Results 41 to 50 of about 2,960 (140)
New radical-cation salts based on tetramethyltetrathiafulvalene (TMTTF) and tetramethyltetraselenefulvalene (TMsTSF) with metallacarborane anions (TMTTF)[3,3′-Cr(1,2-C2B9H11)2], (TMTTF)[3,3′-Fe(1,2-C2B9H11)2], and (TMTSF)2[3,3′-Cr(1,2-C2B9H11)2] were ...
Denis M. Chudak +11 more
doaj +1 more source
Global Twist of Sunspot Magnetic Fields Obtained from High Resolution Vector Magnetograms
The presence of fine structures in the sunspot vector magnetic fields has been confirmed from Hinode as well as other earlier observations. We studied 43 sunspots based on the data sets taken from ASP/DLSP, Hinode (SOT/SP) and SVM (USO).
Bao +28 more
core +1 more source
The Faraday Effect Tracker of Coronal and Heliospheric Structures (FETCH) instrument
There continue to be open questions regarding the solar wind and coronal mass ejections (CMEs). For example: how do magnetic fields within CMEs and corotating/stream interaction regions (CIRs/SIRs) evolve in the inner heliosphere?
Elizabeth A. Jensen +18 more
doaj +1 more source
Bimodal Distribution of Magnetic Fields and Areas of Sunspots
We applied automatic identification of sunspot umbrae and penumbrae to daily observations from the Helioseismic Magnetic Imager (HMI) on board the Solar Dynamics Observatory (SDO) to study their magnetic flux (B) and area (A).
Pevtsov, Alexei A., Tlatov, Andrey G.
core +1 more source
In our previous article (Priyal et al. in Solar Phys. 289, 127, 2014) we have discussed the details of observations and methodology adopted to analyze the Ca-K spectroheliograms obtained at the Kodaikanal Observatory (KO) to study the variation of Ca-K ...
Belur, Ravindra +3 more
core +1 more source
Formation and eruption of sigmoidal structure from a weak field region of NOAA 11942 [PDF]
Using observations from Solar Dynamics Observatory, we studied an interesting example of a sigmoid formation and eruption from small-scale flux canceling regions of active region (AR) 11942.
Doddamani, V. H. +3 more
core +2 more sources
Evolution of magnetic fields and energetics of flares in active region 8210 [PDF]
To better understand eruptive events in the solar corona, we combine sequences of multi-wavelength observations and modelling of the coronal magnetic field of NOAA AR 8210, a highly flare-productive active region.
Canfield, Richard C., Regnier, Stephane
core +1 more source
Solar Sources of Interplanetary Magnetic Clouds Leading to Helicity Prediction
Abstract This study identifies the solar origins of magnetic clouds that are observed at 1 AU and predicts the helical handedness of these clouds from the solar surface magnetic fields. We started with the magnetic clouds listed by the Magnetic Field Investigation (MFI) team supporting NASA's Wind spacecraft in what is known as the MFI table and worked
Roger K. Ulrich, Pete Riley, T. Tran
wiley +1 more source
The Solar Activity Monitor Network – SAMNet
The Solar Activity Magnetic Monitor (SAMM) Network (SAMNet) is a future UK-led international network of ground-based solar telescope stations. SAMNet, at its full capacity, will continuously monitor the Sun’s intensity, magnetic, and Doppler velocity ...
Erdélyi Robertus +39 more
doaj +1 more source
Effect of Polarimetric Noise on the Estimation of Twist and Magnetic Energy of Force-Free Fields
The force-free parameter $\alpha$, also known as helicity parameter or twist parameter, bears the same sign as the magnetic helicity under some restrictive conditions.
Ai +35 more
core +1 more source

