG WATER-TUBE TILTMETER, IN PERIOD 2004 TO 2006 Marek Kaczorowski Space Research.
Introduction The primary geomagnetic storm indicator is the Dst index. This index has a well established ‘recipe’ by which ground-based observations are.
An Automatic Instrument to Measure the Absolute Components of the Earth's Magnetic Field H.-U. Auster, M. Mandea, A. Hemshorn, E. Pulz, M. Korte.
Polish strategy for science in Ukraine and European perspectives REPRESENTATIVE OFFICE OF POLISH ACADEMY OF SCIENCES IN KIEV GEORGES CHARPAK - 90TH ANNIVERSARY.
12th EMS Annual Meeting & 9th European Conference on Applied Climatology (ECAC), Łódź, September 2012 Rajmund Przybylak, Aleksandra Pospieszyńska.
Equipping of Eilat observatory by DIDD magnetometer. Installation features and preliminary results. B. Ginzburg, Nuclear Research Center SOREQ, 81800,
A Verification of Magnetometer’s Time Accuracy by using a GPS Pulse Generator Some magnetic observatories are exchanging one-minute geomagnetic field data.
PILOT PROJECT: External audit of quality assurance system on HEIs Agency for Science and Higher Education Zagreb, October 2007.
Magnetic Observatories Jeffrey J. Love Carol A. Finn Jennifer L. Gannon Geomagnetism Program GeoHazards Science Center geomag.usgs.gov.
High Sensitivity Magnetic Gradiometer for Earthquake Research Applications ISRAEL 2005 Ivan Hrvoic H. Ginzburg, H. Zafrir, G. Steinitz, B. Shirman, G.
Management & Technology Consultants A Good Practice Framework to Reinforce the Exchange of Good Practice in eGovernment IST4Balt WORKSHOP June.
Integration Development Programme in the Field of Statistics of the Eurasian Economic Union for EEC THE EURASIAN ECONOMIC COMMISSION.
Croatian Report on new Environmental Protection Law Josipa Blažević-Perušić, B.Sc. Arch. State Secretary Anita Pokrovac-Patekar, B.Sc. Pharm. Senior Environmental.
The Tiksi Hydrometeorological Observatory Program International Collaboration for Climate Studies U.S. Science Contact:
NEW VECTOR MAGNETOMETER IN OBSERVATORY PRACTICE L. Hegymegi, 1 J. Szöllősy, 2 L. Merényi, 3 L. Szabados 3 1 MinGeo – 2 Araconsys – 3 Eötvös L. Geophysical.
International Conference on Climate Change Impact of Sea Level Rise on storm surge in Hong Kong and the Pearl River Delta by WONG, Agnes K.M. LAU, Alexis.
5 th European Space Weather Week, November 2008, Brussels Operational implementation of the SWIF model in DIAS system Tsagouri Ioanna Koutroumbas.
Dariusz Pęchorzewski, PhD Szczecin Renovation Centre Ltd. Institute of Economic Analyses, Diagnoses and Forecasts The impact of the global financial crisis.
Secular variation in Germany from repeat station data and a recent global field model Monika Korte and Vincent Lesur Helmholtz Centre Potsdam, German Research.
XVI th IAGA Workshop – 15 October 2014 XVI th IAGA Workshop on Geomagnetic Observatories, Data Acquisition and Processing October 2014 Hyderabad.
Anomalous Geomagnetic Variations Possibly Linked with the Taiwan Earthquake Mw= 6.4, 19 December 2009 Takla E. M 1 ; K. Yumoto 1, 2 ; J. Y. Liu 3 ; Y.
© NERC All rights reserved UK Repeat Station Report T J G Shanahan and S Macmillan June 2009 MagNetE Workshop Helsinki, Finland.
PERFORMANCE MONITORING OF A NEW INSTALLATION AT APIA OBSERVATORY A.Jackson, A.Beraducci, T.Tafua.
BEST METROPOLISES Best development conditions in European metropolises: Paris, Berlin and Warsaw Transport, job accessibility and daily mobility Piotr.
Time-Series Forecasting Overview Moving Averages Exponential Smoothing Seasonality.
© NERC All rights reserved Chris Turbitt Observatories Manager Geomagnetism Team British Geological Survey BGS Observatory Network.
GP33A-06 / Fall AGU Meeting, San Francisco, December 2004 Magnetic signals generated by the ocean circulation and their variability. Manoj,
CEGRN 2015 Campaign A. Caporali (1), J. Zurutuza (1), O. Khoda (2), G. Stangl (3), M. Becker (4), M. Bertocco (1), L. Gerhatova (5), M. Mojzes (5), M.
Some remarks to the derivation of mean hourly values with incomplete data Pavel Hejda Institute of Geophysics of the ASCR, Prague, Czech Republic.
N. Petrov, P. Duchlev, K. Koleva, M. Dechev Institute of Astronomy and National Astronomical Observatory ROZHEN, BAS 72 Tsarigradsko Chaussee, Sofia 1784,
Wavelet Based Estimation of the Hurst Exponent for the Horizontal Geomagnetic Field at MAGDAS Equatorial Stations G. Gopir1,2,*, N. S. A. Hamid1,2, N.
IAGA Symposium A12.2 Geomagnetic networks, computation and definition of products for space weather and space climate Melbourne, Australia, 2011 GLOBAL,
OMI validation by ground-based remote sensing: ozone columns and atmospheric profiles A. Shavrina,Ya. Pavlenko, A. Veles, I. Synyavsky, M. Sosonkin, Ya.
Don Chambers Center for Space Research, The University of Texas at Austin Josh Willis Jet Propulsion Laboratory, California Institute of Technology R.
GETG meeting Brussels, BE, November 2007 Status of GE-relevant activities at DMI Jurgen Watermann, Danish Meteorological Institute (DMI)
A.A. Soloviev, Sh.R. Bogoutdinov, S.M. Agayan, A.D. Gvishiani (GC RAS, Russia), A. Chulliat (IPGP, France) Automated recognition of spikes on 1-minute.
Geomagnetic Charts of Southern Part of Korean Peninsula as of LIM, Mutaek* 1, MOON, Jiyoung 2, PARK, Youngsue 1, SHIN, Younghong 1, RIM, Hyoungrae.
AUTOMATED QUALITY CONTROL OF GEOPHYSICAL TIME SERIES The algorithmic systems developed at Geophysical Center of Russian Academy of Sciences are intended.
Felt earthquake in the Little Carpathians Mts. source zone (March 5th, 2012) and related seismic activity in the area AIM third annual meeting October.
NATIONAL INSTITUTE OF GEOPHYSICS, GEODESY AND GEOGRAPHY BULGARIAN ACADEMY OF SCIENCES
MAGNETOMETERS IN HYPACK® Data Collection & Data Processing.
Preliminary Results of Total Field Magnetometer Comparison Introduction During the XIVth IAGA Workshop (hereafter referred to as “the workshop”), several.
GEM Challenge: ground magnetic field perturbations Pulkkinen, A., L. Rastätter, M. Kuznetsova and A. Chulaki Summer GEM, June 21-26, 2009, Snowmass, CO.
Incorporation of geomagnetic data and services into EPOS infrastructure Pavel Hejda 1, Aude Chambodut 2, Juan-Jose Curto 3, Simon Flower 4, Elena Kozlovskaya.
SOUTHERN REGIONAL SPACE RESEARCH CENTER – CRS/INPE-MCT SPACE SCIENCE LABORATORY OF SANTA MARIA – LACESM/CT-UFSM LOW COST FLUXGATE MAGNETOMETER DEVELOPMENT.
Synthetic benchmark datasets for homogenization of IWV time series
Institute of Meteorology Alfred Dubicki, Assist. Prof. Dr
Rapid core field variations just before Swarm
M.J. Rivas [1,2], C. Cid [1] RELATIONSHIP BETWEEN THE INTENSITY OF X-RAY FLARES AND THEIR EFFECTS IN THE HORIZONTAL COMPONENT OF THE.
An advantage of magnetic index h to show high local disturbances in ionosphere during quiet day conditions Beata Dziak-Jankowska1, Iwona Stanisławska1,
Recent progress of WDC for Geophysics, Beijing
Variable Sun-Earth energy coupling: dependence on solar cycle strength
MAGNETOMETERS IN HYPACK® Data Collection & Data Processing.
Medium-term Precipitation Projections with Neural Networks
DI3 – A new Procedure for Absolute Directional Measurements
P Kotzé (1), M Korte (2), M Mandea (2,3)
New Magnetic Observatory Installation
European Plate Observing System
REPEAT STATIONS MEASUREMENTS IN UKRAINE IN 2006
Presentation transcript:

