Results 41 to 50 of about 541,779 (282)

Solar-Cycle Characteristics Examined in Separate Hemispheres: Phase, Gnevyshev Gap, and Length of Minimum [PDF]

open access: yes, 2009
Research results from solar-dynamo models show the northern and southern hemispheres may evolve separately throughout the solar cycle. The observed phase lag between the hemispheres provides information regarding the strength of hemispheric coupling ...
A. A. Norton   +25 more
core   +1 more source

Solar wind parameters in rising phase of solar cycle 25: Similarities and differences with solar cycles 23 and 24

open access: yesSolar-Terrestrial Physics, 2023
Solar activity and solar wind parameters decreased significantly in solar cycles (SCs) 23–24. In this paper, we analyze solar wind measurements at the rising phase of SC 25 and compare them with similar data from the previous cycles. For this purpose, we
Yermolaev Y. I.   +8 more
doaj   +1 more source

Deciphering Solar Magnetic Activity: The Solar Cycle Clock

open access: yesFrontiers in Astronomy and Space Sciences, 2022
The Sun’s variability is controlled by the progression and interaction of the magnetized systems that form the 22-year magnetic activity cycle (the “Hale Cycle”) as they march from their origin at ∼55° latitude to the equator, over ∼19 years. We will discuss the end point of that progression, dubbed “terminator” events, and our means of diagnosing them.
Robert J. Leamon   +3 more
openaire   +3 more sources

Precursors of an upcoming solar cycle at high latitudes from coronal green line data [PDF]

open access: yes, 2018
After reviewing potential early indicators of an upcoming solar cycle at high latitudes, we focus attention on the rush-to-the-poles (RTTP) phenomenon in coronal green line emission.
Gerják, T.   +3 more
core   +2 more sources

MnI‐Functionalized Covalent Organic Framework as Efficient Electrocatalyst for CO2 Reduction in a Catholyte‐Free Zero‐Gap Electrolyzer

open access: yesAdvanced Functional Materials, EarlyView.
This work demonstrates the successful integration of a phenanthroline‐based 2D COF with MnI catalytic sites into a catholyte‐free membrane‐electrode‐assembly cell for CO2 electroreduction. The crystalline COF actively suppresses Mn⁰–Mn⁰ dimerization, achieving a turnover frequency of 617 h⁻¹ at 2.8 V (full‐cell potential), and enabling stable operation.
Laura Spies   +8 more
wiley   +1 more source

Solar-cycle-related variation of solar differential rotation [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2013
19 pages, 8 figures, accepted by MNRAS.
Li, K. J.   +6 more
openaire   +2 more sources

Photometric Trends in the Visible Solar Continuum and Their Sensitivity to the Center-to-Limb Profile [PDF]

open access: yes, 2015
Solar irradiance variations over solar rotational time-scales are largely determined by the passage of magnetic structures across the visible solar disk.
Peck, Courtney, Rast, Mark
core   +5 more sources

Demonstration of an All‐Optical AND Gate Mediated by Photochromic Molecules

open access: yesAdvanced Functional Materials, EarlyView.
A logic AND gate that runs on photons is demonstrated. It relies on two spatially separated photochromic molecules that work in tandem. Abstract The realization of a photonic logic AND gate, i.e. a logic AND gate that runs on photons rather than electrons, and where all steps are controlled by light, is demonstrated. In a proof‐of‐principle experiment,
Heyou Zhang   +7 more
wiley   +1 more source

Solar Cycle Modulation of Nighttime Ozone Near the Mesopause as Observed by MLS

open access: yesEarth and Space Science, 2020
Eleven‐year solar cycle variations of nighttime ozone near the secondary ozone maximum layer in the mesosphere are analyzed with Aura Microwave Limb Sounder (MLS) observations since 2004, fully covering solar cycle 24.
Jae N. Lee, Dong L. Wu
doaj   +1 more source

Correlation between Supergranular Lane Widths and Sunspot Number; A Simple Way to Predict the Amplitude of Sunspot Cycle

open access: yesThe Astrophysical Journal Letters, 2023
The network structure seen in the solar images is the outline of supergranulation, which is the large-scale convection in the Sun with a size of about 30 Mm and a lifetime of 24 hr.
K P Raju   +3 more
doaj   +1 more source

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