scholarly journals THE POSSIBILITY OF GENERALIZED PROTEST AND SOCIAL EXPLOSION IN THE YEARS OF MAXIMUM SOLAR ACTIVITY

2019 ◽  
Vol 1 (7) ◽  
pp. 170-177
Author(s):  
V. Souponitsky
Keyword(s):  
Solar Activity ◽  
Solar Cycle ◽  
The Creation ◽  
Ecological Industry ◽  
Social Management ◽  
Program Creation ◽  
Russian Program ◽  
Maximum Solar Activity ◽  
Protest Activity

The article has been devoted to the analysis and substantiation of the possibility of using the regularities of behavior of society and its individuals during the solar cycle, discovered by A. L. Chizhevsky, in the planning and implementation of social management. It has been proposed to exclude the negative development of events in our country during the 25th solar cycle to use the potential of the protest activity of society for the creation and development of the country, deploying the all-Russian program “Creation of modern ecological industry of Russia”, which requires the mobilization of efforts of the whole country and can create up to 10 million jobs for the youth.

scholarly journals Proton Fluxes Measured by the PAMELA Experiment from the Minimum to the Maximum Solar Activity for Solar Cycle 24

2018 ◽  
Vol 854 (1) ◽  
pp. L2 ◽  
Author(s):  
M. Martucci ◽  
R. Munini ◽  
M. Boezio ◽  
V. Di Felice ◽  
O. Adriani ◽  
...  
Keyword(s):  
Solar Activity ◽  
Solar Cycle ◽  
Pamela Experiment ◽  
Proton Fluxes ◽  
Solar Cycle 24 ◽  
Cycle 24 ◽  
Maximum Solar Activity

scholarly journals Forecast of solar maximum and minimum dates for solar cycles 23 to 29

1998 ◽  
Vol 41 (1) ◽  
Author(s):  
A. G. Elias ◽  
N. Ortiz de Adler
Keyword(s):  
Solar Activity ◽  
Solar Cycle ◽  
Multiple Regression ◽  
Cycle Length ◽  
Solar Cycles ◽  
Time Record ◽  
Two Phases ◽  
Solar Cycle Length ◽  
Off Time ◽  
Maximum Solar Activity

The solar cycle length for cycles 23 to 29 are forecasted. Two methods are analysed. In the first one, the solar cycle length is separated into its two phases í the rise time and the fall off time í and a multiple regression method is applied to each phase using lagged values as independent variables. In the second method, the multiple regression is fitted directly to the solar cycle length. The minimum and maximum solar activity dates are listed for the cycles predicted with the latter method which proves to be more accurate. Two lagged values appear in the multiple regression adjusted to the solar cycle length. One is associated with the Gleissberg period, also observed in the maximum sunspot number, and the other is coincident with one of the periodicities in the C14 time record, which is associated with solar activity variation

Prominences and Solar Activity

1979 ◽  
Vol 44 ◽  
pp. 357-372
Author(s):  
Z. Švestka
Keyword(s):  
Solar Activity ◽  
Solar Cycle ◽  
List Type ◽  
Type Number ◽  
Flare Loops ◽  
Filament Activation

The following subjects were discussed:(1)Filament activation(2)Post-flare loops.(3)Surges and sprays.(4)Coronal transients.(5)Disk vs. limb observations.(6)Solar cycle variations of prominence occurrence.(7)Active prominences patrol service.Of all these items, (1) and (2) were discussed in most detail and we also pay most attention to them in this report. Items (3) and (4) did not bring anything new when compared with the earlier invited presentations given by RUST and ZIRIN and therefore, we omit them.

The Heights of Solar Radio Sources at 1424 MHz and 696 MHz

1969 ◽  
Vol 1 (5) ◽  
pp. 192-194 ◽  
Author(s):  
D. G. Cole ◽  
R. F. Mullaly
Keyword(s):  
Solar Activity ◽  
High Resolution ◽  
Solar Disk ◽  
Previous Investigation ◽  
Solar Radio ◽  
Radio Sources ◽  
Grating Interferometer ◽  
Maximum Solar Activity

The heights of solar radio sources at 1424 MHz and 696 MHz have been measured during the years 1965 and 1966. Solar activity at this time was near minimum. The number of radio sources appearing on the solar disk rarely exceeded three at any time and it thus was possible to resolve the majority of these with a high resolution grating interferometer. Many of the previous height measurements at these frequencies have been made near times of maximum solar activity and the confusion of sources within the beam has limited their accuracy. The number of sources studied here is quite considerably higher than in any previous investigation at these frequencies, and the period of observation has been continuous.

