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field solar published presentations and documents on DocSlides.

Polarimetric shapes of spectral lines in solar observations
Polarimetric shapes of spectral lines in solar observations
by karlyn-bohler
Egidio Landi Degl’Innocenti. Dipartimento di Fi...
Cosmic Rays, Neutron Monitors, Solar Cycles &
Cosmic Rays, Neutron Monitors, Solar Cycles &
by isabella2
the Heliosphere. Riaan Steenkamp. University of Na...
Photoelectrons traveling in both directions along the magnetic field reveal an unexpected loop that
Photoelectrons traveling in both directions along the magnetic field reveal an unexpected loop that
by daniella
Open: Venus – solar wind. Closed: Venus – Venu...
The Mean Field and Large-Scale
The Mean Field and Large-Scale
by callie
Multipole. . Components. The figures show the sol...
Probing Energy Release of Solar Flares
Probing Energy Release of Solar Flares
by genevieve
M. . Prijatelj. Carnegie Mellon University. Adviso...
THE DYNAMICS OF DEEP SOLAR MERIDIONAL CIRCULATION
THE DYNAMICS OF DEEP SOLAR MERIDIONAL CIRCULATION
by calandra-battersby
OVER THE SOLAR CYCLE. DÁRIO PASSOS - CENTRA...
Drivers and Solar Cycles Trends of
Drivers and Solar Cycles Trends of
by danika-pritchard
Extreme Space . Weather Disturbances . Emilia Kil...
Drivers and Solar Cycles Trends of
Drivers and Solar Cycles Trends of
by conchita-marotz
Extreme Space . Weather Disturbances . Emilia Kil...
Solar Orbiter
Solar Orbiter
by test
Heliosphere= . the . region of space, encompassin...
An overview of the cycle variations in the solar corona
An overview of the cycle variations in the solar corona
by yoshiko-marsland
Louise Harra. lkh. @mssl.ucl.ac.uk. UCL Departmen...
unit
unit
by sherrill-nordquist
5: Sun and . Star formation. General Properties. ...
The Sun and the Stars
The Sun and the Stars
by alida-meadow
The Sun and the Stars. The Sun and the Stars. Lim...
Theoretical
Theoretical
by luanne-stotts
. Astrophysics. II. Markus Roth. Fakultät für...
Introduction to the Ionosphere
Introduction to the Ionosphere
by tatiana-dople
Julie A. . Feldt. CEDAR-GEM workshop. June 26. th...
Global MHD Simulations of Dayside Magnetopause Dynamics.
Global MHD Simulations of Dayside Magnetopause Dynamics.
by natalia-silvester
THEMIS Event: May 20, 2008. 20:30 – 22:30. NASA...
Theoretical
Theoretical
by giovanna-bartolotta
. Astrophysics. II. Markus Roth. Fakultät für...
Theoretical
Theoretical
by stefany-barnette
. Astrophysics. II. Markus Roth. Fakultät für...
Solar magnetic fields:
Solar magnetic fields:
by celsa-spraggs
basic concepts and magnetic topology . Anna (. An...
Space Weather
Space Weather
by pasty-toler
Dr. Phillip C. Anderson. W. B. Hanson Center for ...
Figure 1. Sketch of the axisymmetric case (
Figure 1. Sketch of the axisymmetric case (
by pamella-moone
m. = 0) tube structure. Twisted field lines are...
Evolution of the heliospheric magnetic field
Evolution of the heliospheric magnetic field
by tatiana-dople
Mathew Owens. 1. Space and Atmospheric Electricit...
Long-term evolution of magnetic fields on the Sun
Long-term evolution of magnetic fields on the Sun
by alida-meadow
. Alexei A. . Pevtsov. US National Solar ...
The Helioseismic and Magnetic Imager (HMI) on NASA’s Solar Dynamics Observatory (SDO) has conti
The Helioseismic and Magnetic Imager (HMI) on NASA’s Solar Dynamics Observatory (SDO) has conti
by esther
HMI Observations of Solar Flares in Solar Cycle . ...
Modelling the Effect of Magnetic Field Variation on Solar Flares
Modelling the Effect of Magnetic Field Variation on Solar Flares
by caroline
Introduction. Solar flares occur when energy is co...
The Asymmetric Polar Field Reversal – Long-Term Observati
The Asymmetric Polar Field Reversal – Long-Term Observati
by danika-pritchard
J. . Todd . Hoeksema, . Solar Observatories Group...
Back Reaction on the Photospheric Magnetic field in Solar E
Back Reaction on the Photospheric Magnetic field in Solar E
by olivia-moreira
Dandan Ye. Contents. Paper review: . 2005 J....
The Asymmetric Polar Field Reversal – Long-Term Observati
The Asymmetric Polar Field Reversal – Long-Term Observati
by sherrill-nordquist
J. . Todd . Hoeksema, . Solar Observatories Group...
Faraday Rotation:
Faraday Rotation:
by tatyana-admore
Unique Measurements of Magnetic Fields in the Out...
HF Propagation
HF Propagation
by debby-jeon
How to snag that DX!. Michael Smith, N5TGL. Agend...
31 st
31 st
by stefany-barnette
Annual General Meeting. 26. th. July, 2012. 2. ...
Defects in solar cell materials: the good, the bad, and the
Defects in solar cell materials: the good, the bad, and the
by test
Tim Gfroerer. Davidson College, Davidson, NC. wit...
A New Solar Observing Network For Space Weather Operations
A New Solar Observing Network For Space Weather Operations
by faustina-dinatale
Frank Hill, NSO, USA. Markus Roth, KIS, Germany. ...
Science Requirements for Helioseismology
Science Requirements for Helioseismology
by stefany-barnette
Frank Hill. NSO. SPRING Workshop. Nov. 26, 2013. ...
The Sun
The Sun
by mitsue-stanley
Solar Prominence. Sun Fact Sheet. The Sun is a no...
What can helicity redistribution in solar eruptions tell us
What can helicity redistribution in solar eruptions tell us
by karlyn-bohler
by Brian Welsch,. JSPS Fellow (Short-Term. ),. Sp...
Global Distribution of Slow Solar Wind
Global Distribution of Slow Solar Wind
by jane-oiler
N. U. Crooker, S. W. . Antiochos. ,. . X. Zhao, ...
Propagation Trends 2014-2015
Propagation Trends 2014-2015
by myesha-ticknor
Dayton 2014. . Solar Maximum!. But the slow decl...
Image credit: NASA
Image credit: NASA
by luanne-stotts
Response of the Earth’s environment to solar ra...
An introduction to the sun
An introduction to the sun
by danika-pritchard
Contents. Introduction. General . information. St...
Going Green
Going Green
by tawny-fly
By: Michael Raletz. Green is the . N. ew Black!. ...