'Quiet sun' presentation slideshows

Comments for a preliminary EIS science plan

Comments for a preliminary EIS science plan. H. Hara 2005 Oct 31. For the science meeting at ISAS. Observables. ??. ?w. Line intensity Line shift by Doppler motion Line width temperature, nonthermal motion Information from selected two line ratio Temperature Density.

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The magnetism of the very quiet Sun

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The EUV spectral irradiance of the Sun from minimum to maximum

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Heating from Reconnection Quantified

Heating from Reconnection Quantified. Dana Longcope Montana State University. Acknowledgments:. Erik Aver Jonathan Cirtain Charles Kankelborg Dave McKenzie Jason Scott Alexei Pevtsov Robert Close Clare Parnell Eric Priest NASA grant NAG5-10489 NSF grant ATM 97227. MSU. NSO Sac Peak.

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Initial Results of EIS

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Signatures of ~ axions in astrophysical observations ? QSO s, PVLAS @ ~eV

Signatures of ~ axions in astrophysical observations ? QSO s, PVLAS @ ~eV ? linear polarization ? ~axions ? favour ~ eV ? ? ww indirect DM searches @ HE For axions a few Konstantin Zioutas University of Patras & CERN Patras 19 th May 2006.

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Quiet Sun intensity distributions

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New Opportunities: Flux Emergence Modeling

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High Energy Measurements for Solar, Heliospheric, Magnetospheric, and Atmospheric Physics

High Energy Measurements for Solar, Heliospheric, Magnetospheric, and Atmospheric Physics. R. P. Lin J. Sample, A. Shih, S. Christe, S. Krucker, I. Hannah Physics Department & Space Sciences Laboratory University of California, Berkeley & D. Smith (UCSC), R. Millan (Dartmouth).

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UCB-SSL Plans for Next Year Joint CCHM/CWMM Workshop, July 2007

UCB-SSL Plans for Next Year Joint CCHM/CWMM Workshop, July 2007. W.P. Abbett, G.H. Fisher, and B.T. Welsch. RADMHD: Modeling the combined convection zone-to-corona system:. The code solves the resistive, fully-compressible MHD system of equations:.

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G.N. Rajasekhara Girish Kumar Beeharry Mauritius Radio Telescope

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EIS - MSSL/NRL EUV Imaging Spectrometer SOT - ISAS/NAOJ Solar Optical Telescope

EIS - MSSL/NRL EUV Imaging Spectrometer SOT - ISAS/NAOJ Solar Optical Telescope XRT - SAO/ISAS X-ray Telescope FPP - Lockheed/NAOJ Focal Plane Package. Mission Characteristics. Launch date: August 2006 Launch vehicle: ISAS MV Mission lifetime: 3 years. Orbit: Polar, sun synchronous

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The Physical Consequences of Under-resolution for N-dimensional Models of the Solar Atmosphere

The Physical Consequences of Under-resolution for N-dimensional Models of the Solar Atmosphere. Dr. Stephen Bradshaw. Prof. Peter Cargill. Imperial College London & University of St. Andrews. Rice University. 1. Questions.

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Kostas Tziotziou IAASARS, National Observatory of Athens, Greece Work in collaboration with:

Free Magnetic E nergy and R elative H elicity in Quiet Sun Regions and their role in Solar Dynamics. Kostas Tziotziou IAASARS, National Observatory of Athens, Greece Work in collaboration with: Georgia Tsiropoula , IAASARS, National Observatory of Athens, Greece

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Emergence of Small-Scale Magnetic Loops in the Quiet Sun Internetwork

Emergence of Small-Scale Magnetic Loops in the Quiet Sun Internetwork. R. Centeno, H Socas-Navarro, B. Lites, M. Kubo High Altitude Observatory (NCAR), Boulder CO 80301, USA. Z. Frank, R. Shine, T. Tarbell, A. Title Lockheed Martin Space and Astrophysics Laboratory, Palo Alto, CA, USA.

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Flux Emergence Rate in Coronal Holes and in Adjacent Quiet-sun Regions

Flux Emergence Rate in Coronal Holes and in Adjacent Quiet-sun Regions. Valentyna Abramenko Big Bear Solar Observatory Lennard Fisk University of Michigan Vasyl Yurchyshyn Big Bear Solar Observatory. Abstract. 1. Coronal holes are regions where the open magnetic

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Four slit/slot selections available EUV line spectroscopy - Slits

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Locating the solar source of 13 April 2006 Magnetic Cloud

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Joint Planning of SOT/XRT/EIS Observations Outline of 90 Day Initial Observing Plans

Joint Planning of SOT/XRT/EIS Observations Outline of 90 Day Initial Observing Plans. T. Shimizu, L Culhane. SOT Initial Science Plan. Principal Topics. Active region tracking: - Emerging AR - Mature/decaying AR - Flaring AR - Subsurface flows - MHD waves Quiet Sun:

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