Sentences with phrase «for magnetic flux»

Not exact matches

The simulated reconnection also supports the observations of bright flaring loops where the hyperbolic flux tube and filament met — evidence for magnetic reconnection.

For certain applications, there is indeed a desire for a kind of compensator, namely for a relatively low magnetic flux to match conditions as under very strong fielFor certain applications, there is indeed a desire for a kind of compensator, namely for a relatively low magnetic flux to match conditions as under very strong fielfor a kind of compensator, namely for a relatively low magnetic flux to match conditions as under very strong fielfor a relatively low magnetic flux to match conditions as under very strong fields.

Fine details of a magnetic flux rope captured by the New Solar Telescope at Big Bear Solar Observatory for Solar Active Region 11817 on 2013 August 11.

Laboratory studies of magnetic flux leakage turned out to be crucial for repairing broken gas pipelines (see «How to Fix Our Most Vexing Problems, From Mosquitoes to Potholes to Missing Corpses»).

Using all available geologic, tectonic and geothermal heat flux data for Greenland — along with geothermal heat flux data from around the globe — the team deployed a machine learning approach that predicts geothermal heat flux values under the ice sheet throughout Greenland based on 22 geologic variables such as bedrock topography, crustal thickness, magnetic anomalies, rock types and proximity to features like trenches, ridges, young rifts, volcanoes and hot spots.

This project will characterize the quiet - sun magnetic field by studying observational signatures of events such as for example flux cancelation, convective collapse and granular buffeting of magnetic elements.

The results of analysis of thermobaric field variations for the periods of invasion of abnormally powerful solar cosmic ray fluxes and magnetic storms confirm the reality of manifestation of heliogeophysical disturbances.

Similarly to the solar magnetic modulation, high geomagnetic field intensity decreases the flux of galactic cosmic rays and radionuclide production rates and the opposite for low geomagnetic field intensity.

The primary physical mechanism responsible for much of this energy, mass, and momentum flow is magnetic reconnection, which can explosively convert magnetic energy into kinetic energy of the magnetospheric plasma and disconnect or break parcels of magnetic flux.

We also use the solar magnetic field (B0) and F10.7 flux data from http://spidr.ngdc.noaa.gov; these data are available only for the last two and last five SCs, respectively.

We thank the SIDC team, World Data Center, NOAA - NGDC, and SPIDR, NGDCNOAA, for the data on sunspot, SC characteristics, solar magnetic field, and F10.7 flux data respectively.

The solar heliosphere is the name for the tenuous gas and pieces of magnetic flux that is ejected off the surface of the sun.

The planets may have a spin - orbit coupling effect on the Sun which affects its rotation rate, which would then affect the solar dynamo and sunspot production, and therefore the build up of magnetic flux at the poles, and the length of a solar cycle: if the solar cycle is weaker with less sunspots, it'll take longer for the build up of opposing flux to reach the point when it flips the poles.

I was looking for a correspondence of magnetic flux and solar UV — see Fig 5 — it seems to be there (but I wonder why).

Inductive heating occurs when a conductor (like the Earth) moves through magnetic flux (e.g. rotates and revolves around the Sun) or when the flux through a stationary conductor changes for other reasons.

For an alternative calibration see: Nicola Scafetta & Richard C. Willson, ACRIM - gap and TSI trend issue resolved using a surface magnetic flux TSI proxy model, Geophysical Research Letters, Vol.

Recent work attempts to account for the chain of physical processes in which solar magnetic fi elds modulate the heliosphere, in turn altering the penetration of the galactic cosmic rays, the flux of which produces the cosmogenic isotopes that are subsequently deposited in the terrestrial system following additional transport and chemical processes.

Supporting material document for: ACRIM - gap and TSI trend issue resolved using a surface magnetic flux TSI proxy model, Nicola Scafetta, Richard C. Willson, Supplement, 2009 (PDF)

Volker Doormann says: July 27, 2011 at 2:38 pm http://adsabs.harvard.edu/abs/2010JGRA..11501104S We have reconstructed the interplanetary magnetic field (IMF), its radial component, and the open solar magnetic flux using the solar modulation potential derived from cosmogenic 10Be radionuclide data for a period covering the past 9300 years.

During the Maunder Minimum, the strength of the IMF was approximately 2 nT compared to a mean value of 6.6 nT for the past 40 years, corresponding to an increase of the open solar magnetic flux of about 350 %.

http://adsabs.harvard.edu/abs/2010JGRA..11501104S «We have reconstructed the interplanetary magnetic field (IMF), its radial component, and the open solar magnetic flux using the solar modulation potential derived from cosmogenic 10Be radionuclide data for a period covering the past 9300 years.

As the process continues and magnetic flux strength of the sunspot group declines, the lifetime of a sunspot group (of the few sunspot groups that do form) has decreased to where we are now at the point that a sunspot group's lifetime is for a number of cases only a few days.

This is in agreement with the recent results of [CITE], but it is in contrast to the earlier analysis of [CITE], and suggests that the source of the irradiance variations is the same for cycles 22 and 23, namely the evolution of the magnetic flux at the solar surface.

This provides strong support for the hypothesis that solar irradiance variations are caused by changes in the amount and distribution of magnetic flux at the solar surface.

If GCR flux is modulated by solar magnetic variability then how do we account for the rise in OHC since around 1970?

The oversize Double Fluxor Magnetic Arrays deliver the greatest flux density of any headphone, an astounding 1.5 Tesla for oustanding control of the driver.

Custom - made Magnetic - flux Low - Hum EI Power Transformer, Fully Enclosed and Shielded for Minimal Leakage