Space Weather Research in KASI. Yeon-Han Kim & KASI people Space Science Division(SSD) Korea Astronomy and Space Science Institute(KASI)
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1 Space Weather Research in KASI Yeon-Han Kim & KASI people Space Science Division(SSD) Korea Astronomy and Space Science Institute(KASI)
2 I. SSD in KASI Sun-Earth Connection (CME geoeffectiveness) Solar Activity (CME, flare, Type II) Near-Earth Space Env. (Solar wind/magnet./iono.) SDO data center, RBSP antenna NST, KSRBL, VHF Radar etc. Projects Research Solar/Space Weather Group Observations Solar Observation Ionospheric Observation Space Weather Prediction Center Model and Service (Nowcast, Forecast, Alert) Geomagnetic Observation C Korea Astronomy and Space Science Institute. All rights reserved. 2
3 Roadmap for Space Weather Project Phase 1 Phase Infrastructure Construction & Operation System Design Development of Ground & Space Observation System System operation DB & Network Design DB & Network Development Analysis System development Construction of Korean Space Weather Center (14 million$ for 7yrs) Space Weather effects (Satellite, Telecommunication) International Cooperation (NASA, NAOJ, Nagoya U.) Space Weather prediction models (Solar/magnetosphere/Ionosphere) Space Weather Forecast system (Monitoring, Now-Forecasting SW) Center Operation & Preparation of a new space project Space Weather Service System (ARS, Mobile, user-friendly Contents) C Korea Astronomy and Space Science Institute. All rights reserved. 3
4 Science Roadmap Phase 1 Phase 2 Phase CME Kinematics Solar Activity Geoeffective CMEs NST Science High Resolution study of Solar activity SDO Science Magnetosphere Relationship among CME-IP shock-magnetosphere Storm prediction based on CME RBSP Science (Radiation Belt Storm Probe) Ionosphere/ Thermosphere Effects of CME & IP shock on Thermoshphre/Ionosphere Coupling between magnetosphere & Ionosphere * NST(New Solar Telescope) * SDO(Solar Dynamics Observatory) C Korea Astronomy and Space Science Institute. All rights reserved. 4
5 II. Instrument Construction SWML (2007): space weather monitoring <Magnetosphere> Magnetometers: geo-magnetic field v Fluxgate (2007), Proton (2009), MI sensors (2009) <Ionosphere/upper atmosphere> All Sky Imager (2008): ionosphere, optical (97, 250 km) SCINTMON (2008): ionosphere, scintillation VHF Radar (2009): ionosphere E-, F-layer irregularity (will be presented by Dr. Young-Sil Kwak in this afternoon) <Sun> e-callisto (2007): solar radio burst, spectrum KSRBL (2009): solar radio burst, spectrum, source location 1.6m NST: world largest ground-based optical solar telescope (photosphere, chromosphere) v CT (2009), FISS (2010) C Korea Astronomy and Space Science Institute. All rights reserved. 5
6 Instrument Location C Korea Astronomy and Space Science Institute. All rights reserved. 6
7 III. KASI Space Weather Researches CMEs geoeffectiveness v Forecast of geoeffective CMEs v Earthward direction of CMEs Empirical relationship between CMEs initial speed and solarwind dynamic pressure IP shock propagation model High resolution study of solar activities v Small pores, spicule oscillations, solar tornado Satellite drag during strong solar and geomagnetic activities Satellite anomalies due to space weather effect (will be presented by Dr. Jaejin Lee tomorrow) High lat. thermospheric density depending on IMF Auroral observation by STSAT-1 C Korea Astronomy and Space Science Institute. All rights reserved. 7
8 IV. Space Weather Monitoring System (2007~) C Korea Astronomy and Space Science Institute. All rights reserved. 8
9 Contents of SWMS 1. Observational data from oversea and domestic 2. Shock propagation models v Empirical models for shock arrival time 3. Geomagnetic storm forecast v CME initial speed, source location, direction para. -> probability forecast for geomag. storm occurrence 4. Solarwind prediction v Coronal hole information -> solarwind information 5. Space weather monitoring for GEO sat. v Magnetopause monitor, satellite anomaly region, meteor information, etc. 6. Space weather monitoring for polar route flight v Information for high E. ptcls. & communication <- Most contents are based on the solar & space weather researches in KASI C Korea Astronomy and Space Science Institute. All rights reserved. 9
10 Space weather forecast C Korea Astronomy and Space Science Institute. All rights reserved. 10
11 V. Future Plans KASI-NASA collaboration (LOA, 2010) 1. To obtain the real-time space weather data from satellite obs. 2. SDO data center Storage (1.5TB/day) Data analysis server Gloriad (inter-cont. network) Real-time monitoring 3. RBSP receiving station Antenna (7m) Receiver Data server Real-time monitoring C Korea Astronomy and Space Science Institute. All rights reserved. 11
12 C Korea Astronomy and Space Science Institute. All rights reserved. 12
13 Data Centers for SDO UCLan, United Kingdom KDC for SDO KASI, Korea SDO at SIDC ROB, Belgium JSOC (AIA and HMI) Stanford Univ. and LMSAL, USA IAS, France EVE Univ. of Colorado at Boulder, USA GDC for SDO DLR, Germany Full Data Short-term and Selected Data DLR, Deutsches Zentrum für Luft- und RaumfahKDC, Korean Data Center (German Aerospace Center) LMSAL, Lockheed Martin Solar and Astrophysics Lab GDC, German Data Center ROB, Royal Observatory of Belgium IAS, Institut d'astrophysique Spatiale SIDC, Solar Influences Data Center JSOC, Joint Science Operations Center UCLan, University of Central Lancashire C Korea Astronomy and Space Science Institute. All rights reserved. 13
14 GLORIAD 14
15 Korea-Japan Network Korean Network (KOREN, 10 Gbps) Japanese Network (JGN2plus, 10 Gbps) International Network - APII : Asia Pacific Information Infrastructure - GLORIAD : Global Ring Network for Advanced Application Development GLORIAD 10 Gbps KISTI-PNWGP Daejeon KAIST-KASI Busan Chungoku Tokai-Nagoya University APII 10 Gbps Kinki Fukuoka-Kyushu C Korea Astronomy and Space Science Institute. All rights reserved. 15
16 The Radiation Belt Storm Probes (RBSP) NASA will launch two identical probes into the radiation belts to provide unprecedented insight into the physical dynamics of near-earth space. The radiation belts are now part of our technology infrastructure. v If we can understand the belts, we can improve our mission planning, and spacecraft o peration and system design Data collected by the probes will help researchers develop and improve various models for the radiation belts that can be used by: engineers to design radiationhardened spacecraft forecasters to predict space w eather phenomena and alert astronauts and spacecraft op erators to potential hazards spacecraft operators for ano maly resolution 16
17 S-band 7m Antenna assembly in KASI Korean RBSP receiving station started to construct last month and will be completed before June C Korea Astronomy and Space Science Institute. All rights reserved. 17
18 S-band 7m Antenna assembly in KASI RBSP antenna (3 days ago) 18
19 C Korea Astronomy and Space Science Institute. All rights reserved. 19
20 Thank you C Korea Astronomy and Space Science Institute. All rights reserved. 20
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