Recent results from Odessa Observatory Yuri Sumaruk , Vitaly Starostenko Institute of Geophysics, National Academy of Sciences of Ukraine, Kiev, Ukraine

Historical events I 1859-1875 Inclination and horizontal component were measured near Odessa and along the Black Sea by Dikov. 1880-1886 Magnetic observations along the coast of the Black Sea were performed under the leadership of Baron Maidel. 1890-1891 Isocline map of Odessa anomaly was published by Prof. Popruzhenko

Historical events II In 1894 the Odessa meteorological observatory began regular magnetic observations. The magnetic pavilions on the Maloy Fontane had been built by Prof. Klossovsky 1924 - Geophysical observatory “Odessa” 1931 – The observatory was transferred by 60 km from Odessa to Stepanovka. 3

Historical events III Since 1948 regular observations of the geomagnetic field components have been made at the observatory with La Cour magnetometers. In the 1970s Bobrov magnetometers were installed. 4

Geomagnetic observatory Odessa Fluxgate magnetometer LEMI-018M 5

Geomagnetic observatory Odessa Torsion photoelectric magnetometer 6

Intermagnet meeting, Paris, October 2010

Absolute and variation pavilions

Process of determining adopted baselines 1) Manual review , removal of abnormal observations 2) Preliminary automatic calculation of adopted baseline using moving average technique 3) Possible manual adjustment of automatic calculations after visual inspecting

Conclusions The geomagnetic observatory Odessa has a long series of data reaching back to 1948. It is valuable for studying long-period and secular variations. The level of artificial noise at the observatory is very low. Modern equipment has been installed at the observatory Odessa. Since the end of 2013 data from observatory Odessa have been sent to Edinburg in IAGA2002 format. The Application form, 12 month of definitive one-minute mean data , a baseline file, an annual mean file, and a readme file in INTERMAGNET formats have been prepared and submitted. We hope that geomagnetic observatory Odessa will be accepted as full member of INTERMAGNET. 14

Acknowledgments We express thanks to Colleagues from Deutsches GeoForschungs Zentrum, Potsdam, Germany and from Institute of Geophysics, Polish Academy of Sciences, Warsaw, Poland for help in equipping the observatory “Odessa” of Institute of geophysics of NASU with instruments meeting INTERMAGNET standards. Staff of the geomagnetic observatory “Niemegk” for help in installing the equipment. Dr. Hans-Joachim Linthe for consultations and help to prepare application form. Dr. Jan Reda and Mariusz Neska from IG PAS for help to prepare data from observatory “Odessa” according to INTERMAGNET standards.

Thank You for Your Attention!