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Fast Solar Image Classification Using Deep Learning and Its Importance for Automation in Solar Physics
DOI: 10.1007/s11207-019-1473-z Bibcode: 2019SoPh..294...80A

Fletcher, Lyndsay; Armstrong, John A.

The volume of data being collected in solar physics has exponentially increased over the past decade and with the introduction of the Daniel K. Inouye Solar Telescope (DKIST) we will be entering the age of petabyte solar data. Automated feature detection will be an invaluable tool for post-processing of solar images to create catalogues of data re…

2019 Solar Physics
Hinode 29
Modeling of the Sunspot-Associated Microwave Emission Using a New Method of DEM Inversion
DOI: 10.1007/s11207-019-1406-x Bibcode: 2019SoPh..294...23A

Patsourakos, S.; Alissandrakis, C. E.; Bogod, V. M. +2 more

We develope a method to compute the temperature and density structure along the line of sight by inversion of the differential emission measure (DEM), under the assumptions of stratification and hydrostatic equilibrium. We apply this method to the DEM obtained from the Atmospheric Imaging Assembly (AIA) observations and use the results, together w…

2019 Solar Physics
Hinode 14
Analysis of Quiescent Corona X-ray Spectra from SphinX During the 2009 Solar Minimum
DOI: 10.1007/s11207-019-1565-9 Bibcode: 2019SoPh..294..176S

Phillips, K. J. H.; Sylwester, B.; Sylwester, J. +3 more

The SphinX X-ray spectrophotometer on the CORONAS-PHOTON mission observed the 1 - 15 keV X-ray spectrum of the spatially integrated solar corona during the deep minimum of 2009, when solar activity was exceptionally low. Its sensitivity for energies >1.2 keV was higher than that of any other solar X-ray spectrometer in orbit at the time, includ…

2019 Solar Physics
Hinode 7
Comprehensive Determination of the Hinode/EIS Roll Angle
DOI: 10.1007/s11207-019-1451-5 Bibcode: 2019SoPh..294...59P

Warren, Harry P.; Brooks, David H.; Baker, Deborah +5 more

We present a new coalignment method for the EUV Imaging Spectrometer (EIS) on board the Hinode spacecraft. In addition to the pointing offset and spacecraft jitter, this method determines the roll angle of the instrument, which has never been systematically measured, and which is therefore usually not corrected. The optimal pointing for EIS is com…

2019 Solar Physics
Hinode 4
Association of Calcium Network Bright Points with Underneath Photospheric Magnetic Patches
DOI: 10.1007/s11207-019-1419-5 Bibcode: 2019SoPh..294...40N

Pant, Vaibhav; Banerjee, Dipankar; Narang, Nancy +1 more

Recent dedicated Hinode polar region campaigns revealed the presence of concentrated kilogauss patches of the magnetic field in the polar regions of the Sun, which are also shown to be correlated with facular bright points at the photospheric level. In this work, we demonstrate that this spatial intermittency of the magnetic field persists even up…

2019 Solar Physics
Hinode 4
Velocity Structure and Temperature Dependence of an Extreme-Ultraviolet Jet Observed by Hinode
DOI: 10.1007/s11207-019-1469-8 Bibcode: 2019SoPh..294...74K

Imada, S.; Kawai, T.; Kanda, N.

The acceleration mechanism of EUV and X-ray jets is still unclear. In general, there are two candidates for the mechanism. One is magnetic reconnection, and the other is chromospheric evaporation. We observed a relatively compact X-ray jet that occurred between 10:50 - 11:10 UT on 18 February 2011 by using the Solar Dynamics Observatory/Atmospheri…

2019 Solar Physics
Hinode 1