Response of the Upper/Middle Atmosphere to Coronal Holes and Powerful High-Speed Solar Wind Streams in 2003

Recurrent Magnetic Storms: Corotating Solar Wind Streams

Volumn , Issue , 2013, Pages 319-340

  Kozyra, J U ^a   Crowley, G ^b   Emery, B A ^c   Fang, X ^a   Maris, G ^d   Mlynczak, M G ^e   Niciejewski, R J ^a   Palo, S E ^f   Paxton, L J ^g   Randall, C E ^f   Rong, P P ^h   Russell, J M ^h   Skinner, W ^a   Solomon, S C ^c   Talaat, E R ^g   Wu, Q ^c   Yee, J H ^g  

^a UNIVERSITY OF MICHIGAN   (United States)

^b SOUTHWEST RESEARCH INSTITUTE   (United States)

^c NATIONAL CENTER FOR ATMOSPHERIC RESEARCH   (United States)

^d ACADEMY OF ROMANIAN SCIENTISTS   (Romania)

^e NASA LANGLEY RESEARCH CENTER   (United States)

^f UNIVERSITY OF COLORADO   (United States)

^g JOHNS HOPKINS UNIVERSITY APPLIED PHYSICS LABORATORY   (United States)

^h HAMPTON UNIVERSITY   (United States)

Author keywords

Atmosphere, Upper; Corotating interaction regions; Magnetic storms; Magnetosphere

Indexed keywords

GEOMAGNETISM; IONOSPHERE; MAGNETOSPHERE; NITRIC OXIDE; ORBITS; OZONE LAYER; REFUSE INCINERATORS; SOLAR ENERGY; SOLAR WIND;

COROTATING INTERACTION REGIONS; HIGH-SPEED SOLAR WIND STREAMS; MAGNETIC STORMS; METEOROLOGICAL CONDITION; STRATOSPHERIC OZONE; STRATOSPHERIC VARIABILITY; SYSTEMATIC CHANGES; TOTAL ELECTRON CONTENT;

SPEED;

EID: 84952775206     PISSN: None     EISSN: None     Source Type: Book    
DOI: 10.1029/167GM24     Document Type: Chapter

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