scholarly journals Influence of Forbush Effect on Atmospheric Ionization due to Solar Energtic Particles

2021 ◽  
Author(s):  
Peter I.V. Velinov ◽  
Alexander Mishev
Keyword(s):  
Atmospheric Ionization ◽  
Forbush Effect

scholarly journals Excitation And Ionization By Auroral Protons

1966 ◽  
Vol 19 (3) ◽  
pp. 309 ◽  
Keyword(s):  
Magnetic Field ◽  
Energy Range ◽  
Pitch Angle ◽  
Proton Energy ◽  
Ionization Rate ◽  
Energy Spectra ◽  
Proton Fluxes ◽  
Atmospheric Ionization ◽  
The Magnetic Field

Height distributions are presented for the atmospheric ionization rate and Balmer radiation resulting from precipitation of auroral protons. These results have been computed assuming proton fluxes with several different energy spectra and pitch-angle distributions about the magnetic field, the total proton energy range being restricted to 1-1000 keY.

scholarly journals Atmospheric ionization and cloud radiative forcing

2021 ◽  
Vol 11 (1) ◽  
Author(s):  
Henrik Svensmark ◽  
Jacob Svensmark ◽  
Martin Bødker Enghoff ◽  
Nir J. Shaviv
Keyword(s):  
Radiative Forcing ◽  
Cloud Condensation Nuclei ◽  
Short Wave ◽  
Satellite Observations ◽  
Cloud Formation ◽  
Wave Radiation ◽  
Substantial Impact ◽  
Radiative Balance ◽  
Cloud Radiative Forcing ◽  
Atmospheric Ionization

AbstractAtmospheric ionization produced by cosmic rays has been suspected to influence aerosols and clouds, but its actual importance has been questioned. If changes in atmospheric ionization have a substantial impact on clouds, one would expect to observe significant responses in Earth’s energy budget. Here it is shown that the average of the five strongest week-long decreases in atmospheric ionization coincides with changes in the average net radiative balance of 1.7 W/m$$^2$$ 2 (median value: 1.2 W/m$$^2$$ 2 ) using CERES satellite observations. Simultaneous satellite observations of clouds show that these variations are mainly caused by changes in the short-wave radiation of low liquid clouds along with small changes in the long-wave radiation, and are almost exclusively located over the pristine areas of the oceans. These observed radiation and cloud changes are consistent with a link in which atmospheric ionization modulates aerosol's formation and growth, which survive to cloud condensation nuclei and ultimately affect cloud formation and thereby temporarily the radiative balance of Earth.

scholarly journals Terrestrial effects of moderately nearby supernovae

2017 ◽  
Author(s):  
Adrian L. Melott ◽  
Brian C. Thomas
Keyword(s):  
Cosmic Rays ◽  
Ozone Depletion ◽  
Short Communication ◽  
Early Pleistocene ◽  
Mutation Rates ◽  
Benthic Organisms ◽  
Concomitant Increase ◽  
The Earth ◽  
New Information ◽  
Atmospheric Ionization

AbstractRecent data indicate one or more moderately nearby supernovae in the early Pleistocene, with additional events likely in the Miocene. This has motivated more detailed computations, using new information about the nature of supernovae and the distances of these events to describe in more detail the sorts of effects that are indicated at the Earth. This short communication/review is designed to describe some of these effects so that they may possibly be related to changes in the biota around these times.SummaryIt has been known for some time that moderately nearby supernovae may have substantial effects on the Earth. Events at ˜150 light years will happen on average every few Myr, but will tend to happen in groups, with long periods between with no events. The effects of cosmic rays from such events appears to be greater than estimated previously. Ozone depletion and the increase of hazardous UVB continues to be important, but new effects come to the fore. Muon irradiation on the ground and hundreds of meters down into the ocean will increase cancer and mutation rates, the differences being most notable in terrestrial megafauna and benthic organisms. Typically larger organisms live long enough to develop cancer; in microorganisms the primary effects would be associated with mutation rates. Atmospheric ionization in the troposphere will greatly increase lightning rates, with a concomitant increase in the rate of wildfires.

The Atmospheric Ionization during Substorm Model

2021 ◽  
Author(s):  
Olesya Yakovchuk ◽  
Jan Maik Wissing
Keyword(s):  
High Resolution ◽  
Particle Flux ◽  
Coordinate Systems ◽  
Single Particles ◽  
Polar Cap ◽  
Output Data ◽  
Loss Cone ◽  
Data Format ◽  
Time Period ◽  
Atmospheric Ionization

<p>The Atmospheric Ionization during Substorm Model (AISstorm) is the successor of the Atmospheric Ionization Module Osnabrück (AIMOS) and thus may also be considered as AIMOS 2.0 - AISStorm.</p><p>The overall structure was kept mostly unaltered and splits up into an empirical model that determines the 2D precipitating particle flux and a numerical model that determines the ionization profile of single particles. The combination of these two results in a high resolution 3D particle ionization pattern.</p><p>The internal structure of the model has been completely revised with the main aspects being: a) an internal magnetic coordinate system, b) including substorms characteristics, c) higher time resolution, d) higher spatial resolution, e) energy specific separate handling of drift loss cone, auroal precipitation and polar cap precipitation, partly even in separate coordinate systems, f) better MLT resolution and g) covering a longer time period. All these tasks have been matched while keeping the output data format identical, allowing easy transition to the new version.</p>

THE IONIZATION OF THE ATMOSPHERE MEASURED FROM FLYING AIRCRAFT

1931 ◽  
Vol 5 (6) ◽  
pp. 625-635
Author(s):  
D. C. Rose
Keyword(s):  
Relative Humidity ◽  
Negative Ions ◽  
Ground Level ◽  
The State ◽  
Dust Particles ◽  
Measuring Apparatus ◽  
Positive Ions ◽  
Humidity Measurements ◽  
Water Drops ◽  
Atmospheric Ionization

The Gerdian type of atmospheric ionization measuring apparatus was attached to a cabin aeroplane so that the state of ionization of the atmosphere could be studied. The limitations of the apparatus for aeroplane use are discussed. Measurements were taken from ground level to heights of 15000 ft. The results are plotted in number of ions per cc. (separate curves for positive and negative) at different altitudes.The results indicate that at the cloud level there is an abnormal excess of small positive ions and a minimum in the excess of positive ions over negative ions from 4000–6000 ft. higher. This does not include large ions such as charged water drops or dust particles. The observations were taken in regions free from clouds, the cloud level being determined by observation on clouds in the sky, and by relative humidity measurements taken at the same time.

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