Title: Radial gradients of the low-energy proton background between 1 and 80 AU during solar activity minima Author: Kecskemety Karoly Last modified by
Counts vs. Energy/charge ... Vertical red bars represent high count rates for He2 and H ... Both O and Fe count spectra display tails above the H solar wind speed. ...
Suprathermal electron energization in reconnection jet braking regions A. Vaivads (1), A. Retin (2), A. snes (3), R. Nakamura (2), H. Hasegawa (4), Y ...
Suprathermal Tails at 1 AU during quiet, moderately disturbed, and disturbed time periods ... is lower for He and decreases with the level of disturbance ...
Pickup Ions and Reservoir for Energetic Particles George Gloeckler & Eberhard M bius PUI Session PUI Production Rates Didkowski et al. PUI Sources Drews et al ...
Longitude dependence of composition. Composition over large energy range ... Beacon Data. Real time heavy ion composition - new. H and e- complementary to ACE ...
In Situ Observations of CMES. in the Heliosphere ... [e.g., Gosling, 1990; Neugebauer and Goldstein, 1997] Variability in counter-streaming electrons ...
IMPACT- will sample the 3-D distribution of solar wind plasma electrons, the ... rays), sputtering off the moon, outgassing from comets, solar wind dust ...
f(w)=fow 5 tails are observed at all levels of disturbance throughout the heliosphere ... cm-3 dyne/cm2 ... ru =1.76 10-27 gm/cm3 Pu =1.42 10-13 dyne/cm2 ...
L'avenir du Soleil en France : l'apr s-SOHO Jean-Claude Vial Institut d Astrophysique Spatiale, Orsay, France Solar Terrestrial Relations Observatory ...
Occasional high-speed streams produce a 'shoulder' on the solar wind distribution. ... These are the first spectra to extend continuously from solar wind to cosmic ray ...
OK, it's really the neutron and gamma-ray. detector proposed ... a spectrogram: AUI, NRAO/NSF, NJIT, et al. http://www.ovsa.njit.edu/fasr/ G. Graphics: NJIT/NSF ...
Present and Future Research Directions and Space Missions for ... Spectrogram plot: time-energy, colors represent counts. RHESSI and GOES. GOES in LINEAR scale! ...
... I am going to discuss, so bear with me if I say something trivial ... source located several AU closer to the sun. and closer to the pole than Voyager 1 ...
Longwen Yan, Guangjiu Lei, Jiquan Zhang, Tao Jiang, Yan Zhou, Mingliang Shi, ... Prad/POH 1 at edge lead to disruption. Analyses of NBI heating effects ...
Chemistry in Extreme ... propulsion systems, physical organic chemistry, ... processes involving small boron-bearing systems via quantum chemical methods ...
This work was performed under the auspices of the U.S. Department of Energy by ... S.Skupsky, C.Bibeau, W.Meier, K.Manes, S.Dixit, J.Hunt, E.Moses, J.Murray, R.Town ...
Solar and Heliospheric Observatory (SOHO) Objective: To answer the following three fundamental scientific questions about the Sun: What is the structure and dynamics ...
Hollow profile also observed using 9-chord interferometer. Evidence of outward convective flux ... Coherent Density Fluctuations are Observed on the Interferometer ...
THEORY SUMMARY J. W. Van Dam vandam@physics.utexas.edu Please send me comments! 8th IAEA Technical Committee Meeting on Energetic Particles in Magnetic Confinement ...
... tools and projects below shows the kind of ideas being ... van der Linden ROB Uses fast internet access & caching. ... SWAVES teams UCLA radio data from STEREO. ...
The Solar Corona: Arthur B. C. Walker prepared by Ruth Howes Marquette University with support from the Wisconsin Space Grant Consortium Why Study the Sun?
Basic processes of turbulent plasmas, 2003. A composite fluctuation spectrum in the Solar wind ... Still extremely complex due to dielectric effects, screening, etc...
CYR / STEREO Space Weather and the Space Weather Beacon ... ROBERT ULLRICH, JEREMY MCCAULEY, PAUL TURIN, KEN MCKEE, BILL DONOKOWSKI /The Stereo IMPACT Boom ...
Hyesung Kang. Pusan National University, Korea. Diffusive ... 1041 erg/s ~ 10% LSNe (1051 erg x 1/(30years) x 10 %) = energy of escaping CRs. from our Galaxy ...
Title: Surface-bounded Atmosphere of Europa Author: Shematovich Last modified by: SZEMATOWICZ Created Date: 3/28/2003 9:34:19 AM Document presentation format
The work here presented results from a collaboration with: ... coronagraphic imaging (a 12-cm telescope with a coronagraph to suppress the Moon' disk) ...
loop strands with isothermal cross-sections, at FWHM widths of ... in the CELTIC model is consistent. with a semi-Gaussian distribution. with a Gaussian width of ...
The STEREO Space Weather Group consists of scientists associated with the STEREO ... JAVA-3D Synoptic J. Luhmann, P. Schroeder JAVA-3D applet for viewing 3D Sun ...