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A Non-Linear Magnetic Field Calibration Method for Filter-Based Magnetographs by Multilayer Perceptron
DOI: 10.1007/s11207-019-1573-9 Bibcode: 2020SoPh..295....5G

Ji, Kaifan; Su, Jiangtao; Deng, Yuanyong +5 more

For filter-based magnetographs, the linear calibration method under the weak-field assumption is usually adopted; this leads to magnetic saturation effect in the regions with strong magnetic field. This article explores a new method to overcome the above disadvantage using a multilayer perceptron network, which we call MagMLP, based on a back-prop…

2020 Solar Physics
Hinode 8
CME Productive and Non-productive Recurring Jets Near an Active Region AR11176
DOI: 10.1007/s11207-020-1594-4 Bibcode: 2020SoPh..295...27S

Srivastava, Abhishek K.; Dwivedi, Bhola N.; Solanki, Ritika

We study the recurring jets near AR11176 during the period 2011 March 31 17:00 UT to April 1 05:00 UT using observations from the Atmospheric Imaging Assembly (AIA) on board Solar Dynamics Observatory (SDO). Mini-filaments (mini-filament1 & 2) are found at the base of these recurring jets where mini-filament1 shows the partial signature of eru…

2020 Solar Physics
Hinode SOHO 8
Locating Hot Plasma in Small Flares using Spectroscopic Overlappogram Data from the Hinode EUV Imaging Spectrometer
DOI: 10.1007/s11207-020-01602-6 Bibcode: 2020SoPh..295...34H

Reeves, Katharine K.; Lee, Kyoung-Sun; Hara, Hirohisa +6 more

One of the key processes associated with the "standard" flare model is chromospheric evaporation, a process during which plasma heated to high temperatures by energy deposition at the flare footpoints is driven upwards into the corona. Despite several decades of study, a number of open questions remain, including the relationship between plasma pr…

2020 Solar Physics
Hinode IRIS 6
Statistical Analysis of Asymmetric Sunspot Decay Observed by Hinode
DOI: 10.1007/s11207-020-01724-x Bibcode: 2020SoPh..295..154I

Imada, Shinsuke; Kato, Shota; Fujiyama, Masashi

We statistically studied the transport of magnetic flux in and around sunspots using a magnetic-element tracking technique to investigate whether sunspot-decay processes are isotropic. Using this method, we detected moving magnetic features (MMFs). The observed radius of an MMFs region was approximately 1.7 times the sunspot radius; furthermore, t…

2020 Solar Physics
Hinode 4
Magnetic Flux Emergence in a Coronal Hole
DOI: 10.1007/s11207-020-01629-9 Bibcode: 2020SoPh..295...64P

Denker, Carsten; Temmer, Manuela; Veronig, Astrid +13 more

A joint campaign of various space-borne and ground-based observatories, comprising the Japanese Hinode mission (Hinode Observing Plan 338, 20 - 30 September 2017), the GREGOR solar telescope, and the Vacuum Tower Telescope (VTT), investigated numerous targets such as pores, sunspots, and coronal holes. In this study, we focus on the coronal hole r…

2020 Solar Physics
Hinode 4
New Types of the Chromospheric Anemone Microflares: Case Study
DOI: 10.1007/s11207-020-01662-8 Bibcode: 2020SoPh..295...92D

Dumin, Yurii V.; Somov, Boris V.

Chromospheric anemone microflares (AMFs) are transient solar phenomena whose emission regions have a multi-ribbon configuration. As distinct from the so-called "atypical" solar flares, also possessing a few ribbons, the temporal and spatial scales of AMFs are a few times less, and the configuration of their ribbons is more specific (star-like). Th…

2020 Solar Physics
Hinode 1
Comparative Study of a Sunspot at Two Different Instances of Time
DOI: 10.1007/s11207-020-01627-x Bibcode: 2020SoPh..295...60H

Hamedivafa, Hashem

We investigate the evolutionary effects on the brightness of a sunspot as well as on the properties of its fine-structures using two sets of time series of G-band images of a single sunspot in NOAA 10944 recorded at two symmetric locations on the solar disc by Hinode/SOT (Solar Optical Telescope). The second time series (phase W) was recorded 2.5 …

2020 Solar Physics
Hinode 1