'Solar minimum' presentation slideshows

Surviving in space: the challenges of a manned mission to Mars

837 views • 62 slides

Surviving in space: the challenges of a manned mission to Mars

784 views • 52 slides

The Sun

530 views • 36 slides

Propagation of galactic cosmic rays and Jovian electrons in the heliosphere

Propagation of galactic cosmic rays and Jovian electrons in the heliosphere. R. B. McKibben Department of Physics and Space Science Center, Institute for the Study of Earth, Oceans, and Space University of New Hampshire Durham, NH, USA.

461 views • 31 slides

20 09, December 12

378 views • 31 slides

Solar Modulation: A Theoretical Perspective

Solar Modulation: A Theoretical Perspective Modeling of cosmic ray charge-sign dependence in the heliosphere. Marius Potgieter Unit for Space Physics North-West University Potchefstroom, South Africa. Colaborators: Stefan Ferreira, Bernd Heber

409 views • 28 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

39 th COSPAR Scientific Assembly Mysore, INDIA July 14-22, 2012

Voyager In The Distant Heliosheath: Continuing The Quest Of Victor Hess. F.B. McDonald 1 , W.R. Webber 2 , E.C. Stone 3 , A.C. Cummings 3 , B.C. Heikkila 4 , N. Lal 4 1 Institute for Physical Science and Technology, Univ. of Maryland, College Park, MD, USA

313 views • 23 slides

323 views • 20 slides

National Science Foundation: NSF and Space Weather Rich Behnke

National Science Foundation: NSF and Space Weather Rich Behnke Division of Atmospheric and Geospace Sciences June 21, 2011 . Space Weather at NSF. NSF Role: Fundamental research and modeling Ground-based facilities Education Interagency Partner.

346 views • 19 slides

STEREO PLASTIC STATUS

STEREO PLASTIC STATUS. A.B. Galvin with contributions by C. Farrugia and L. Ellis. Telemetry Losses - STA. Telemetry Losses - STB. Operations.

303 views • 16 slides

Space Weather Measurements: Capabilities and Needs

Space Weather Measurements: Capabilities and Needs. Howard J. Singer NOAA Space Environment Center NSF Workshop on Small Satellite Missions for Space Weather and Atmospheric Research George Mason University, Arlington, VA May 17, 2007. Outline.

368 views • 16 slides

Rodney Viereck NOAA Space Weather Prediction Center Drag Data provided by John Emmert NRL

Neutral Density During the Recent Solar Minimum Contributions from Solar, Geomagnetic Activity, and Anthropogenic. Rodney Viereck NOAA Space Weather Prediction Center Drag Data provided by John Emmert NRL MURI Workshop, Boulder October 2010.

295 views • 14 slides

Solar Physics at UCLan

Solar Physics at UCLan. Dr Barbara Bromage Centre for Astrophysics University of Central Lancashire. Robert Walsh Mike Marsh (postdoc) Jane Noglik (Ph.D.student). Barbara Bromage Steve Higgins (postdoc) Stephen Chapman (Ph.D.student) Martin Birch (part-time Ph.D.student).

261 views • 12 slides

A study of the global heliospheric modulation of galactic Carbon

A study of the global heliospheric modulation of galactic Carbon. M. D. Ngobeni, M . S. Potgieter Centre for Space Research, North-West University, 2520 Potchefstroom, South Africa. Introduction: Observations from V1, V2 and ACE [1997-2010]. Webber, Private Communication 2011.

225 views • 11 slides

Solar Cycle 23 and Early Predictions for Solar Cycle 24

Solar Cycle 23 and Early Predictions for Solar Cycle 24. Carl Luetzelschwab K9LA. Cycle 23. Maximum smoothed sunspot number of 121 in early 2000. Secondary peak in late 2001 Great 6m F2 DX!. we are here. solar minimum. Minimum expected in late 2006 / early 2007.

337 views • 10 slides

NOAA Agency Report Highlights of Activities

183 views • 10 slides

Thermospheric Response to Transient Joule Heating and Solar-Flare Radiation

Thermospheric Response to Transient Joule Heating and Solar-Flare Radiation Yanshi Huang , University of Texas at Arlington Arthur D. Richmond , NCAR High Altitude Observatory Yue Deng , University of Texas at Arlington Philip C. Chamberlin , NASA GFSC Solar Physics Laboratory

195 views • 9 slides

Predictions of Solar Wind Speed and IMF Polarity Using Near-Real-Time Solar Magnetic Field Updates

Purpose & Basis. Purpose of Model: Th e Wang-Sheeley model is an empirical model that predicts the background solar wind speed and the interplanetary magnetic field (IMF) polarity at Earth .

144 views • 1 slides

Interdependence of solar plasma flows and magnetic fields

Interdependence of solar plasma flows and magnetic fields E.J. Zita & C. Smith, The Evergreen State College, Olympia, WA 98505; N.E. Hurlburt, LMSAL, Palo Alto, CA 94304. D. Discussion. I. Abstract. A-B: Testing for Proctor Effect (PE) in Hinode Data.

117 views • 1 slides