'Chromosphere' presentation slideshows

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Exit. Play. Jason Wintz. 15 $1,000,000 14 $500,000 13 $250,000 12 $125,000 11 $64,000 10 $32,000 9 $16,000 8 $8,000 7 $4,000 6 $2,000 5 $1,000 4 $500 3 $300 2 $200 1 $100. Question # 1 For $100. How many planets , excluding Pluto, are in our Solar System? . 7. 8. 6. 9.

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CAN A C H R O M O S P H E R E BE FORMED IN BLACK HOLE DECAYS?

CAN A C H R O M O S P H E R E BE FORMED IN BLACK HOLE DECAYS?. Jane H MacGibbon, B.J. Carr and Don N. Page JANE H MACGIBBON UNIVERSITY OF NORTH FLORIDA. BLACK HOLES IN 4D SPACE-TIME. MacGibbon Carr & Page PRD 78, 064043 (2008) Page Carr & MacGibbon PRD 78, 064044 (2008). MOTIVATION.

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Chapter 29 Section 1

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The Dynamic Chromosphere

The Dynamic Chromosphere. Mats Carlsson Institute of Theoretical Astrophysics, University of Oslo JAXA, November 20 2008. Semi-empirical model. VAL3C. Ca II H-line intensity. 1D NLTE hydrodynamic modelling. SUMER observations. Carlsson, Judge, Wilhelm 1997. Ca H timeseries from Hinode.

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OUR SUN

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OUR SUN

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The Sun

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Solar Radiation

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The Sun http://stardate.org/images/gallery/sun5.jpg

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EARTH SCIENCE

EARTH SCIENCE. THE SUN. ?. 24.3 The Sun .

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Solar Radiation Physical Modeling (SRPM)

Solar Radiation Physical Modeling (SRPM). J. Fontenla June 30, 2005b. Mean Intensity. Emitted Spectra. Radiative Losses. and Net Radiative. Brackett. Atomic. Molecular. Continua. Continua. Atomic Data. Radiative Transfer. Molecular Data. Non-LTE. Molecular. Atomic.

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Photosphere (visible)

Flare (EUV, soft X-rays, hard X-rays). Sunspots (visible). Active Region (Visible, EUV, soft X-rays). Photosphere (visible). Coronal Mass Ejection (Visible, EUV). Chromosphere (EUV, visible). Corona (Visible, EUV, soft X-rays).

296 views • 1 slides