'Solar wind speed' diaporamas de présentation

P.K. Manoharan Radio Astronomy Centre National Centre for Radio Astrophysics

THE SOLAR WIND. THE SOLAR WIND. P.K. Manoharan Radio Astronomy Centre National Centre for Radio Astrophysics Tata Institute of Fundamental Research Ooty 643001, India mano@ncra.tifr.res.in. P.K. Manoharan Radio Astronomy Centre National Centre for Radio Astrophysics

1.13k views • 90 slides

Review of CIR-related Particle Composition, Charge States, & Energy Spectra

Review of CIR-related Particle Composition, Charge States, & Energy Spectra. Joe Mazur The Aerospace Corporation Glenn Mason Johns Hopkins/APL Joe Dwyer Florida Institute of Technology Mihir Desai Southwest Research Institute. Processes for 1 AU observations of solar material.

604 views • 51 slides

What Geomagnetism can Tell Us about the Solar Cycle?

What Geomagnetism can Tell Us about the Solar Cycle?. Leif Svalgaard HEPL, Stanford University Bern, 11 Nov., 2013 ISSI Workshop: The Solar Activity Cycle: Physical Causes and Consequences.

577 views • 35 slides

Solar Drivers of Space Weather

Solar Drivers of Space Weather. Steven Hill NOAA/SEC June 14, 2007. Research Experience for Undergraduates. Energy and Power in Context. Outline. Overview of the Sun Interior Surface Corona Solar Drivers of Space Weather Coronal Holes Flares Coronal Mass Ejections (CMEs) Summary.

425 views • 32 slides

WSA Model and Forecasts

WSA Model and Forecasts. Nick Arge Space Vehicles Directorate Air Force Research Laboratory. WSA Coronal & Solar Wind Model. Schatten Current Sheet Model. PFSS Model. Solar Wind Model (e.g., 1D Kinematic model, ENLIL, HAF) (5-30 Rs to 1AU). 5-30 Rs. 2.5 Rs. Source Surface.

516 views • 27 slides

Axel Korth 1 , Ezequiel Echer 2 , Fernando L. Guarnieri 3 , Q.-G. Zong 4

358 views • 26 slides

He/H variation in the solar wind over the solar cycle

He/H variation in the solar wind over the solar cycle. Justin C Kasper Smithsonian Astrophysical Observatory. NESSC ( CfA ) 27 October 2008. Who is involved. Kasper (SAO) Bennett Maruca ( Harvard University), new analysis of Wind Faraday Cup data

372 views • 23 slides

290 views • 22 slides

??????

??????. ??????????? ????????????? ??????????????. How do Magnetic Storms Form?.

351 views • 22 slides

One year's experience with a recreation-grade GPS receiver

One year's experience with a recreation-grade GPS receiver. Pete Bettinger Warnell School of Forestry and Natural Resources University of Georgia Athens, GA Songlin Fei Department of Forestry University of Kentucky Lexington, KY. 7th Southern Forestry and Natural Resources GIS Conference.

331 views • 20 slides

Forecast of Geomagnetic Storm based on CME and IP condition

IHY WB 2-3 Sep. 23, 2009. Forecast of Geomagnetic Storm based on CME and IP condition. R.-S. Kim 1 , K.-S. Cho 2 , Y.-J. Moon 3 , Yu Yi 1 , K.-H. Kim 3 1 Chungnam National University 2 Korea Astronomy and Space Science Institute 3 Kyunghee University. Geomagnetic storm.

429 views • 19 slides

North-South Asymmetry in the Solar Wind During Recent and Past Solar Cycles

North-South Asymmetry in the Solar Wind During Recent and Past Solar Cycles. Bertalan Zieger Center for Space Physics, Boston University. Questions. Is the solar wind distribution symmetric to the solar equator? What causes the asymmetry?

324 views • 19 slides

Long Term Measurements of Solar Wind Fe Charge States: Charge State Distributions

Long Term Measurements of Solar Wind Fe Charge States: Charge State Distributions. Mark Popecki , A. Galvin, L. M. Kistler,H. Kucharek, E. Moebius, K. Simunac, P. Bochsler, L. M. Blush, B. Klecker. slow. fast. Von Steiger et al., (2000). Solar Wind Fe Charge State Expectations.

349 views • 18 slides

The IceTop Air Shower Array:

339 views • 17 slides

Antiprotons of interstellar origin at balloon altitudes: Flux simulations

Antiprotons of interstellar origin at balloon altitudes: Flux simulations. U. B. Jayanthi , K. C. Talavera Instituto Nacional de Pesquisas Espaciais (INPE), Brasil. A. A. Gusev Space Research Institute (IKIRAS), Moscow , Russia.

204 views • 13 slides

SCINTILLATION MONITORING RESULTS DURING THE 30 OCTOBER 2003 SPACE WEATHER EVENT

SCINTILLATION MONITORING RESULTS DURING THE 30 OCTOBER 2003 SPACE WEATHER EVENT. Marcio Aquino, Alan Dodson Institute of Engineering Surveying and Space Geodesy (IESSG), University of Nottingham, Nottingham, UK Lucilla Alfonsi, Giorgiana De Franceschi, Vincenzo Romano

297 views • 12 slides

Session A Wrap Up

Session A Wrap Up. He Abundance J. Kasper. Helium abundance variation over the solar cycle, latitude and with solar wind speed Slow solar wind appears to be depleted in helium Less speed ordering at solar maximum 6 month periodicity with heliographic latitude

292 views • 10 slides

Background

176 views • 10 slides

Ulyssess

Ulyssess. By: Paul Lim and Brittany Griner. SPACE CRAFT. Reliable, radiation resistance, and spin stabilized Approximately 370kg (814 pounds) Box-like main structure 1.65 meter Earth pointing antenna Energy requirement. Scientific objectives.

181 views • 7 slides

In Situ Observations of Corotating Rarefaction Regions with STEREO

Introduction

163 views • 1 slides