'Solar atmosphere' presentation slideshows

The VTT Helioseismology Concept with HELLRIDE and CARMA J.Staiger , KIS Freiburg

The VTT Helioseismology Concept with HELLRIDE and CARMA J.Staiger , KIS Freiburg. The VTT Helioseismology Concept. KIS Helioseismology Group: Markus Roth Gisela Baumann Hanspeter Doerr Kolja Glogowski Wiebke Herzberg Ariane Schad Aneta Wisniewska Wolfgang Zima

1.13k views • 97 slides

European and French solar physics from space

649 views • 52 slides

The Sun

529 views • 36 slides

ATST Science Requirements

495 views • 34 slides

The REAL OCCULT:

The REAL OCCULT:. Lunar & Solar Eclipses and Asteroid & Stellar Disappearances Sometimes Involving Luna By Dr. Harold Williams of Montgomery College Planetarium http://montgomerycollege.edu/Departments/planet/. Types of Occultations. Lunar Eclipse, Solar Eclipse,

562 views • 31 slides

Lecture 8

Lecture 8. Optical depth. Review: opacity. How does the intensity of radiation depend on opacity and distance travelled through a homogeneous medium? . Opacity ( k ) is a cross-section per unit mass (units m 2 /kg) of material for absorbing photons of a specific wavelength.

693 views • 25 slides

The Advanced Technology Solar Telescope

The Advanced Technology Solar Telescope. The ATST Project is funded by the National Science Foundation through the National Solar Observatory which is operated by the Association of Universities for Research in Astronomy (AURA), Inc. The Site & Buildings for ATST.

357 views • 22 slides

The Sun

The Sun. Sol. Solar Data. Mass (kg) 1.989x10 30 Mass (Earth = 1) 332,830 Equatorial radius (km) 695,000 Equatorial radius (Earth = 1) 108.97 Mean density (gm/cm 3 ) 1.410 Surface gravity (m/s 2 ) 273 Rotational period (days) 25-36 Escape velocity (km/sec) 618.02

335 views • 21 slides

283 views • 21 slides

Martin Asplund

Galactic archeology & planet formation. Martin Asplund. Galactic archaeology. Inner/outer halos. Bulge. Thin/thick disks. Stellar abundances + kinematics to unravel the history of the Milky Way and its populations: Nucleosynthesis, IMF, SFR, infall/outflow, migration etc

440 views • 21 slides

Principle Investigator: Dr. Yu.D. Kotov Tel/fax (007-095)-3240616 E-mail: kotov@mephi.ru

Launch date: end of 2007, from Plesetsk (Russia). Space Research Program. RUSSIAN SATELLITE PROJECT "CORONAS-PHOTON" FOR THE STUDY OF SOLAR FLARE HARD RADIATIONS. Russian Aviation and Space Agency Russian Academy of Science Principal Organization: Moscow Engineering Physics Institute.

398 views • 19 slides

SOHO OVERVIEW

464 views • 17 slides

323 views • 16 slides

The Sun

462 views • 14 slides

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.

189 views • 12 slides

The Sun 24.3

186 views • 9 slides

Abundances in the Solar Atmosphere and in the Solar Wind

Abundances in the Solar Atmosphere and in the Solar Wind. Tuesday afternoon - 25 June 2013 Wednesday morning - 26 June 2013 Daniel Wolf Savin (Columbia University). Abundances (Tues PM). Peter Young (George Mason)

241 views • 8 slides

The Sun

By Elisha. The Sun. The Sun

209 views • 7 slides

Today:

Today:. Neutrinos Solar atmosphere: Photosphere granulation Chromosphere spicules Corona Solar wind Solar magnetic fields Sunpots Sunspot cycle Reconnection, flares, prominences and coronal mass ejections. Neutrinos. Solar atmosphere: photosphere.

168 views • 3 slides

Views of the Sun

How to Make a Forecast. Joe Kunches and Barbara Poppe Space Environment Center. The process of forecasting brings to bear all of the tools available: data, imagery, statistics, models, pattern recognition, and experience.

69 views • 1 slides