'Solar interior' presentation slideshows

The Solar Interior

The Solar Interior. Free stuff from NASA Goddard Space Flight Center. Courtesy Jack Ireland, L3 Communications, Lab of Astrophysics and Solar Physics, NASA GSFC, Greenbelt, MD. Why study the solar interior. Sheer curiosity Solar-stellar connection

1.16k views • 115 slides

Space weather: solar drivers, impacts and forecasts Henrik Lundstedt

Space weather: solar drivers, impacts and forecasts Henrik Lundstedt Swedish Institute of Space Physics Lund. We live inside the continuously expanding solar corona, i.e. the solar wind, which can be very strong e.g. at times of CMEs. Earth is also exposed

735 views • 61 slides

495 views • 49 slides

Solar Interior/ Nuclear Fusion

664 views • 44 slides

Helioseismic Magnetic Imager and Why We Study Helioseismology

Helioseismic Magnetic Imager and Why We Study Helioseismology. Junwei Zhao W. W. Hansen Experimental Physics Laboratory, Stanford University, Stanford, CA94305-4085. Lecture Plans. Lecture 1 HMI and why we want to do helioseismology studies Lecture 2

510 views • 40 slides

397 views • 39 slides

Helioseismology

Helioseismology. Bill Chaplin, School of Physics & Astronomy University of Birmingham, UK. The Physics of the Sun and the Solar Neutrinos Gran-Sasso, Italy, 4 October 2010. The Unseen Interior. Sir Arthur Eddington. The Unseen Interior.

535 views • 38 slides

Solar Interior/ Nuclear Fusion

498 views • 38 slides

Chapter 29 Section 1

523 views • 35 slides

Standard Solar Models I Aldo Serenelli Institute for Advanced Study, Princeton

477 views • 33 slides

Standard Solar Models I Aldo Serenelli Institute for Advanced Study, Princeton

333 views • 33 slides

Maria Pia Di Mauro INAF- Istituto di Astrofisica Spaziale e Fisica Cosmica Rome (Italy)

HELIOSEISMOLOGY. Maria Pia Di Mauro INAF- Istituto di Astrofisica Spaziale e Fisica Cosmica Rome (Italy). The story. Periodic Motions P ? 5 min of the absorption lines of the photospheric spectrum (Leighton et al. 1962). PULSATIONS OF THE PHOTOSPHERE!!!. Normal Modes.

421 views • 28 slides

423 views • 28 slides

Chapter 9 The Sun

Chapter 9 The Sun. 9.4 The Active Sun. Sunspots : appear dark because slightly cooler than surroundings:. 9.4 The Active Sun. Sunspots come and go, typically in a few days. Sunspots are linked by pairs of magnetic field lines :. 9.4 The Active Sun.

430 views • 25 slides

M4111 The Sun and stars Solar Physics

248 views • 24 slides

Helioseismology

Helioseismology. ???. Dean-Yi Chou. ?????? ? ???. (2010.08, ?? ). 1. Solar Oscillations 2. Global and Local Helioseismology Probing magnetic fields and flows in the solar convection zone with helioseismology 4. Solar acoustic energy in magnetic regions

380 views • 20 slides

Guided Notes about the Sun

140 views • 13 slides

Model of the Solar Interior

217 views • 12 slides

The Sun

The Sun. Physical Data. Hydrogen and Helium composition 696,000 km radius 1.4 grams per cubic centimeter density 25.4 solar day rotation 5780K surface temperature. The Solar Interior. Energy production in the core Radiative transfer Convection zone. The Solar Atmosphere. Photosphere

239 views • 11 slides