• No results found

Solar intensity measured during the 2004 experiments

New solar modulation modeling of the galactic proton flux measured by the AMS02 and PAMELA experiments

New solar modulation modeling of the galactic proton flux measured by the AMS02 and PAMELA experiments

... of solar e ff ects on the galactic cosmic rays is rel- evant both to infer the local interstellar spectrum characteristics and to investigate the dynamics of charged particles in the ...AMS02 experiments, ...

5

Solar flare effects observed over Jicamarca during MST-ISR experiments

Solar flare effects observed over Jicamarca during MST-ISR experiments

... radiation intensity at frequencies rang- ing from radiowaves to X-rays followed by energetic charged particles generated during a typical solar flare as a function of ...radiation during ...

92

Five solar neutrino experiments

Five solar neutrino experiments

... in solar neutrino experiments and be used as input for detailed analyses of the particle physics implications of the measured solar neutrino ...be measured more accurately in laboratory ...

8

Topside equatorial zonal ion velocities measured by C/NOFS during rising solar activity

Topside equatorial zonal ion velocities measured by C/NOFS during rising solar activity

... spacecraft during the 2009–2012 time interval, a period of very low to moderate solar activity as determined from ...moderate solar ac- tivity in the 280 ◦ longitude region are organized into a diur- ...

7

Solar Energetic Particles measured by AMS-02

Solar Energetic Particles measured by AMS-02

... MeV/nucleon Solar Energetic Particles (SEPs) are a key target of Heliophysics research, not only as exem- plars of particle acceleration and transport processes that are ubiquitous in astrophysical plasmas, but ...

8

A potential lag between the open solar magnetic source flux and solar EUV and X-ray emissions as measured by the Earth’s ionosphere during total solar eclipses

A potential lag between the open solar magnetic source flux and solar EUV and X-ray emissions as measured by the Earth’s ionosphere during total solar eclipses

... ionisation during an eclipse and com- paring these measurements with an estimate of the unper- turbed ionisation levels (such as those made during a control day, where available) it is possible to estimate ...

8

Variation of the 0+ ion density during low and high solar activity as measured by the SR0SS-C2 satellite

Variation of the 0+ ion density during low and high solar activity as measured by the SR0SS-C2 satellite

... for solar low and high activity ...value during daytime in solar maxima as well as solar ...With solar phase change from minima to maxima, there is a nine times enhancement of the ...

11

A comparison of optically measured daytime OH temperatures over the tropics during solar maximum and minimum periods

A comparison of optically measured daytime OH temperatures over the tropics during solar maximum and minimum periods

... observed during two different so- lar activity epochs from equatorial ...years during the months of ...flux during these periods are indicative of the dominance of dynamical forc- ings on direct ...

7

The Radioactivity of Nuclei & Solar Oscillations: New Experiments

The Radioactivity of Nuclei & Solar Oscillations: New Experiments

... [3], then, when synchronously recording the variations in the intensity of radio activity of the cesium and ura- nium decay products, we should obtain a time shift in the registration of the neutrino outbursts. We ...

13

Upper-mesospheric temperatures measured during intense substorms in the declining phase of the January 2005 solar proton events

Upper-mesospheric temperatures measured during intense substorms in the declining phase of the January 2005 solar proton events

... Considering the size of the calculated heating rate we find it likely to be no immediate significant temperature effects of the particle precipitation in the upper mesosphere above Andøya on the 21–22 January 2005. If ...

15

Night-time F-region and daytime E-region ionospheric drifts measured at Udaipur during solar flares

Night-time F-region and daytime E-region ionospheric drifts measured at Udaipur during solar flares

... Pr¨olss (1982) has discussed mechanisms that can cause heat- ing in the low-latitudes and a change in the wind pattern; these are ring current neutral particle injection, large-scale circulation and travelling ...

6

The Geomagnetic Effects of Solar Activity as Measured at Ouagadougou Station

The Geomagnetic Effects of Solar Activity as Measured at Ouagadougou Station

... the solar maximum ...action during the solar maximum ...that during the solar maximum phase, the reversal electric field occurs early for the one-day-shock activity and later for the ...

13

Quality assessment of solar UV irradiance measured with array spectroradiometers

Quality assessment of solar UV irradiance measured with array spectroradiometers

... spectroradiometer during the operation time, a portable irradiance calibrator is ...times during the intercomparison with three different 250 W tungsten halogen ...stable during the ...

15

Comparison of modelled and measured tilted solar irradiance for photovoltaic applications

Comparison of modelled and measured tilted solar irradiance for photovoltaic applications

... irradiances measured by the pyranometer and the silicon sensors at both sites in ...the measured signal is low and are slightly lower with increasing irradiance in the summer ...values during the ...

18

Simulations of solar radiative transfer in measured and generated cloud fields

Simulations of solar radiative transfer in measured and generated cloud fields

... An enhancement of T can be noticed at the pixels where the extra photons reected at cloud edges end up. R-elds show high intensity pixels where the direct light comes re- ected from dense cumulus nucleus. ...

13

Total Solar Flux Intensity at 11 2 GHz as an Indicator of Solar Activity and Cyclicity

Total Solar Flux Intensity at 11 2 GHz as an Indicator of Solar Activity and Cyclicity

... of solar radio observations at ...observed during the solar cycles 23 and 24 (2001-2013) both in solar maxima and ...180 solar radio bursts, with varying intensities and prop- erties, ...

9

Sensitivity of the intensity frontier experiments for neutrino and scalar portals: Analytic estimates.

Sensitivity of the intensity frontier experiments for neutrino and scalar portals: Analytic estimates.

... Uncertainties. According to the theoretical predictions the dσ/dp T distribution of B mesons at the LHC has a maximum at p T ∼ GeV, see figure 4. The region of low p T is complicated for the theoretical predictions ...

42

Equatorial vertical plasma drifts and the measured and IRI model predicted F2 layer parameters above Ouagadougou during solar minimum

Equatorial vertical plasma drifts and the measured and IRI model predicted F2 layer parameters above Ouagadougou during solar minimum

... present during the daytime that will favor the daytime higher val- ues of h m F 2 and enhanced f o F 2 (or N m F 2 ) at low solar ...by solar UV radiation ...

17

Long term changes in EUV and X-ray emissions from the solar corona and chromosphere as measured by the response of the Earth’s ionosphere during total solar eclipses from 1932 to 1999

Long term changes in EUV and X-ray emissions from the solar corona and chromosphere as measured by the response of the Earth’s ionosphere during total solar eclipses from 1932 to 1999

... frequency. During the eclipse, however, the ionosphere was changing faster than the operators could change frequency, resulting in a series of measurements con- taining few critical frequency values, and many ...

11

Show all 10000 documents...

Related subjects