Results 31 to 40 of about 979,369 (340)

Solar mean magnetic field of the chromosphere

open access: yesJournal of Astrophysics and Astronomy, 2023
The Solar Mean Magnetic Field (SMMF) is the mean value of the line of sight (LOS) component of the solar vector magnetic field averaged over the visible hemisphere of the Sun. So far, the studies on SMMF have mostly been confined to the magnetic field measurements at the photosphere. In this study, we calculate and analyse the SMMF using magnetic field
M. Vishnu, K. Nagaraju, Harsh Mathur
openaire   +2 more sources

VECTOR MAGNETIC FIELDS OF SOLAR GRANULATION [PDF]

open access: yesThe Astrophysical Journal, 2008
24 pages in total, 9 ...
Chunlan Jin, Jingxiu Wang, Meng Zhao
openaire   +4 more sources

The solar and interplanetary causes of the recent minimum in geomagnetic activity (MGA23): a combination of midlatitude small coronal holes, low IMF B Z variances, low solar wind speeds and low solar magnetic fields

open access: yes, 2011
. Minima in geomagnetic activity (MGA) at Earth at the ends of SC23 and SC22 have been identified. The two MGAs (called MGA23 and MGA22, respectively) were present in 2009 and 1997, delayed from the sunspot number minima in 2008 and 1996 by ~1/2–1 years.
B. Tsurutani, E. Echer, W. Gonzalez
semanticscholar   +1 more source

TANGLED MAGNETIC FIELDS IN SOLAR PROMINENCES [PDF]

open access: yesThe Astrophysical Journal, 2010
Solar prominences are an important tool for studying the structure and evolution of the coronal magnetic field. Here we consider so-called "hedgerow" prominences, which consist of thin vertical threads. We explore the possibility that such prominences are supported by tangled magnetic fields. A variety of different approaches are used.
A. A. van Ballegooijen   +1 more
openaire   +3 more sources

Solar Magnetism in the Polar Regions

open access: yesLiving Reviews in Solar Physics, 2015
This review describes observations of the polar magnetic fields, models for the cyclical formation and decay of these fields, and evidence of their great influence in the solar atmosphere.
Gordon J. D. Petrie
doaj   +1 more source

Magnetic Reconnection as the Driver of the Solar Wind

open access: yesThe Astrophysical Journal, 2023
We present EUV solar observations showing evidence for omnipresent jetting activity driven by small-scale magnetic reconnection at the base of the solar corona.
Nour E. Raouafi   +18 more
doaj   +1 more source

Solar Vortices and Magnetic Fields [PDF]

open access: yesNature, 1908
SEVERAL weeks ago I discussed with Prof. Hale the matter of solar vortices and magnetic fields, with reference to his recent discoveries, briefly described in NATURE for August 20 (p. 368). It did not seem to me probable that the effects could be accounted for by unequal diffusivity of the positive and negative ions, or by centrifugal separation, nor ...
openaire   +3 more sources

Observational Study of Recurrent Jets Confined by Active Region Loops

open access: yesThe Astrophysical Journal, 2023
With high spatial and temporal resolution data from the Solar Dynamics Observatory and the New Vacuum Solar Telescope (NVST), we present observations of recurrent jets confined by coronal loops that occurred in the active region NOAA 11726 from 02:00 to ...
Liheng Yang   +6 more
doaj   +1 more source

Fractality of Magnetic Helicity Distribution in the Solar Corona

open access: yesThe Astrophysical Journal
We find a universal power-law scaling of magnetic helicity distribution in the solar corona. Magnetic helicity is a dynamical invariant for ideal magnetohydrodynamics (MHD) and characterizes complex magnetic field structure by measuring the degree of ...
Anda Xiong   +3 more
doaj   +1 more source

Ferrocene Derivatives Enable Ultrasensitive Perovskite Photodetectors with Enhanced Reverse Bias Stability

open access: yesAdvanced Functional Materials, EarlyView.
Novel ferrocene derivatives (e.g., FcPhc2) are used as an ultrathin layer hole‐blocking layer, reducing hole injection from the Ag contact. This results in an ultralow noise spectral density of 1.2 × 10−14 A Hz−1/2, and a high specific detectivity of 8.1 × 1012 Jones at −0.5 V.
Eunyoung Hong   +16 more
wiley   +1 more source

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