E-Print Archive

There are 4618 abstracts currently viewable.


Search:

Advanced Search
Options
Main Page Add New E-Print Submitter
Information
Feedback
News Help/FAQ About Preferences
Manage Key Phrase
Notification
Terrestrial temperature, sea levels and ice area links with solar activity and solar orbital motion View all abstracts by submitter

Valentina Zharkova   Submitted: 2023-11-11 07:31

This paper explores the links between terrestrial temperature, sea levels and ice areas in both hemispheres with solar activity in- dices expressed through averaged sunspot numbers together with the summary curve of eigen vectors of the solar background magnetic field (SBMF) and with changes of Sun-Earth distances caused by solar inertial motion resulting from the gravitation of large planets in the solar system. Using the wavelet analy- sis of the GLB and HadCRUTS datasets two periods: 21.4 and 36 years in GLB, set and the period of about 19.6 years in the HadCRUTS are discovered. The 21.4 year period is as- sociated with variations in solar activity defined by the sum- mary curve of the largest eigen vectors of the SBMF. A dom- inant 21.4-year period is also reported in the variations of the sea level, which is linked with the period of 21.4 years de- tected in the GLB temperature and the summary curve of the SBMF variations. The wavelet analysis of ice and snow ar- eas shows that in the Southern hemisphere it does not show any links to solar activity periods while in the Northern hemi- sphere the ice area reveals a period of 10.7 years equal to a usual solar acitviity cycle. The TSI in March-August of every year is found to grow with every year following closely the tem- perature curve, because the Sun moves closer to the Earth or- bit owing to gravitation of large planets. (solar inertial mo- tion, SIM). While the variations of solar radiation during a whole year have more steady distribution without a sharp TSI in- crease during the last two centuries. The additional TSI con- tribution caused by SIM is likely to secure the additional energy input and exchange between the ocean and atmosphere.

Authors: V.Zharkova and I. Vasilieva
Projects: Other

Publication Status: in press
Last Modified: 2023-11-11 13:29
Go to main E-Print page  Phase mixed Alfven waves in partially ionised solar plasmas  A model of failed solar eruption initiated and destructed by magnetic reconnection  Edit Entry  Download Preprint  Submitter's Homepage Delete Entry 

Key
Go to main E-Print pageGo to main E-Print page.
Previous AbstractPrevious Abstract.
Next AbstractNext Abstract.
Download PreprintDownload Preprint.
Submitter's HomepageSubmitters Homepage.
Edit EntryEdit Entry.
View All Abstracts By SubmitterView all abstracts by submitter.
Delete AbstractDelete abstract.

Latest Entries
Formation and Dynamics in an Observed Preeruptive Filament
Unveiling the spectacular over 24-hour flare of star CD-36 3202
The centroid speed as a characteristic of the group speed of solar coronal fast magnetoacoustic wave trains
Coronal dimmings as indicators of early CME propagation direction
A Chromatic Treatment of Linear Polarization in the Solar Corona at the 2023 Total Solar Eclipse
MinXSS-2 CubeSat mission overview: Improvements from the successful MinXSS-1 mission
Small Satellite Mission Concepts for Space Weather Research and as Pathfinders for Operations
Study of Time Evolution of Thermal and Nonthermal Emission from an M-class Solar Flare
Achievements and Lessons Learned From Successful Small Satellite Missions for Space Weather-Oriented Research
Scaling of Electron Heating by Magnetization During Reconnection and Applications to Dipolarization Fronts and Super-Hot Solar Flares
Defining the Middle Corona
First Results for Solar Soft X-Ray Irradiance Measurements from the Third-generation Miniature X-Ray Solar Spectrometer
Deciphering the solar coronal heating: Energizing small-scale loops through surface convection
Using Potential Field Extrapolations to Explore the Origin of Type II Spicules
Phase mixed Alfvén waves in partially ionised solar plasmas
Terrestrial temperature, sea levels and ice area links with solar activity and solar orbital motion
A model of failed solar eruption initiated and destructed by magnetic reconnection
Energetics of a solar flare and a coronal mass ejection generated by a hot channel eruption
An Optically Thin View of the Flaring Chromosphere: Nonthermal widths in a chromospheric condensation during an X-class solar flare
A Database of Magnetic and Thermodynamic Properties of Confined And Eruptive Solar Flares

Related Pages
MSU Solar Physics.
Max Millennium Science Mail Archive.
Max Millennium Message of the Day Mail Archive.
Max Millennium Flare Catalog

Archive Maintainer
Alisdair Davey



© 2000-2020 Solar Physics Group - Montana State University