Results 171 to 180 of about 5,203 (216)
SuryaBench: Benchmark Dataset for Advancing Machine Learning in Heliophysics and Space Weather Prediction. [PDF]
Roy S +24 more
europepmc +1 more source
Back reaction of the untwisting solar corona scars sunspots. [PDF]
Xing C, Cheng X, Aulanier G, Ding M.
europepmc +1 more source
Flux equipartition in astrophysical plasma turbulence. [PDF]
Marino R, Xie JH.
europepmc +1 more source
Extraction of metadata from solar disk H-alpha observations at Sacramento Peak Observatory. [PDF]
Illarionov EA, Yukui W, Pevtsov AA.
europepmc +1 more source
Noise in Maps of the Sun at Radio Wavelengths II: Solar Use Cases. [PDF]
Bastian T +3 more
europepmc +1 more source
Polarimetric calibration of the Tunable Magnetograph for the Sunrise III mission
Campos-Jara A +9 more
europepmc +1 more source
Improving the Spectral Resolution and Wavelength Scale of SDO/EVE MEGS-A Flare Observations. [PDF]
Gonzalez G, Chamberlin P, Herde V.
europepmc +1 more source
Differential rotation: the chromosphere to the quiet chromosphere
ABSTRACT Synoptic maps of Ca II K-normalized intensity at ±40° latitude belt from Carrington rotations 827 (1915 August 10) to 1764 (1985 July 7) are utilized to investigate the long-term variation of the quiet chromospheric differential rotation within solar activity cycles through removing some large values of Ca II-normalized ...
J L Xie
exaly +2 more sources
The quiet-Sun photosphere and chromosphere [PDF]
Abstract The overall structure and the fine structure of the solar photosphere outside active regions are largely understood, except possibly the important roles of a turbulent near-surface dynamo at its bottom, internal gravity waves at its top and small-scale vorticity. Classical one-dimensional static radiation-escape modelling has
Robert J Rütten
exaly +4 more sources
Some of the next articles are maybe not open access.
Related searches:
Related searches:
Solar Physics, 1979
In this paper the dependance of the rotation rate of chromospheric features on their is discussed. The angular velocity of short lived emission features at chromospheric level has been determined by analyzing daily filtergrams in the Ca 11K3 line, obtained at the Anacapri Observatory, in the period 8 May-14August 1972.
Antonucci E. +4 more
openaire +3 more sources
In this paper the dependance of the rotation rate of chromospheric features on their is discussed. The angular velocity of short lived emission features at chromospheric level has been determined by analyzing daily filtergrams in the Ca 11K3 line, obtained at the Anacapri Observatory, in the period 8 May-14August 1972.
Antonucci E. +4 more
openaire +3 more sources

