Results 91 to 100 of about 630 (149)

Microwave Bright Points with Multiple Periodic Oscillations in the Solar Polar Coronal Hole during Solar Cycle Minimum

open access: yesThe Astrophysical Journal
During solar cycle minimum, polar coronal holes show a prominent radio brightening cap. The analysis of polar microwave enhanced radiation in polar coronal holes is helpful for understanding the magnetic field characteristics and the origin of the solar ...
Jing Huang   +6 more
doaj   +1 more source

Giant Postflare Loops in Active Regions with an Extremely Strong Coronal Magnetic Field

open access: yesThe Astrophysical Journal
We report for the first time the detection of thermal free–free emission from post-flare loops at 34 GHz in images from the Nobeyama Radioheliograph. We studied eight loops, seven of which were from regions with an extremely strong coronal magnetic field
Costas E. Alissandrakis   +4 more
doaj   +1 more source

The Diagnostic Temperature Discrepancy as Evidence for Non-Maxwellian Coronal Electrons

open access: yesThe Open Journal of Astrophysics
Two independent electron temperature diagnostics applied to the quiet solar corona yield systematically different results. Radio brightness temperatures from the Nançay Radioheliograph indicate Tₑ ≈ 0.6 MK, while hydrostatic scale-height modeling of the ...
Victor Edmonds
doaj   +1 more source

Restoration of solar images by the Steer algorithm

open access: yes, 2003
Restoration of diffuse features and computational time have been more serious problems in solar observations than in non-solar observations because of complicated brightness structures in enormous time-series images.
H. Koshiishi
core   +1 more source

Long-term Solar Activity Studies using Microwave Imaging Observations and Prediction for Cycle 25. [PDF]

open access: yesJ Atmos Sol Terr Phys, 2018
Gopalswamy N   +3 more
europepmc   +1 more source

The behavior of the spotless active regions during the solar minimum 23-24

open access: yes, 2016
In this work, we analysed the physical parameters of the spotless actives regions observed during solar minimum 23 – 24 (2007 – 2010). The study was based on radio maps at 17 GHz obtained by the Nobeyama Radioheliograph (NoRH) and magnetograms provided ...
Caius Lucius Selhorst   +1 more
core   +1 more source

Lambda 8-CM Solar Maps Observed with the RSIP, A Real-Time Multi-Channel Digital Correlator Backend Installed to the Radioheliograph at Toyokawa [PDF]

open access: yes
1987-03-25The lambda 8-cm radioheliograph at Toyokawa has been improved with respect to sensitivity and time resolution by the introduction of a new real-time digital correlator backend, which is called RSIP (Real-Time Solar Image Processor ...
ENOME, Shinzo   +5 more
core  

Loss-cone instability modulation due to a magnetohydrodynamic sausage mode oscillation in the solar corona. [PDF]

open access: yesNat Commun, 2019
Carley EP   +6 more
europepmc   +1 more source

Automatic detection of limb prominences in 304 Å EUV images [PDF]

open access: yes, 2010
A new algorithm for automatic detection of prominences on the solar limb in 304 Å EUV images is presented, and results of its application to SOHO/EIT data discussed.
Labrosse, N., Dalla, S., Marshall, S.
core  

On-Disc Observations of Flux Rope Formation Prior to Its Eruption. [PDF]

open access: yesSol Phys, 2017
James AW   +8 more
europepmc   +1 more source

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