'Cusp' presentation slideshows

657 views • 59 slides

A High Latitude Source for Radiation Belt Particles?

A High Latitude Source for Radiation Belt Particles?. Robert Sheldon, NSSTC October 19, 2004 Huntsville Modelling Workshop. McIlwain, 1966. Correlations. Highest SW correlation for energetic particles in the radiation belts is: velocity. R=.7-.8 during high-speed streams)

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467 views • 33 slides

443 views • 33 slides

C u r v e

C u r v e. S t i t c h i n g. 2 Parabolas. 4 Parabolas. 8 Parabolas. 8 Parabolas. How many lines?. Sum (1 to 17). (17 x 18)/2 = 153. Cardioid. n ? 2n. Single Cusp. 144. 73. 143. 142. 74. 141. 75. 140. 71. 72. 1. 76. 70. 2. 69. 3. 139. 77. 68. 4. n ? 2n. Cardioid.

493 views • 32 slides

PERMANENT PREMOLARS

1.37k views • 32 slides

Comprehensive Unit-based Safety Program (CUSP)

557 views • 30 slides

Cusp Formation in Galactic Nuclei

Cusp Formation in Galactic Nuclei . Brian Murphy ( Butler University ) Kim Phifer, Brian Geiss, and Michael McFall. A Bit of History. Peebles (1972) : Suggests possible observable light cusp near black hole suggest a non thermal power-law cusp r -9/4 Bachall & Ostriker (1975)

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Theory and simulation predict:

374 views • 28 slides

CLABSI Supplemental Call Series

CLABSI Supplemental Call Series. How CUSP Enables Nurse Empowerment November 15, 2011 at 2ET/1 CT/12 MT/11 PT. Presenters: Pat Posa , RN, BSN, MSA Joanne Timmel , MSN, RN, NE-BC. CLABSI Supplemental Call Series. Pat Posa , RN, BSN, MSA System Performance Improvement Leader

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Presenters: Pat Posa, RN, BSN, MSA Joanne Timmel, MSN, RN, NE-BC

Presenters: Pat Posa, RN, BSN, MSA Joanne Timmel, MSN, RN, NE-BC. CLABSI Supplemental Call Series. How CUSP Enables Nurse Empowerment November 15, 2011 at 2ET/1 CT/12 MT/11 PT. CLABSI Supplemental Call Series. Pat Posa, RN, BSN, MSA System Performance Improvement Leader

316 views • 23 slides

Past cusp researches: (potentially) missing facts

Past cusp researches: (potentially) missing facts. M. Yamauchi. Swedish Institute of Space Physics (IRF), Kiruna. cause of cusp-auroral electron ? ?V // ? 100-500 eV (2) Multiple entry points (3) F ull of escaping ionospheric ions ? mass-loading. (Potentially) missing facts.

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The HST GOALS Survey: Probing the Morphology and Evolution of U/LIRGs

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pp scattering lengths measurement from K e4 and K 3 p decays at CERN SPS experiment NA48/2

pp scattering lengths measurement from K e4 and K 3 p decays at CERN SPS experiment NA48/2. Sergio Giudici University of Pisa and INFN On behalf of the NA48/2 collaboration :

295 views • 19 slides

Pulsed Flows Along a Cusp Structure Observed with SDO/AIA

288 views • 19 slides

Daytime Aurora

244 views • 11 slides

Course & Unit of Study Portal (CUSP)

216 views • 10 slides

Course & Unit of Study Portal (CUSP)

239 views • 10 slides

Investigating the Cusp at Multiple Altitudes

Investigating the Cusp at Multiple Altitudes. by W. Keith 1 , M. Goldstein 1 , D. Winningham 2 , M. Wilber 3 , A. Fazakerley 4 , H. Reme 5 , T. Fritz 6 , A. Balogh 7 and N. Cornilleau-Wehrlin 8. 1 NASA Goddard Space Flight Center, Code 692, Greenbelt, MD 20771, USA

180 views • 9 slides

1 F. Dahlgren, 1 T. Dodson, 1 T. Kozub, 1 C. Priniski, 1 C. Gentile, 2 J. Sethian,

123 views • 1 slides