首页 | 本学科首页   官方微博 | 高级检索  
     检索      


The NOAA Real-Time Solar-Wind (RTSW) System using ACE Data
Authors:Zwickl  RD  Doggett  KA  Sahm  S  Barrett  WP  Grubb  RN  Detman  TR  Raben  VJ  Smith  CW  Riley  P  Gold  RE  Mewaldt  RA  Maruyama  T
Institution:(1) Space Environment Center, NOAA, Boulder, Colorado, 80303, U.S.A.;(2) Bartol Research Institute, University of Delaware, Newark, Delaware, 19716, U.S.A.;(3) Applied Physics Laboratory, Johns Hopkins University, Laurel, Maryland, 20707, U.S.A.;(4) California Institute of Technology, Pasadena, California, 91125, U.S.A.;(5) Communications Research Laboratory, Tokyo 184, Japan
Abstract:The Advanced Composition Explorer (ACE) RTSW system is continuously monitoring the solar wind and produces warnings of impending major geomagnetic activity, up to one hour in advance. Warnings and alerts issued by NOAA allow those with systems sensitive to such activity to take preventative action. The RTSW system gathers solar wind and energetic particle data at high time resolution from four ACE instruments (MAG, SWEPAM, EPAM, and SIS), packs the data into a low-rate bit stream, and broadcasts the data continuously. NASA sends real-time data to NOAA each day when downloading science data. With a combination of dedicated ground stations (CRL in Japan and RAL in Great Britain), and time on existing ground tracking networks (NASA's DSN and the USAF's AFSCN), the RTSW system can receive data 24 hours per day throughout the year. The raw data are immediately sent from the ground station to the Space Environment Center in Boulder, Colorado, processed, and then delivered to its Space Weather Operations center where they are used in daily operations; the data are also delivered to the CRL Regional Warning Center at Hiraiso, Japan, to the USAF 55th Space Weather Squadron, and placed on the World Wide Web. The data are downloaded, processed and dispersed within 5 min from the time they leave ACE. The RTSW system also uses the low-energy energetic particles to warn of approaching interplanetary shocks, and to help monitor the flux of high-energy particles that can produce radiation damage in satellite systems. This revised version was published online in June 2006 with corrections to the Cover Date.
Keywords:
本文献已被 SpringerLink 等数据库收录!
设为首页 | 免责声明 | 关于勤云 | 加入收藏

Copyright©北京勤云科技发展有限公司  京ICP备09084417号