%0 Journal Article %@holdercode {isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S} %@nexthigherunit 8JMKD3MGPCW/3EU29DP %@archivingpolicy denypublisher denyfinaldraft24 %@issn 1364-6826 %@usergroup administrator %3 science.pdf %@dissemination WEBSCI; PORTALCAPES; AGU; MGA; COMPENDEX. %X Slow (VSW<400 km s-1) magnetic clouds have been analyzed to determine their characteristics and geoeffectiveness. It is found that slow clouds have mean magnetic field strengths of ~13 nT, peak BS~9 nT, and dawn–dusk electric fields of ESW~2.5 mV m-1. The clouds are small in spatial size, typically ~0.18 AU. The slowest events may have been accelerated to their speeds by interaction with the slow solar wind. Slow clouds are surprisingly geoeffective. Five out of 27 events caused major (DST-100 nT) magnetic storms. Likewise, these geoeffective clouds may have been decelerated to VSW<400 km s-1. The issue of interplanetary acceleration/deceleration will be examined with SOHO coronal mass ejection data in the near future. Author Keywords: Slow (VSW<400 km s-1) magnetic clouds have been analyzed to determine their characteristics and geoeffectiveness. It is found that slow clouds have mean magnetic field strengths of ~13 nT, peak BS~9 nT, and dawn–dusk electric fields of ESW~2.5 mV m-1. The clouds are small in spatial size, typically ~0.18 AU. The slowest events may have been accelerated to their speeds by interaction with the slow solar wind. Slow clouds are surprisingly geoeffective. Five out of 27 events caused major (DST-100 nT) magnetic storms. Likewise, these geoeffective clouds may have been decelerated to VSW<400 km s-1. The issue of interplanetary acceleration/deceleration will be examined with SOHO coronal mass ejection data in the near future. %8 Jan. %N 2 %T Properties of slow magnetic clouds %K Slow magnetic clouds, Geoeffectiveness, Interplanetary magnetic fields. %@secondarytype PRE PI %@group DGE-INPE-MCT-BR %@copyholder SID/SCD %@secondarykey INPE-10797-PRE/6253 %2 sid.inpe.br/marciana/2004/01.22.13.15.15 %@affiliation Jet Propulsion Laboratory, California Institute of Technology, MS 169-506, 4800 Oak Grove Drive, %@affiliation Pasadena, CA 91109, USA, %@affiliation Instituto Nacional de Pesquisas Espaciais, Sao Jose dos Campos, 12201-970, Sao Paulo, Brazil, %@affiliation Goddard Space Flight Center, Greenbelt, MD 20771, USA, %@affiliation Max-Planck-Institut für Aeronomie, Katlenburg-Lindau, D-37191, Germany, %B Journal of Atmospheric and Solar-Terrestrial Physics %@language English %P 147-151 %4 sid.inpe.br/marciana/2004/01.22.13.15 %D 2004 %V 66 %A Tsurutani, Bruce T., %A González-Alarcon, Walter Demétrio, %A Zhoua, Xian. Yan, %A Leppingc, R. P., %A Bothmerd, V., %@area CEA