scholarly journals On the Prediction of Solar Cycles

Solar Physics ◽  
2021 ◽  
Vol 296 (1) ◽  
Author(s):  
V. Courtillot ◽  
F. Lopes ◽  
J. L. Le Mouël
Keyword(s):  
Solar Activity ◽  
Solar Cycle ◽  
Transfer Function ◽  
Singular Spectrum Analysis ◽  
Activity Cycle ◽  
Solar Activity Cycle ◽  
Planetary Motion ◽  
Data Sets ◽  
Solar Cycles ◽  
Jovian Planets

AbstractThis article deals with the prediction of the upcoming solar activity cycle, Solar Cycle 25. We propose that astronomical ephemeris, specifically taken from the catalogs of aphelia of the four Jovian planets, could be drivers of variations in solar activity, represented by the series of sunspot numbers (SSN) from 1749 to 2020. We use singular spectrum analysis (SSA) to associate components with similar periods in the ephemeris and SSN. We determine the transfer function between the two data sets. We improve the match in successive steps: first with Jupiter only, then with the four Jovian planets and finally including commensurable periods of pairs and pairs of pairs of the Jovian planets (following Mörth and Schlamminger in Planetary Motion, Sunspots and Climate, Solar-Terrestrial Influences on Weather and Climate, 193, 1979). The transfer function can be applied to the ephemeris to predict future cycles. We test this with success using the “hindcast prediction” of Solar Cycles 21 to 24, using only data preceding these cycles, and by analyzing separately two 130 and 140 year-long halves of the original series. We conclude with a prediction of Solar Cycle 25 that can be compared to a dozen predictions by other authors: the maximum would occur in 2026.2 (± 1 yr) and reach an amplitude of 97.6 (± 7.8), similar to that of Solar Cycle 24, therefore sketching a new “Modern minimum”, following the Dalton and Gleissberg minima.

Length of the Solar Cycle: An Indicator of Solar Activity Closely Associated with Climate

Science ◽  
1991 ◽  
Vol 254 (5032) ◽  
pp. 698-700 ◽  
Author(s):  
E. FRIIS-CHRISTENSEN ◽  
K. LASSEN
Keyword(s):  
Solar Activity ◽  
Solar Cycle

scholarly journals North–south asymmetry of different solar activity features during solar cycle 23

New Astronomy ◽  
2010 ◽  
Vol 15 (6) ◽  
pp. 561-568 ◽  
Author(s):  
Neeraj Singh Bankoti ◽  
Navin Chandra Joshi ◽  
Seema Pande ◽  
Bimal Pande ◽  
Kavita Pandey
Keyword(s):  
Solar Activity ◽  
Solar Cycle ◽  
Solar Cycle 23 ◽  
South Asymmetry

scholarly journals Solar Cycle Signals in the Pacific and the Issue of Timings

2012 ◽  
Vol 69 (4) ◽  
pp. 1446-1451 ◽  
Author(s):  
Indrani Roy ◽  
Joanna D. Haigh
Keyword(s):  
Solar Activity ◽  
Solar Cycle ◽  
Aleutian Low ◽  
Positive Signal ◽  
Tropical Eastern Pacific ◽  
Sea Level Pressure ◽  
The Pacific ◽  
Strong Positive Signal ◽  
The Relationship ◽  
The Tropical Pacific

Abstract The solar cycle signal in sea level pressure during 1856–2007 is analyzed. Using composites of data from January–February in solar cycle peak years the strong positive signal in the region of the Aleutian low, found by previous authors, is confirmed. It is found, however, that signals in other regions of the globe, particularly in the South Pacific, are very sensitive to the choice of reference climatology. Also investigated is the relationship between solar activity and sea surface temperatures in the tropical eastern Pacific. A marked overall association of higher solar activity with colder temperatures in the tropical Pacific that is not restricted to years of peak sunspot number is noted. The ENSO-like variation following peak years that has been suggested by other authors is not found as a consistent signal. Both the SLP and SST signals vary coherently with the solar cycle and neither evolves on an ENSO-like time scale. The solar signals are weaker during the period spanning approximately 1956–97, which may be due to masking by a stronger innate ENSO variability at that time.

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