Dependence the Umbral Intensity of Sunspot on Its Magnetic Field Strength

doi 10.31725/0552-5829-2019-169-172
Full Text
Abstract

Available in full text

Date
Authors
Publisher

The Central Astronomical Observatory of the Russian Academy of Sciences at Pulkovo

Related search

Brightness, Distribution, and Evolution of Sunspot Umbral Dots

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2008English

High Resolution Magnetic Field Measurements in the Sunspot Photosphere

International Astronomical Union Colloquium
1993English

19F Spin–lattice Relaxation of Perfluoropolyethers: Dependence on Temperature and Magnetic Field Strength (7.0–14.1T)

Journal of Magnetic Resonance
BiochemistryNuclearHigh Energy PhysicsCondensed Matter PhysicsBiophysics
2014English

The Three-Dimensional Structure of the Magnetic Field of a Sunspot

Proceedings of the International Astronomical Union
AstrophysicsAstronomyPlanetary ScienceSpace
2008English

Magnetic Field Variations Associated With Umbral Flashes and Penumbral Waves

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2018English

Evolutionary Characteristics of the Interplanetary Magnetic Field Intensity

Astronomical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
2018English

Relationship Between the Variations of Sunspot Magnetic Field and the Brightness of Its Umbra for the Long-Term Oscillations of Sunspots

2019English

Measurement of the Tilt Angle of the Sunspot Magnetic Field Axis (Method and Results)

2019English

The Effect of Changing the Magnetic Field Strength on HiPIMS Deposition Rates

Journal of Physics D: Applied Physics
SurfacesUltrasonicsCondensed Matter PhysicsAcousticsOpticalMagnetic MaterialsFilmsCoatingsElectronic
2015English

Amanote Research

Note-taking for researchers

Follow Amanote

© 2024 Amaplex Software S.P.R.L. All rights reserved.

Privacy PolicyRefund Policy