The interplanetary shock propagation model : a model for predicting solar-flare-caused geomagnetic storms, based on the 2 1/2 D, MHD numerical simulation results from the interplanetary global model (2D IGM) /

The interplanetary shock propagation model : a model for predicting solar-flare-caused geomagnetic storms, based on the 2 1/2 D, MHD numerical simulation results from the interplanetary global model (2D IGM) /

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Bibliographic Details
Author / Creator:	Smith, Zdenka K.
Imprint:	Boulder, Colo. : National Oceanic and Atmospheric Administration, Environmental Research Laboratories, Space Environment Laboratory ; Springfield, VA : For sale by the National Technical Information Service, [1995]
Description:	iv, 56 p. : ill. ; 28 cm.
Language:	English
Series:	NOAA technical memorandum ERL SEL 89
Subject:	Shock waves -- Mathematical models. Solar flares. Magnetic storms -- Forecasting. Magnetohydrodynamics -- Simulation methods. Magnetic storms -- Forecasting. Shock waves -- Mathematical models. Solar flares.
Format:	Microform U.S. Federal Government Document Book
URL for this record:	http://pi.lib.uchicago.edu/1001/cat/bib/3246575

Hidden Bibliographic Details
Other authors / contributors:	Dryer, Murray. Space Environment Laboratory.
Notes:	Distributed to depository libraries in microfiche. Shipping list no.: 95-0764-M. "July 1995." Includes bibliographical references (p. 44-47). Microfiche. [Washington, D.C.?] : Supt. of Docs., U.S. G.P.O., [1995] 1 microfiche : negative.
GPO item no.:	0208-C-02 (MF)
Govt.docs classification:	C 55.13/2:ERL SEL-89

Regenstein, B Level, Science Microforms

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Holdings details from Regenstein, B Level, Science Microforms
Call Number:	microfc QC168.85.S45S55 1995
c.1	Available Loan period: standard loan Need help? - Ask a Librarian