On the basis of the analysis of the data of auroral observations at middle latitudes during low solar activity, and modern spectrophotometric research, the feasibility of their joint use for the estimation of the level of the solar activity during periods without instrumental measurements is discussed. In this paper an attempt is undertaken to determine quantitative information on solar activity by comparing the data of visual auroral observations with the modern parameter of their luminescence
Abstract. In 1957-59 within the framework of the International Geophysical Year (IGY) (the period of...
As our civilization depends increasingly on space-borne assets and on a delicate and vulnerable eart...
The intensity of a specrtal line from an optically thin plasma such as the outer atmosphere of the S...
International audienceOn the basis of the analysis of the data of auroral observations at middle lat...
International audienceIn this short contribution the use of different sunspot numbers for the estima...
Estimation of past solar and upper atmosphere conditions from historical and modern auroral observat...
It is shown that such data that exist on auroral activity in the period between 1450 and 1550 do no...
Abstract. Knowledge of solar variability and its effects on the Earth is essential since the Sun aff...
Recent research on the scientific interpretation of historical auroral records is summarised, with s...
The extension of sunspot number series and auroral observations backward in time is of considerable ...
A prominent manifestation of the solar dynamo is the 11-year activity cycle, evident in indicators o...
Based on a quantitative study of the common fluctuations of 14C and 10Be production rates, we have d...
The auroral radiation, 3914 AO, received from the entire sky on a horizontal diffusing plate was mo...
Both auroral and geomagnetic activity provide information from which the behavior of the magnet-osph...
This report presents data and analysis of visual, photographic and auroral spectral data, obtained ...
Abstract. In 1957-59 within the framework of the International Geophysical Year (IGY) (the period of...
As our civilization depends increasingly on space-borne assets and on a delicate and vulnerable eart...
The intensity of a specrtal line from an optically thin plasma such as the outer atmosphere of the S...
International audienceOn the basis of the analysis of the data of auroral observations at middle lat...
International audienceIn this short contribution the use of different sunspot numbers for the estima...
Estimation of past solar and upper atmosphere conditions from historical and modern auroral observat...
It is shown that such data that exist on auroral activity in the period between 1450 and 1550 do no...
Abstract. Knowledge of solar variability and its effects on the Earth is essential since the Sun aff...
Recent research on the scientific interpretation of historical auroral records is summarised, with s...
The extension of sunspot number series and auroral observations backward in time is of considerable ...
A prominent manifestation of the solar dynamo is the 11-year activity cycle, evident in indicators o...
Based on a quantitative study of the common fluctuations of 14C and 10Be production rates, we have d...
The auroral radiation, 3914 AO, received from the entire sky on a horizontal diffusing plate was mo...
Both auroral and geomagnetic activity provide information from which the behavior of the magnet-osph...
This report presents data and analysis of visual, photographic and auroral spectral data, obtained ...
Abstract. In 1957-59 within the framework of the International Geophysical Year (IGY) (the period of...
As our civilization depends increasingly on space-borne assets and on a delicate and vulnerable eart...
The intensity of a specrtal line from an optically thin plasma such as the outer atmosphere of the S...