13,675 research outputs found
Correspondence to Mary Ann Smith From William H. Borders and C.M. Lowe, March 22, 1961
No full textCorrespondence from William H. Borders and C.M. Lowe to Mary Ann Smith notifying her of a meeting for the Atlanta Student Adult Liaison. 1 page
Map of Isanti County : with adjacent portions of Chisago, Anoka, Sherburne, and Mille Lacs counties, Minnesota.
No full textCadastral map showing drainage, section lines and numbers, land ownership, landowners' names, roads, railroads, etc."C.M. Foote Publishing Co.--E.J. Foote, Geo. F. Weston, Minneapolis, Minn."Label on recto: J.L. Smith Map Publisher ... Philada."Indexed.LC Land ownership maps, 37
C.M. Smith to John Philip Trinkaus, 1972
No full textLetter asking Trinkaus to provide a reference for Cheryll Tickle; with information about the Medical Research Council attached.Typed letter5-pagesCorrespondenc
A note containing land boundaries by Walding Smith and C.M Waddin
No full textA note containing land boundaries by Walding Smith and C.M Waddin.https://mavmatrix.uta.edu/specialcollections_mckinneymilamfamily/1735/thumbnail.jp
Hirt
No full textWhen in the wood, Far far from thee, Thine image fair Followeth meEnglish words by C.M. Smith. Lyrics in English, German and Swedish. "Entered according to act of Congress, in the year 1874, by Lous Meyer, in the office of the Librarian of Congress, at Wash'n.
Cortical sensory processing in experimental and clinical models of persistent pain. EEG studies in healthy volunteers and patients
No full textContains fulltext :
110719.pdf (Publisher’s version ) (Open Access)Radboud Universiteit Nijmegen, 16 mei 2012Promotores : Vissers, K.C.P., Scheffer, G.J. Co-promotores : Wilder-Smith, O.H.G., Rijn, C.M. van161 p
Dr. Charles Merrill Smith
No full textPortrait of Dr. C.M. Smith, who was the first resident doctor, arriving in 1905. Dr. Smith's sister Minnie Smith was the first permanently appointed teacher
Magnetic reconnection in Saturn's magnetotail: a comprehensive magnetic field survey
No full textReconnection within planetary magnetotails is responsible for locally energizing particles and changing the magnetic topology. Its role in terms of global magnetospheric dynamics can involve changing the mass and flux content of the magnetosphere. We have identified reconnection related events in spacecraft magnetometer data recorded during Cassini's exploration of Saturn's magnetotail. The events are identified from deflections in the north-south component of the magnetic field, significant above a background level. Data were selected to provide full tail coverage, encompassing the dawn and dusk flanks as well as the deepest midnight orbits. Overall 2094 reconnection related events were identified, with an average rate of 5.0 events per day. The majority of events occur in clusters (within 3 h of other events). We examine changes in this rate in terms of local time and latitude coverage, taking seasonal effects into account. The observed reconnection rate peaks postmidnight with more infrequent but steady loss seen on the dusk flank. We estimate the mass loss from the event catalog and find it to be insufficient to balance the input from the moon Enceladus. Several reasons for this discrepancy are discussed. The reconnection X line location appears to be highly variable, though a statistical separation between events tailward and planetward of the X line is observed at a radial distance of between 20 and 30RS downtail. The small sample size at dawn prevents comprehensive statistical comparison with the dusk flank observations in terms of flux closure
Smith, William (Birth, 1884-04-22)
No full text1828/Pg 192/1884/M W/U.S./U.S./C.M. Sparks,M.D.Original record filed in drawer labeled 'SMITH-SNYDE'
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